Welcome to Jupiter – NASA’s Juno Achieves Orbit around ‘King of the Planets’

Illustration of NASA's Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter. Lockheed Martin built the Juno spacecraft for NASA's Jet Propulsion Laboratory. Credit: NASA/Lockheed Martin
Illustration of NASA's Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter. Lockheed Martin built the Juno spacecraft for NASA's Jet Propulsion Laboratory.
Illustration of NASA’s Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter. Lockheed Martin built the Juno spacecraft for NASA’s Jet Propulsion Laboratory. Credit: NASA/Lockheed Martin

Welcome to Jupiter! NASA’s Juno spacecraft is orbiting Jupiter at this moment!

“NASA did it again!” pronounced an elated Scott Bolton, investigator of Juno from Southwest Research Institute in San Antonio, to loud cheers and applause from the overflow crowd of mission scientists and media gathered at the post orbit media briefing at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif.

After a nearly five year journey covering 1.7-billion-miles (2.8-billion-kilometers) across our solar system, NASA’s basketball court-sized Juno orbiter achieved orbit around Jupiter, the ‘King of the Planets’ late Monday night, July 4, in a gift to all Americans on our 240th Independence Day and a gift to science to elucidate our origins.

“We are in orbit and now the fun begins, the science,” said Bolton at the briefing. “We just did the hardest thing NASA’s ever done! That’s my claim. I am so happy … and proud of this team.”

And the science is all about peering far beneath the well known banded cloud tops for the first time to investigate Jupiter’s deep interior with a suite of nine instruments, and discover the mysteries of its genesis and evolution and the implications for how we came to be.

“The deep interior of Jupiter is nearly unknown. That’s what we are trying to learn about. The origin of us.”

Solar powered Juno successfully entered a polar elliptical orbit around Jupiter after completing a must-do 35-minute-long firing of the main engine known as Jupiter Orbital Insertion or JOI.

The spacecraft approached Jupiter over its north pole, affording an unprecedented perspective on the Jovian system – “which looks like a mini solar system” – as it flew through the giant planets intense radiation belts in ‘autopilot’ mode.

“The mission team did great. The spacecraft did great. We are looking great. It’s a great day,” Bolton gushes.

Engineers tracking the telemetry received confirmation that the JOI burn was completed as planned at 8:53 p.m. PDT (11:53 p.m. EDT) Monday, July 4.

Juno is only the second probe from Earth to orbit Jupiter and the first solar powered probe to the outer planets. The gas giant is two and a half times more massive than all of the other planets combined.

“Independence Day always is something to celebrate, but today we can add to America’s birthday another reason to cheer — Juno is at Jupiter,” said NASA administrator Charlie Bolden in a statement.

“And what is more American than a NASA mission going boldly where no spacecraft has gone before? With Juno, we will investigate the unknowns of Jupiter’s massive radiation belts to delve deep into not only the planet’s interior, but into how Jupiter was born and how our entire solar system evolved.”

Artists concept NASA's Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter on July 4, 2016 nearly five years after launch.   Credit: NASA
Artists concept NASA’s Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter on July 4, 2016 nearly five years after launch. Credit: NASA

The do-or-die burn of Juno’s 645-Newton Leros-1b main engine started at 8:18 p.m. PDT (11:18 p.m. EDT), which had the effect of decreasing the spacecraft’s velocity by 1,212 miles per hour (542 meters per second) and allowing Juno to be captured in orbit around Jupiter. There were no second chances.

All of the science instruments were turned off on June 30 to keep the focus on the nail-biting insertion maneuver and preserve battery power, said Bolton.

“So tonight through tones Juno sang to us. And it was a song of perfection. After a 1.7 billion mile journey we hit tour burn targets within one second,” Rick Nybakken, Juno project manager from JPL, gleefully reported at the briefing.

“That’s how good our team is! And that’s how well our Juno spacecraft performed tonight.”

To accomplish the burn, the spacecraft first had to adjust it’s attitude to point the engine in the required direction to slow the spacecraft and then simultaneously also had the effect that the life giving solar panels were pointing away from the sun. It the only time during the entire mission at Jupiter that the solar panels were in darkness and not producing energy.

The spacecraft’s rotation rate was also spun up from 2 to 5 revolutions per minute (RPM) to help stabilize it during JOI. Juno is spin stabilized to maintain pointing.

After the burn was complete, Juno was spun down and adjusted to point to the sun before it ran out of battery power.

We have to get the blood flowing through Juno’s veins, Bolton emphasized.

It is equipped with 18,698 individual solar cells over 60 square meters of surface on the solar arrays to provide energy. Juno is spinning like a windmill through space with its 3 giant solar arrays. It is about 540 million miles (869 million kilometers) from Earth.

Juno mission briefing on  July 5, 2016 at JPL after the successful JOI orbit insertion on July 4.  Credit: Roland Keller/rkeusa.blogspot.com
Juno mission briefing on July 5, 2016 at JPL after the successful JOI orbit insertion on July 4. Credit: Roland Keller/rkeusa.blogspot.com

Signals traveling at the speed of light take 48 minutes to reach Earth, said Nybakken.

So the main engine burn, which was fully automated, was already over for some 13 minutes before the first indications of the outcome reach Earth via a series of Doppler signals and tones.

“Tonight, 540 million miles away, Juno performed a precisely choreographed dance at blazing speeds with the largest, most intense planet in our solar system,” said Guy Beutelschies, director of Interplanetary Missions at Lockheed Martin Space Systems.

“Since launch, Juno has operated exceptionally well, and the flawless orbit insertion is a testament to everyone working on Juno and their focus on getting this amazing spacecraft to its destination. NASA now has a science laboratory orbiting Jupiter.”

“The spacecraft is now pointed back at the sun and the antenna back at Earth. The spacecraft performed well and did everything it needed to do,” he reported at the briefing.

“We are looking forward to getting all that science data to Scott and the team.”

“Juno is also the farthest mission to rely on solar power. And although they provide only 1/25th the power at Earth, they still provide over 500 watts of power at Jupiter,” said Nybakken.

Initially the spacecraft enters a long, looping polar orbit lasting about 53 days. That highly elliptical orbit will be trimmed to 14 days for the regular science orbits.

The orbits are designed to minimize contact with Jupiter’s extremely intense radiation belts. The nine science instruments are shielded inside a ½ thick vault built of Titanium to protect them from the utterly deadly radiation of some 20,000,000 rads.

During a 20 month long science mission – entailing 37 orbits lasting 14 days each – the probe will plunge to within about 3000 miles of the turbulent cloud tops and collect unprecedented new data that will unveil the hidden inner secrets of Jupiter’s origin and evolution.

But the length and number of the science orbits has changed since the mission was launched almost 5 years ago in 2011.

Originally Juno was planned to last about one year with an orbital profile involving 33 orbits of 11 days each.

I asked the team to explain the details of how and why the change from 11 to 14 days orbits and increasing the total number of orbits to 37 from 33, especially in light of the extremely harsh radiation hazards?

“The original plan of 33 orbits of 11 days was an example but there were other periods that would work,” Bolton told Universe Today.

“What we really cared about was dropping down over the poles and capturing each longitude, and laying a map or net around Jupiter.”

“Also, during the Earth flyby we went into safe mode. And as we looked at that it was a hiccup by the spacecraft but it actually behaved as it should have.”

“So we said well if that happened at Jupiter we would like to be able to recover and not lose an orbit. So we started to look at the timeline of how long it took to recover, and did we want to add a couple of days to the orbit for conservatism – to ensure the science mission.”

“So it made sense to add 3 days. It didn’t change the science and it made the probability of success even greater. So that was the basis of the change.”

“We also evaluated the radiation. And it wasn’t much different. Juno is designed to take data at a very low risk. The radiation slowly accumulates at the start. As you get to the later part of the mission, it gets a faster and faster accumulation.”

“So we still retained that conservatism as well and the overall radiation dose was pretty much the same,” Bolton explained.

“The radiation we accumulate is not just the more time you spend the more radiation,” Steve Levin, Juno Project Scientist at JPL, told Universe Today.

“Each time we come in close to the planet we get a dose of radiation. Then the spacecraft is out far from Jupiter and is relatively free from that radiation until we come in close again.”

“So just changing from 11 to 14 day orbits does not mean we get more radiation because you are there longer.”

“It’s really the number of times we come in close to Jupiter that determines how much radiation we are getting.”

Juno is the fastest spacecraft ever to arrive at Jupiter and was moving at over 165,000 mph relative to Earth and 130,000 mph relative to Jupiter at the moment of JOI.

Juno’s principal goal is to understand the origin and evolution of Jupiter.

“With its suite of nine science instruments, Juno will investigate the existence of a solid planetary core, map Jupiter’s intense magnetic field, measure the amount of water and ammonia in the deep atmosphere, and observe the planet’s auroras. The mission also will let us take a giant step forward in our understanding of how giant planets form and the role these titans played in putting together the rest of the solar system. As our primary example of a giant planet, Jupiter also can provide critical knowledge for understanding the planetary systems being discovered around other stars,” according to a NASA description.

The $1.1 Billion Juno was launched on Aug. 5, 2011 from Cape Canaveral, Florida atop the most powerful version of the Atlas V rocket augmented by 5 solid rocket boosters and built by United Launch Alliance (ULA). That same Atlas V 551 version just launched MUOS-5 for the US Navy on June 24.

The Juno spacecraft was built by prime contractor Lockheed Martin in Denver.

United Launch Alliance Atlas V liftoff with NASA’s Juno to Jupiter orbiter on Aug. 5, 2011 from Cape Canaveral Air Force Station, Florida. Credit: Ken Kremer/kenkremer.com
United Launch Alliance Atlas V liftoff with NASA’s Juno to Jupiter orbiter on Aug. 5, 2011 from Cape Canaveral Air Force Station, Florida. Credit: Ken Kremer/kenkremer.com

The last NASA spacecraft to orbit Jupiter was Galileo in 1995. It explored the Jovian system until 2003.

Bolton also released new views of Jupiter taken by JunoCam – the on board public outreach camera that snapped a final gorgeous view of the Jovian system showing Jupiter and its four largest moons, dancing around the largest planet in our solar system.

The newly released color image was taken on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter – just before the probe went into autopilot mode.

This is the final view taken by the JunoCam instrument on NASA's Juno spacecraft before Juno's instruments were powered down in preparation for orbit insertion. Juno obtained this color view on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter.  See timelapse movie below.  Credits: NASA/JPL-Caltech/MSSS
This is the final view taken by the JunoCam instrument on NASA’s Juno spacecraft before Juno’s instruments were powered down in preparation for orbit insertion. Juno obtained this color view on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter. See timelapse movie below. Credits: NASA/JPL-Caltech/MSSS

It shows a dramatic view of the clouds bands of Jupiter, dominating a spectacular scene that includes the giant planet’s four largest moons — Io, Europa, Ganymede and Callisto.

Scott Bolton and NASA also released this spectacular new time-lapse JunoCam movie at today’s briefing showing Juno’s approach to Jupiter and the Galilean Moons.

Watch and be mesmerized -“for humanity, our first real glimpse of celestial harmonic motion” says Bolton.

Video caption: NASA’s Juno spacecraft captured a unique time-lapse movie of the Galilean satellites in motion about Jupiter. The movie begins on June 12th with Juno 10 million miles from Jupiter, and ends on June 29th, 3 million miles distant. The innermost moon is volcanic Io; next in line is the ice-crusted ocean world Europa, followed by massive Ganymede, and finally, heavily cratered Callisto. Galileo observed these moons change position with respect to Jupiter over the course of a few nights. From this observation he realized that the moons were orbiting mighty Jupiter, a truth that forever changed humanity’s understanding of our place in the cosmos. Earth was not the center of the Universe. For the first time in history, we look upon these moons as they orbit Jupiter and share in Galileo’s revelation. This is the motion of nature’s harmony. Credits: NASA/JPL-Caltech/MSSS

Along the 5 year journey to Jupiter, Juno made a return trip to Earth on Oct. 9, 2013 for a flyby gravity assist speed boost that enabled the trek to the Jovian system.

During the Earth flyby (EFB), the science team observed Earth using most of Juno’s nine science instruments including, JunoCam, since the slingshot also served as an important dress rehearsal and key test of the spacecraft’s instruments, systems and flight operations teams.

The JunoCam images will be made publicly available to see and process.

During the Earth flyby, Junocam snapped some striking images of Earth as it sped over Argentina, South America and the South Atlantic Ocean and came within 347 miles (560 kilometers) of the surface.

For example a dazzling portrait of our Home Planet high over the South American coastline and the Atlantic Ocean gives a hint of what’s to come from Jupiter’s cloud tops. See our colorized Junocam mosaic of land, sea and swirling clouds, created by Ken Kremer and Marco Di Lorenzo

This colorized composite shows more than half of Earth’s disk over the coast of Argentina and the South Atlantic Ocean as the Juno probe slingshotted by on Oct. 9, 2013 for a gravity assisted acceleration to Jupiter. The mosaic was assembled from raw images taken by the Junocam imager. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo
This colorized composite shows more than half of Earth’s disk over the coast of Argentina and the South Atlantic Ocean as the Juno probe slingshotted by on Oct. 9, 2013 for a gravity assisted acceleration to Jupiter. The mosaic was assembled from raw images taken by the Junocam imager. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

Rick Nybakken, Juno project manager at JPL illustrates how Juno will enter orbit around Jupiter during Juno mission briefing on July 4, 2016 at JPL. Credit: Roland Keller/rkeusa.blogspot.com
Rick Nybakken, Juno project manager at JPL illustrates how Juno will enter orbit around Jupiter during Juno mission briefing on July 4, 2016 at JPL. Credit: Roland Keller/rkeusa.blogspot.com

Juno Snaps Final View of Jovian System Ahead of ‘Independence Day’ Orbital Insertion Fireworks Tonight – Watch Live

This is the final view taken by the JunoCam instrument on NASA's Juno spacecraft before Juno's instruments were powered down in preparation for orbit insertion. Juno obtained this color view on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter. See timelapse movie below. Credits: NASA/JPL-Caltech/MSSS
This is the final view taken by the JunoCam instrument on NASA's Juno spacecraft before Juno's instruments were powered down in preparation for orbit insertion. Juno obtained this color view on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter.  Credit:  Credits: NASA/JPL-Caltech/MSSS
This is the final view taken by the JunoCam instrument on NASA’s Juno spacecraft before Juno’s instruments were powered down in preparation for orbit insertion. Juno obtained this color view on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter. See timelapse movie below. Credits: NASA/JPL-Caltech/MSSS

After a nearly 5 year odyssey across the solar system, NASA’s solar powered Juno orbiter is all set to ignite its main engine late tonight and set off a powerful charge of do-or-die fireworks on America’s ‘Independence Day’ required to place the probe into orbit around Jupiter – the ‘King of the Planets.’

To achieve orbit, Juno must will perform a suspenseful maneuver known as ‘Jupiter Orbit Insertion’ or JOI tonight, Monday, July 4, upon which the entire mission and its fundamental science hinges. There are no second chances!

You can be part of all the excitement and tension building up to and during that moment, which is just hours away – and experience the ‘Joy of JOI’ by tuning into NASA TV tonight!

Watch the live webcast on NASA TV featuring the top scientists and NASA officials starting at 10:30 p.m. EDT (7:30 p.m. PST, 0230 GMT) – direct from NASA’s Jet Propulsion Laboratory: https://www.nasa.gov/nasatv

Illustration of NASA's Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter. Lockheed Martin built the Juno spacecraft for NASA's Jet Propulsion Laboratory.
Illustration of NASA’s Juno spacecraft firing its main engine to slow down and go into orbit around Jupiter. Lockheed Martin built the Juno spacecraft for NASA’s Jet Propulsion Laboratory. Credit: NASA/Lockheed Martin

And for a breathtaking warm-up act, Juno’s on board public outreach JunoCam camera snapped a final gorgeous view of the Jovian system showing Jupiter and its four largest moons, dancing around the largest planet in our solar system.

The newly released color image was taken on June 29, 2016, at a distance of 3.3 million miles (5.3 million kilometers) from Jupiter – just before the probe went into autopilot mode.

It shows a dramatic view of the clouds bands of Jupiter, dominating a spectacular scene that includes the giant planet’s four largest moons — Io, Europa, Ganymede and Callisto.

NASA also released this new time-lapse JunoCam movie today:

Video caption: Juno’s Approach to Jupiter: After nearly five years traveling through space to its destination, NASA’s Juno spacecraft will arrive in orbit around Jupiter on July 4, 2016. This video shows a peek of what the spacecraft saw as it closed in on its destination. Credits: NASA/JPL-Caltech/MSSS

The spacecraft is approaching Jupiter over its north pole, affording an unprecedented perspective on the Jovian system – “which looks like a mini solar system,” said Juno Principal Investigator and chief scientist Scott Bolton, from the Southwest Research Institute (SwRI) in San Antonio, Tx, at today’s media briefing at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif.

“The deep interior of Jupiter is nearly unknown. That’s what we are trying to learn about.”

The 35-minute-long main engine burn is preprogrammed to start at 11:18 p.m. EDT (8:18 p.m. PST, 0318 GMT). It is scheduled to last until approximately 11:53 p.m. (8:53 p.m. PST, 0353 GMT).

Juno mission briefing July 4, 2016 at JPL by Jim Green, Scott Bolton, Rick Nybakken and Heidi Becker.  Credit: Roland Keller
Juno mission briefing July 4, 2016 at JPL by Jim Green, Scott Bolton, Rick Nybakken and Heidi Becker. Credit: Roland Keller/rkeusa.blogspot.com

All of the science instruments were turned off on June 30 to keep the focus on the nail-biting insertion maneuver and preserve battery power, said Bolton. Solar powered Juno is pointed away from the sun during the engine firing.

JOI is required to slow the spacecraft so it can be captured into the gas giant’s orbit as it closes in over the north pole.

Initially the spacecraft will enter a long, looping polar orbit lasting about 53 days. That highly elliptical orbit will quickly be trimmed to 14 days for the science orbits.

The orbits are designed to minimize contact with Jupiter’s extremely intense radiation belts. The science instruments are shielded inside a ½ thick vault built of Titanium to protect them from the utterly deadly radiation – of some 20,000,000 rads.

Artist's concept of NASA's Juno spacecraft crossing the orbits of Jupiter's four largest moons -- Callisto, Gaynmede, Europa and Io -- on its approach to Jupiter. Credits: NASA/JPL-Caltech
Artist’s concept of NASA’s Juno spacecraft crossing the orbits of Jupiter’s four largest moons — Callisto, Gaynmede, Europa and Io — on its approach to Jupiter.
Credits: NASA/JPL-Caltech

Juno is the fastest spacecraft ever to arrive at Jupiter and is moving at over 165,000 mph relative to Earth and 130,000 mph relative to Jupiter.

After a five-year and 2.8 Billion kilometer (1.7 Billion mile) outbound trek to the Jovian system and the largest planet in our solar system and an intervening Earth flyby speed boost, the moment of truth for Juno is now inexorably at hand.

Signals traveling at the speed of light take 48 minutes to reach Earth, said Rick Nybakken, Juno project manager from NASA’s Jet Propulsion Laboratory, at the media briefing.

So the main engine burn, which is fully automated, will already be over for some 13 minutes before the first indications of the outcome reach Earth via a series of Doppler shifts and tones. It is about 540 million miles (869 million kilometers) from Earth.

“By the time the burn is complete, we won’t even hear about it until 13 minutes later.”

“The engine burn will slow Juno by 542 meters/second (1,212 mph) and is fully automated as it approaches over Jupiter’s North Pole,” explained Nybakken.

“The long five year cruise enabled us to really learn about the spacecraft and how it operates.”

As it travels through space, the basketball court sized Juno is spinning like a windmill with its 3 giant solar arrays.

“Juno is also the farthest mission to rely on solar power. The solar panels are 60 square meters in size. And although they provide only 1/25th the power at Earth, they still provide over 500 watts of power at Jupiter.”

Rick Nybakken, Juno project manager at JPL illustrates how Juno will enter orbit around Jupiter during Juno mission briefing on July 4, 2016 at JPL. Credit: Roland Keller
Rick Nybakken, Juno project manager at JPL illustrates how Juno will enter orbit around Jupiter during Juno mission briefing on July 4, 2016 at JPL. Credit: Roland Keller/rkeusa.blogspot.com

The protective cover that shields Juno’s main engine from micrometeorites and interstellar dust was opened on June 20.

During a 20 month long science mission – entailing 37 orbits lasting 14 days each – the probe will plunge to within about 3000 miles of the turbulent cloud tops and collect unprecedented new data that will unveil the hidden inner secrets of Jupiter’s origin and evolution.

“Jupiter is the Rosetta Stone of our solar system,” says Bolton. “It is by far the oldest planet, contains more material than all the other planets, asteroids and comets combined and carries deep inside it the story of not only the solar system but of us. Juno is going there as our emissary — to interpret what Jupiter has to say.”

During the orbits, Juno will probe beneath the obscuring cloud cover of Jupiter and study its auroras to learn more about the planet’s origins, structure, atmosphere and magnetosphere.

The $1.1 Billion Juno was launched on Aug. 5, 2011 from Cape Canaveral, Florida atop the most powerful version of the Atlas V rocket augmented by 5 solid rocket boosters and built by United Launch Alliance (ULA). That same Atlas V 551 version just launched MUOS-5 for the US Navy on June 24.

The Juno spacecraft was built by prime contractor Lockheed Martin in Denver.

Juno soars skyward to Jupiter on Aug. 5, 2011 from launch pad 41 at Cape Canaveral Air Force Station at 12:25 p.m. EDT. View from the VAB roof. Credit: Ken Kremer/kenkremer.com
Juno soars skyward to Jupiter on Aug. 5, 2011 from launch pad 41 at Cape Canaveral Air Force Station at 12:25 p.m. EDT. View from the VAB roof. Credit: Ken Kremer/kenkremer.com

Along the way Juno made a return trip to Earth on Oct. 9, 2013 for a flyby gravity assist speed boost that enabled the trek to Jupiter.

The flyby provided 70% of the velocity compared to the Atlas V launch, said Nybakken.

During the Earth flyby (EFB), the science team observed Earth using most of Juno’s nine science instruments since the slingshot also serves as an important dress rehearsal and key test of the spacecraft’s instruments, systems and flight operations teams.

Juno also went into safe mode – something the team must avoid during JOI.

What lessons were learned from the safe mode event and applied to JOI, I asked?

“We had the battery at 50% state of charge during the EFB and didn’t accurately predict the sag on the battery when we went into eclipse. We now have a validated high fidelity power model which would have predicted that sag and we would have increased the battery voltage,” Nybakken told Universe Today

“It will not happen at JOI as we don’t go into eclipse and are at 100% SOC. Plus the instruments are off which increases our power margins.”

Junocam also took some striking images of Earth as it sped over Argentina, South America and the South Atlantic Ocean and came within 347 miles (560 kilometers) of the surface.

For example the dazzling portrait of our Home Planet high over the South American coastline and the Atlantic Ocean.

For a hint of what’s to come, see our colorized Junocam mosaic of land, sea and swirling clouds, created by Ken Kremer and Marco Di Lorenzo

NASA's Juno probe captured the image data for this composite picture during its Earth flyby on Oct. 9 over Argentina,  South America and the southern Atlantic Ocean. Raw imagery was reconstructed and aligned by Ken Kremer and Marco Di Lorenzo, and false-color blue has been added to the view taken by a near-infrared filter that is typically used to detect methane. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo
NASA’s Juno probe captured the image data for this composite picture during its Earth flyby on Oct. 9 over Argentina, South America and the southern Atlantic Ocean. Raw imagery was reconstructed and aligned by Ken Kremer and Marco Di Lorenzo, and false-color blue has been added to the view taken by a near-infrared filter that is typically used to detect methane. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo

The last NASA spacecraft to orbit Jupiter was Galileo in 1995. It explored the Jovian system until 2003.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

Infographic about Juno’s Jupiter Orbit Insertion (JOI) maneuver on July 4, 2016.   Credit: NASA/Lockheed Martin
Infographic about Juno’s Jupiter Orbit Insertion (JOI) maneuver on July 4, 2016. Credit: NASA/Lockheed Martin

NASA Approves New Horizons Extended KBO Mission, Keeps Dawn at Ceres

New Horizons trajectory and the orbits of Pluto and 2014 MU69.
New Horizons trajectory and the orbits of Pluto and 2014 MU69.
New Horizons trajectory and the orbits of Pluto and 2014 MU69.

In an ‘Independence Day’ gift to a slew of US planetary research scientists, NASA has granted approval to nine ongoing missions to continue for another two years this holiday weekend.

The biggest news is that NASA green lighted a mission extension for the New Horizons probe to fly deeper into the Kuiper Belt and decided to keep the Dawn probe at Ceres forever, rather than dispatching it to a record breaking third main belt asteroid.

And the exciting extension news comes just as the agency’s Juno probe is about to ignite a do or die July 4 fireworks display to achieve orbit at Jupiter – detailed here.

“Mission approved!” the researchers gleefully reported on the probes Facebook and Twitter social media pages.

“Our extended mission into the #KuiperBelt has been approved. Thanks to everyone for following along & hopefully the best is yet to come.

Dwarf planet Ceres is shown in this false-color renderings, which highlight differences in surface materials.  The image is centered on Ceres brightest spots at Occator crater. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
Dwarf planet Ceres is shown in this false-color renderings, which highlight differences in surface materials. The image is centered on Ceres brightest spots at Occator crater. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

The New Horizons spacecraft will now continue on course in the Kuiper Belt towards an small object known as 2014 MU69, to carry out the most distant close encounter with a celestial object in human history.

“Here’s to continued success!”

The spacecraft will rendezvous with the ancient rock on New Year’s Day 2019.

Researchers say that 2014 MU69 is considered as one of the early building blocks of the solar system and as such will be invaluable to scientists studying the origin of our solar system how it evolved.

It was almost exactly one year ago on July 14, 2015 that New Horizons conducted Earth’s first ever up close flyby and science reconnaissance of Pluto – the most distant planet in our solar system and the last of the nine planets to be explored.

Pluto Explored at Last. The New Horizons mission team celebrates successful flyby of Pluto in the moments after closest approach at 7:49 a.m. EDT on July 14, 2015.   New Horizons Principal Investigator Alan Stern of Southwest Research Institute (SwRI), Boulder, CO., left, Johns Hopkins University Applied Physics Laboratory (APL) Director Ralph Semmel, center, and New Horizons Co-Investigator Will Grundy Lowell Observatory hold an enlarged print of an U.S. stamp with their suggested update after Pluto became the final planet in our solar system to be explored by an American space probe (crossing out the words ‘not yet’) - at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Maryland.  Credit: Ken Kremer/kenkremer.com
Pluto Explored at Last. The New Horizons mission team celebrates successful flyby of Pluto in the moments after closest approach at 7:49 a.m. EDT on July 14, 2015. New Horizons Principal Investigator Alan Stern of Southwest Research Institute (SwRI), Boulder, CO., left, Johns Hopkins University Applied Physics Laboratory (APL) Director Ralph Semmel, center, and New Horizons Co-Investigator Will Grundy Lowell Observatory hold an enlarged print of an U.S. stamp with their suggested update after Pluto became the final planet in our solar system to be explored by an American space probe (crossing out the words ‘not yet’) – at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Maryland. Credit: Ken Kremer/kenkremer.com

The immense volume of data gathered continues to stream back to Earth every day.

“The New Horizons mission to Pluto exceeded our expectations and even today the data from the spacecraft continue to surprise,” said NASA’s Director of Planetary Science Jim Green at NASA HQ in Washington, D.C.

“We’re excited to continue onward into the dark depths of the outer solar system to a science target that wasn’t even discovered when the spacecraft launched.”

This new global mosaic view of Pluto was created from the latest high-resolution images to be downlinked from NASA’s New Horizons spacecraft and released on Sept. 11, 2015. The images were taken as New Horizons flew past Pluto on July 14, 2015, from a distance of 50,000 miles (80,000 kilometers). This new mosaic was stitched from over two dozen raw images captured by the LORRI imager and colorized. Annotated with informal place names. Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Marco Di Lorenzo/Ken Kremer/kenkremer.com
This new global mosaic view of Pluto was created from the latest high-resolution images to be downlinked from NASA’s New Horizons spacecraft and released on Sept. 11, 2015. The images were taken as New Horizons flew past Pluto on July 14, 2015, from a distance of 50,000 miles (80,000 kilometers). This new mosaic was stitched from over two dozen raw images captured by the LORRI imager and colorized. Annotated with informal place names. Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Marco Di Lorenzo/Ken Kremer/kenkremer.com

While waiting for news on whether NASA would approve an extended mission, the New Horizons engineering and science team already ignited the main engine four times to carry out four course changes in October and November 2015, in order to preserve the option of the flyby past 2014 MU69 on Jan 1, 2019.

Green noted that mission extensions into fiscal years 2017 and 2018 are not final until Congress actually passes sufficient appropriation to fund NASA’s Planetary Science Division.

“Final decisions on mission extensions are contingent on the outcome of the annual budget process.”

Tough choices were made even tougher because the Obama Administration has cut funding for the Planetary Sciences Division – some of which was restored by a bipartisan majority in Congress for what many consider NASA’s ‘crown jewels.’

NASA’s Dawn asteroid orbiter just completed its primary mission at dwarf planet Ceres on June 30, just in time for the global celebration known as Asteroid Day.

“The mission exceeded all expectations originally set for its exploration of protoplanet Vesta and dwarf planet Ceres,” said NASA officials.

The Dawn science team had recently submitted a proposal to break out of orbit around the middle of this month in order to this conduct a flyby of the main belt asteroid Adeona.

Green declined to approve the Dawn proposal, citing additional valuable science to be gathered at Ceres.

The long-term monitoring of Ceres, particularly as it gets closer to perihelion – the part of its orbit with the shortest distance to the sun — has the potential to provide more significant science discoveries than a flyby of Adeona,” he said.

The funding required for a multi-year mission to Adeona would be difficult in these cost constrained times.

However the spacecraft is in excellent shape and the trio of science instruments are in excellent health.

Dawn arrived at Ceres on March 6, 2015 and has been conducting unprecedented investigation ever since.

Dawn is Earth’s first probe in human history to explore any dwarf planet, the first to explore Ceres up close and the first to orbit two celestial bodies.

The asteroid Vesta was Dawn’s first orbital target where it conducted extensive observations of the bizarre world for over a year in 2011 and 2012.

The mission is expected to last until at least later into 2016, and possibly longer, depending upon fuel reserves.

Due to expert engineering and handling by the Dawn mission team, the probe unexpectedly has hydrazine maneuvering fuel leftover.

Dawn will remain at its current altitude at the Low Altitude Mapping Orbit (LAMO) for the rest of its mission, and indefinitely afterward, even when no further communications are possible.

Green based his decision on the mission extensions on the biannual peer review scientific assessment by the Senior Review Panel.

Dawn was launched in September 2007.

The other mission extensions – contingent on available resources – are: the Mars Reconnaissance Orbiter (MRO), Mars Atmosphere and Volatile EvolutioN (MAVEN), the Opportunity and Curiosity Mars rovers, the Mars Odyssey orbiter, the Lunar Reconnaissance Orbiter (LRO), and NASA’s support for the European Space Agency’s Mars Express mission.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Curiosity Finds Ancient Mars Likely Had More Oxygen and Was More Hospitable to Life

This scene shows NASA's Curiosity Mars rover at a location called "Windjana," where the rover found rocks containing manganese-oxide minerals, which require abundant water and strongly oxidizing conditions to form. Credits: NASA/JPL-Caltech/MSSS
This scene shows NASA's Curiosity Mars rover at a location called "Windjana," where the rover found rocks containing manganese-oxide minerals, which require abundant water and strongly oxidizing conditions to form. Credits: NASA/JPL-Caltech/MSSS
This scene shows NASA’s Curiosity Mars rover at a location called “Windjana,” where the rover found rocks containing manganese-oxide minerals, which require abundant water and strongly oxidizing conditions to form. Credits: NASA/JPL-Caltech/MSSS

New chemical science findings from NASA’s Mars rover Curiosity indicate that ancient Mars likely had a higher abundance of molecular oxygen in its atmosphere compared to the present day and was thus more hospitable to life forms, if they ever existed.

Thus the Red Planet was much more Earth-like and potentially habitable billions of years ago compared to the cold, barren place we see today.

Curiosity discovered high levels of manganese oxide minerals in rocks investigated at a location called “Windjana” during the spring of 2014.

Manganese-oxide minerals require abundant water and strongly oxidizing conditions to form.

“Researchers found high levels of manganese oxides by using a laser-firing instrument on the rover. This hint of more oxygen in Mars’ early atmosphere adds to other Curiosity findings — such as evidence about ancient lakes — revealing how Earth-like our neighboring planet once was,” NASA reported.

The newly announced results stem from results obtained from the rovers mast mounted ChemCam or Chemistry and Camera laser firing instrument. ChemCam operates by firing laser pulses and then observes the spectrum of resulting flashes of plasma to assess targets’ chemical makeup.

“The only ways on Earth that we know how to make these manganese materials involve atmospheric oxygen or microbes,” said Nina Lanza, a planetary scientist at Los Alamos National Laboratory in New Mexico, in a statement.

“Now we’re seeing manganese oxides on Mars, and we’re wondering how the heck these could have formed?”

The discovery is being published in a new paper in the American Geophysical Union’s Geophysical Research Letters. Lanza is the lead author.

The manganese oxides were found by ChemCam in mineral veins investigated at “Windjana” and are part of geologic timeline being assembled from Curiosity’s research expedition across of the floor of the Gale Crater landing site.

Scientists have been able to link the new finding of a higher oxygen level to a time when groundwater was present inside Gale Crater.

“These high manganese materials can’t form without lots of liquid water and strongly oxidizing conditions,” says Lanza.

“Here on Earth, we had lots of water but no widespread deposits of manganese oxides until after the oxygen levels in our atmosphere rose.”

The high-manganese materials were found in mineral-filled cracks in sandstones in the “Kimberley” region of the crater.

Curiosity’s Panoramic view of Mount Remarkable at ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 603, April 17, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo.  Featured on APOD - Astronomy Picture of the Day on May 7, 2014
Curiosity’s Panoramic view of Mount Remarkable at ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. The navcam raw images were taken on Sol 603, April 17, 2014, stitched and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo. Featured on APOD – Astronomy Picture of the Day on May 7, 2014

High concentrations of manganese oxide minerals in Earth’s ancient past correspond to a major shift in our atmosphere’s composition from low to high oxygen atmospheric concentrations. Thus its reasonable to suggest the same thing happened on ancient Mars.

As part of the investigation, Curiosity also conducted a drill campaign at Windjana, her 3rd of the mission.

Composite photo mosaic shows deployment of NASA Curiosity rovers robotic arm and two holes after drilling into ‘Windjana’ sandstone rock on May 5, 2014, Sol 621, at Mount Remarkable as missions third drill target for sample analysis by rover’s chemistry labs.  The navcam raw images were stitched together from several Martian days up to Sol 621, May 5, 2014 and colorized.   Credit: NASA/JPL-Caltech/Ken Kremer - kenkremer.com/Marco Di Lorenzo
Composite photo mosaic shows deployment of NASA Curiosity rovers robotic arm and two holes after drilling into ‘Windjana’ sandstone rock on May 5, 2014, Sol 621, at Mount Remarkable as missions third drill target for sample analysis by rover’s chemistry labs. The navcam raw images were stitched together from several Martian days up to Sol 621, May 5, 2014 and colorized. Credit: NASA/JPL-Caltech/Ken Kremer – kenkremer.com/Marco Di Lorenzo

How much manganese oxide was detected and what is the meaning?

“The Curiosity rover observed high-Mn abundances (>25 wt% MnO) in fracture-filling materials that crosscut sandstones in the Kimberley region of Gale crater, Mars,” according to the AGU paper.

“On Earth, environments that concentrate Mn and deposit Mn minerals require water and highly oxidizing conditions, hence these findings suggest that similar processes occurred on Mars.”

“Based on the strong association between Mn-oxide deposition and evolving atmospheric dioxygen levels on Earth, the presence of these Mn-phases on Mars suggests that there was more abundant molecular oxygen within the atmosphere and some groundwaters of ancient Mars than in the present day.”

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

NASA Completes Awesome Test Firing of World’s Most Powerful Booster for Human Mission to Mars – Gallery

Ignition of the qualification motor (QM-2) booster during test firing for NASA’s Space Launch System as seen on Tuesday, June 28, 2016, at Orbital ATK Propulsion System's (SLS) test facilities in Promontory, Utah. Credit: Julian Leek
Ignition of the qualification motor (QM-2) booster during test firing for NASA’s Space Launch System as seen on Tuesday, June 28, 2016, at Orbital ATK Propulsion System's (SLS) test facilities in Promontory, Utah.  Credit: Julian Leek
Ignition of the qualification motor (QM-2) booster during test firing for NASA’s Space Launch System as seen on Tuesday, June 28, 2016, at Orbital ATK Propulsion System’s (SLS) test facilities in Promontory, Utah. Credit: Julian Leek

The world’s most powerful booster that will one day propel NASA astronauts on exciting missions of exploration to deep space destinations including the Moon and Mars was successfully ignited this morning, June 28, during an awesome ground test firing on a remote mountainside in Utah, that qualifies it for an inaugural blastoff in late 2018.

The two-minute-long, full-duration static test for NASA’s mammoth Space Launch System (SLS) rocket involved firing the new five-segment solid rocket booster for its second and final qualification ground test as it sat restrained in a horizontal configuration at Orbital ATK’s test facilities at a desert site in Promontory, Utah.

The purpose was to provide NASA and prime contractor Orbital ATK with critical data on 82 qualification objectives. Engineers will use the data gathered by more than 530 instrumentation channels on the booster to certify the booster for flight.

The 154-foot-long (47-meter) booster was fired up on the test stand by the Orbital ATK operations team at 11:05 a.m. EDT (9:05 a.m. MT) for what is called the Qualification Motor-2 (QM-2) test.

“We have ignition of NASA’s Space Launch System motor powering us on our Journey to Mars,” said NASA commentator Kim Henry at ignition!

A gigantic plume of black smoke and intense yellow fire erupted at ignition spewing a withering cloud of ash into the Utah air and barren mountainside while consuming propellant at a rate of 5.5 tons per second.

It also sent out a shock wave reverberating back to excited company, NASA and media spectators witnessing the event from about a mile away as well as to another 10,000 or so space enthusiasts and members of the general public gathered to watch from about 2 miles away.

Ignition of the qualification motor (QM-2) booster during test firing for NASA’s Space Launch System as seen on Tuesday, June 28, 2016, at Orbital ATK Propulsion System's (SLS) test facilities in Promontory, Utah.  Credit: Julian Leek
Ignition of the qualification motor (QM-2) booster during test firing for NASA’s Space Launch System as seen on Tuesday, June 28, 2016, at Orbital ATK Propulsion System’s (SLS) test facilities in Promontory, Utah. Credit: Julian Leek

“What an absolutely amazing day today for all of us here to witness this test firing. And it’s not just a test firing. It’s really a qualification motor test firing that says this design is ready to go fly and ready to go do the mission which it’s designed to go do,” said William Gerstenmaier, associate administrator for the Human Exploration and Operations Mission Directorate at NASA Headquarters in Washington, during the post QM-2 test media briefing today.

Thrilled spectators witness the Qualification Motor-2 (QM-2) test firing on June 28, 2016 at Orbital ATK test facilities in Promontory, Utah.  Credit: Jean Leek
Thrilled spectators witness the Qualification Motor-2 (QM-2) test firing on June 28, 2016 at Orbital ATK test facilities in Promontory, Utah. Credit: Jean Leek

The critically important test marks a major milestone clearing the path to the first SLS launch that could happen as soon as September 2018, noted Gerstenmaier

“The team did a tremendous professional job to get all this ready for the firing. We will get over 500 channels of data on this rocket. They will pour over the data to ensure it will perform exactly the way we intended it to at these cold conditions.”

Qualification motor (QM-2) booster fires up erupting massive smoke cloud during test of NASA’s Space Launch System on Tuesday, June 28, 2016, at Orbital ATK test facilities in Promontory, Utah.  Credit: Dawn Taylor
Qualification motor (QM-2) booster fires up erupting massive smoke cloud during test of NASA’s Space Launch System on Tuesday, June 28, 2016, at Orbital ATK test facilities in Promontory, Utah. Credit: Dawn Taylor

The QM-2 booster had been pre-chilled for several weeks inside a huge test storage shed to conduct this so called ‘cold motor test’ at approximately 40 degrees Fahrenheit (5 C) – corresponding to the colder end of its accepted propellant temperature range.

NASA’s Space Launch System (SLS) rocket with lift off using two of the five segment solid rocket motors and four RS-25 engines to power the maiden launch of SLS and NASA’s Orion deep space manned spacecraft in late 2018.

The SLS boosters are derived from the four segment solid rocket boosters (SRBs) originally delevoped for NASA’s space shuttle program and used for 3 decades.

“This final qualification test of the booster system shows real progress in the development of the Space Launch System,” said NASA associate administrator Gerstenmaier.

“Seeing this test today, and experiencing the sound and feel of approximately 3.6 million pounds of thrust, helps us appreciate the progress we’re making to advance human exploration and open new frontiers for science and technology missions in deep space.”

Despite being cooled to 41 F (5 C) for the cold motor test the flames emitted by the 12-foot-diameter (3.6-meter) booster are actually hot enough at some 6000 degrees Fahrenheit to boil steel.

The internal pressure reaches about 900 psi.

NASA's Space Launch System Solid Rocket Booster infographic
NASA’s Space Launch System Solid Rocket Booster infographic

The first ground test called QM-1 was conducted at 90 degrees Fahrenheit, at the upper end of the operating range, in March 2015 as I reported earlier here.

This second ground test firing took place about 1 hour later than originally planned due to a technical issue with the ground sequencing computer control system.

The next time one of these solid rocket boosters fire will be for the combined SLS-1/Orion EM-1 test flight in late 2018.

Each booster generates approximately 3.6 million pounds of thrust. Overall they will provide more than 75 percent of the thrust needed for the rocket and Orion spacecraft to escape Earth’s gravitational pull, says NASA.

“It was awesome to say the least,” space photographer and friend Julian Leek who witnessed the test first hand told Universe Today.

“Massive fire power released over the Utah mountains. There was about a five second delay before you could hear the sound – that really got everyone’s attention!”

“It was absolutely magnificent,” space photographer friend Dawn Taylor told me. “Can’t wait to see it at the Cape when it goes vertical.”

To date Orbital ATK has cast 3 of the 10 booster segments required for the 2018 launch, said Charlie Precourt, vice president and general manager of Orbital ATK’s Propulsion Systems Division in Promontory, Utah.

I asked Precourt about the production timing for the remaining segments.

“All of the segments will be delivered to NASA at the Kennedy Space Center (KSC) in Florida by next fall,” Precourt replied during the media briefing.

“They will be produced at a rate of roughly one a month. We also have to build the nozzles up and so forth.”

When will booster stacking begin inside the Vehicle Assembly Building (VAB) at KSC?

Booster shipments start shipping from Utah this fall. Booster stacking in the VAB starts in the spring of 2018,” Alex Priskos, manager of the NASA SLS Boosters Office at Marshall Space Flight Center in Huntsville, Alabama, told me.

Furthermore a preliminary look at the data indicates that all went well.

“What an outstanding test. After a look at some very preliminary data everything looks great so far,” Priskos said at the briefing. “We’re going to be digging into the data a lot more as we go forward.”

The five-segment Qualification Motor-2 (QM-2) test booster for NASA's SLS just prior to full duration firing at Orbital ATK test facility in Promontory, Utah, on June 28, 2016.  Credit: Julian Leek
The spent five-segment Qualification Motor-2 (QM-2) test booster for NASA’s SLS soon after the full duration firing at Orbital ATK test facility in Promontory, Utah, on June 28, 2016. Credit: Julian Leek

Meanwhile the buildup of US flight hardware continues at NASA and contractor centers around the US, as well as the Orion service module from ESA.

The maiden test flight of the SLS/Orion is targeted for no later than November 2018 and will be configured in its initial 70-metric-ton (77-ton) version with a liftoff thrust of 8.4 million pounds.

In February 2016 the welded skeletal backbone for the Orion EM-1 mission arrived at the Kennedy Space Center for outfitting with all the systems and subsystems necessary for flight.

The core stage fuel tank holding the cryogenic liquid oxygen and hydrogen propellants is being welded together at NASA’s Michoud Assembly Facility in New Orleans, LA.

Orion crew module pressure vessel for NASA’s Exploration Mission-1 (EM-1) is unveiled for the first time on Feb. 3, 2016 after arrival at the agency’s Kennedy Space Center (KSC) in Florida. It is secured for processing in a test stand called the birdcage in the high bay inside the Neil Armstrong Operations and Checkout (O&C) Building at KSC. Launch to the Moon is slated in 2018 atop the SLS rocket.  Credit: Ken Kremer/kenkremer.com
Orion crew module pressure vessel for NASA’s Exploration Mission-1 (EM-1) is unveiled for the first time on Feb. 3, 2016 after arrival at the agency’s Kennedy Space Center (KSC) in Florida. It is secured for processing in a test stand called the birdcage in the high bay inside the Neil Armstrong Operations and Checkout (O&C) Building at KSC. Launch to the Moon is slated in 2018 atop the SLS rocket. Credit: Ken Kremer/kenkremer.com

Although the SLS-1 flight in 2018 will be uncrewed, NASA plans to launch astronauts on the SLS-2/EM-2 mission slated for the 2021 to 2023 timeframe.

It all depends on the budget NASA receives from Congress and who is elected President in the election in November 2016.

“If we can keep our focus and keep delivering, and deliver to the schedules, the budgets and the promise of what we’ve got, I think we’ve got a very capable vision that actually moves the nation very far forward in moving human presence into space,” Gerstenmaier explained at the briefing.

“This is a very capable system. It’s not built for just one or two flights. It is actually built for multiple decades of use that will enable us to eventually allow humans to go to Mars in the 2030s.

One forerunner to the Mars mission could be a habitation module around the Moon perhaps five years from now.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

An Orbital ATK technician inspects hardware and instrumentation on a full-scale, test version booster for NASA's new rocket, the Space Launch System. The booster is being cooled to approximately 40 degrees Fahrenheit ahead of its second qualification ground test June 28 at Orbital ATK's test facilities in Promontory, Utah. Testing at the thermal extremes experienced by the booster on the launch pad is important to understanding the effects of temperature on the performance of how the propellant burns.   Credits: Orbital ATK
An Orbital ATK technician inspects hardware and instrumentation on a full-scale, test version booster for NASA’s new rocket, the Space Launch System. The booster is being cooled to approximately 40 degrees Fahrenheit ahead of its second qualification ground test June 28 at Orbital ATK’s test facilities in Promontory, Utah. Testing at the thermal extremes experienced by the booster on the launch pad is important to understanding the effects of temperature on the performance of how the propellant burns. Credits: Orbital ATK
The second and final qualification motor (QM-2) test for the Space Launch System’s booster is seen, Tuesday, June 28, 2016, at Orbital ATK Propulsion Systems test facilities in Promontory, Utah. During the Space Launch System flight the boosters will provide more than 75 percent of the thrust needed to escape the gravitational pull of the Earth, the first step on NASA’s Journey to Mars. Photo Credit: (NASA/Bill Ingalls)
The second and final qualification motor (QM-2) test for the Space Launch System’s booster is seen, Tuesday, June 28, 2016, at Orbital ATK Propulsion Systems test facilities in Promontory, Utah. During the Space Launch System flight the boosters will provide more than 75 percent of the thrust needed to escape the gravitational pull of the Earth, the first step on NASA’s Journey to Mars. Photo Credit: (NASA/Bill Ingalls)
Mountainside test location for the Qualification motor-2 (QM-2) test of the 5-segment solid rocket motor designed for NASA's Space Launch System (SLS) at Orbital ATK test facility in Promontory, Utah, on June 28, 2016.  Credit: Julian Leek
Mountainside test location for the Qualification motor-2 (QM-2) test of the 5-segment solid rocket motor designed for NASA’s Space Launch System (SLS) at Orbital ATK test facility in Promontory, Utah, on June 28, 2016. Credit: Julian Leek
The five-segment Qualification motor-2 (QM-2) test booster for NASA's Space Launch System (SLS) being readied for full duration firing at Orbital ATK test facility in Promontory, Utah, on June 28, 2016.  Credit: NASA
The five-segment Qualification motor-2 (QM-2) test booster for NASA’s Space Launch System (SLS) being readied for full duration firing at Orbital ATK test facility in Promontory, Utah, on June 28, 2016. Credit: NASA

7 Days Out From Orbital Insertion, NASA’s Juno Images Jupiter and its Largest Moons

This annotated color view of Jupiter and its four largest moons -- Io, Europa, Ganymede and Callisto -- was taken by the JunoCam camera on NASA's Juno spacecraft on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) from Jupiter. Image credit: NASA/JPL-Caltech/MSSS
This annotated color view of Jupiter and its four largest moons -- Io, Europa, Ganymede and Callisto -- was taken by the JunoCam camera on NASA's Juno spacecraft on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) from Jupiter. Image credit: NASA/JPL-Caltech/MSSS
This annotated color view of Jupiter and its four largest moons — Io, Europa, Ganymede and Callisto — was taken by the JunoCam camera on NASA’s Juno spacecraft on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) from Jupiter. Image credit: NASA/JPL-Caltech/MSSS

Now just 7 days out from a critical orbital insertion burn, NASA’s Jupiter-bound Juno orbiter is closing in fast on the massive gas giant. And as its coming into focus the spacecraft has begun snapping a series of beautiful images of the biggest planet and its biggest moons.

In a newly released color image snapped by the probes educational public outreach camera named Junocam, banded Jupiter dominates a spectacular scene that includes the giant planet’s four largest moons — Io, Europa, Ganymede and Callisto.

Junocam’s image of the approaching Jovian system was taken on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) and hints at the multitude of photos and science riches to come from Juno.

“Juno on Jupiter’s Doorstep,” says a NASA description. “And the alternating light and dark bands of the planet’s clouds are just beginning to come into view,” revealing its “distinctive swirling bands of orange, brown and white.”

This color view of Jupiter and its four largest moons -- Io, Europa, Ganymede and Callisto -- was taken by the JunoCam camera on NASA's Juno spacecraft on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) from Jupiter. Image credit: NASA/JPL-Caltech/MSSS
This color view of Jupiter and its four largest moons — Io, Europa, Ganymede and Callisto — was taken by the JunoCam camera on NASA’s Juno spacecraft on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) from Jupiter. Image credit: NASA/JPL-Caltech/MSSS

Rather appropriately for an American space endeavor, the fate of the entire mission hinges on do or die ‘Independence Day’ fireworks.

On the evening of July 4, Juno must fire its main engine for 35 minutes.

The Joy of JOI – or Jupiter Orbit Insertion – will place NASA’s robotic explorer into a polar orbit around the gas giant.

The approach over the north pole is unlike earlier probes that approached from much lower latitudes nearer the equatorial zone, and thus provide a perspective unlike any other.

After a five-year and 2.8 Billion kilometer (1.7 Billion mile) outbound trek to the Jovian system and the largest planet in our solar system and an intervening Earth flyby speed boost, the moment of truth for Juno is now inexorably at hand.

This colorized composite shows more than half of Earth’s disk over the coast of Argentina and the South Atlantic Ocean as the Juno probe slingshotted by on Oct. 9, 2013 for a gravity assisted acceleration to Jupiter. The mosaic was assembled from raw images taken by the Junocam imager. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo
This colorized composite shows more than half of Earth’s disk over the coast of Argentina and the South Atlantic Ocean as the Juno probe slingshotted by on Oct. 9, 2013 for a gravity assisted acceleration to Jupiter. The mosaic was assembled from raw images taken by the Junocam imager. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo

And preparations are in full swing by the science and engineering team to ensure a spectacular Fourth of July fireworks display.

The team has been in contact with Juno 24/7 since June 11 and already uplinked the rocket firing parameters.

Signals traveling at the speed of light take 10 minutes to reach Earth.

The protective cover that shields Juno’s main engine from micrometeorites and interstellar dust was opened on June 20.

“And the software program that will command the spacecraft through the all-important rocket burn was uplinked,” says NASA.

The pressurization of the propulsion system is set for June 28.

“We have over five years of spaceflight experience and only 10 days to Jupiter orbit insertion,” said Rick Nybakken, Juno project manager from NASA’s Jet Propulsion Laboratory in Pasadena, California, said in a statement.

“It is a great feeling to put all the interplanetary space in the rearview mirror and have the biggest planet in the solar system in our windshield.”

On the night of orbital insertion, Juno will fly within 2,900 miles (4,667 kilometers) of the Jovian cloud tops.

All instruments except those critical for the JOI insertion burn on July 4, will be tuned off on June 29. That includes shutting down Junocam.

“If it doesn’t help us get into orbit, it is shut down,” said Scott Bolton, Juno’s principal investigator from the Southwest Research Institute in San Antonio.

“That is how critical this rocket burn is. And while we will not be getting images as we make our final approach to the planet, we have some interesting pictures of what Jupiter and its moons look like from five-plus million miles away.”

During a 20 month long science mission – entailing 37 orbits lasting 11 days each – the probe will plunge to within about 3000 miles of the turbulent cloud tops and collect unprecedented new data that will unveil the hidden inner secrets of Jupiter’s origin and evolution.

“Jupiter is the Rosetta Stone of our solar system,” says Bolton. “It is by far the oldest planet, contains more material than all the other planets, asteroids and comets combined and carries deep inside it the story of not only the solar system but of us. Juno is going there as our emissary — to interpret what Jupiter has to say.”

During the orbits, Juno will probe beneath the obscuring cloud cover of Jupiter and study its auroras to learn more about the planet’s origins, structure, atmosphere and magnetosphere.

Junocam has already taken some striking images during the Earth flyby gravity assist speed boost on Oct. 9, 2013.

For example the dazzling portrait of our Home Planet high over the South American coastline and the Atlantic Ocean.

For a hint of what’s to come, see our colorized Junocam mosaic of land, sea and swirling clouds, created by Ken Kremer and Marco Di Lorenzo.

NASA's Juno probe captured the image data for this composite picture during its Earth flyby on Oct. 9 over Argentina,  South America and the southern Atlantic Ocean. Raw imagery was reconstructed and aligned by Ken Kremer and Marco Di Lorenzo, and false-color blue has been added to the view taken by a near-infrared filter that is typically used to detect methane. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo
NASA’s Juno probe captured the image data for this composite picture during its Earth flyby on Oct. 9 over Argentina, South America and the southern Atlantic Ocean. Raw imagery was reconstructed and aligned by Ken Kremer and Marco Di Lorenzo, and false-color blue has been added to the view taken by a near-infrared filter that is typically used to detect methane. Credit: NASA/JPL/SwRI/MSSS/Ken Kremer/Marco Di Lorenzo

As Juno sped over Argentina, South America and the South Atlantic Ocean it came within 347 miles (560 kilometers) of Earth’s surface.

During the flyby, the science team observed Earth using most of Juno’s nine science instruments since the slingshot also serves as an important dress rehearsal and key test of the spacecraft’s instruments, systems and flight operations teams.

Juno soars skyward to Jupiter on Aug. 5, 2011 from launch pad 41 at Cape Canaveral Air Force Station at 12:25 p.m. EDT. View from the VAB roof. Credit: Ken Kremer/kenkremer.com
Juno soars skyward to Jupiter on Aug. 5, 2011 from launch pad 41 at Cape Canaveral Air Force Station at 12:25 p.m. EDT. View from the VAB roof. Credit: Ken Kremer/kenkremer.com

The $1.1 Billion Juno was launched on Aug. 5, 2011 from Cape Canaveral, Florida atop the most powerful version of the Atlas V rocket augmented by 5 solid rocket boosters and built by United Launch Alliance (ULA). That same Atlas V 551 version just launched MUOS-5 for the US Navy on June 24.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.
Ken Kremer

Juno spacecraft and its science instruments. Image credit: NASA/JPL
Juno spacecraft and its science instruments. Image credit: NASA/JPL
Juno graphic
Juno orbital graphic

Spectacular Launch of Most Powerful Atlas Completes Constellation of Navy’s Advanced Tactical Comsats – Gallery

A United Launch Alliance (ULA) Atlas V rocket carrying the MUOS-5 mission lifts off from Space Launch Complex-41 at 10:30 a.m. EDT on June 24, 2016. Credit: United Launch Alliance
A United Launch Alliance (ULA) Atlas V rocket carrying the MUOS-5  mission lifts off from Space Launch Complex-41 at 10:30 a.m. EDT.  Credit:  United Launch Alliance
A United Launch Alliance (ULA) Atlas V rocket carrying the MUOS-5 mission lifts off from Space Launch Complex-41 at 10:30 a.m. EDT on June 24, 2016. Credit: United Launch Alliance

Today’s (June 24) spectacular launch of the most powerful version of the venerable Atlas V rocket from the sunshine state completes the orbital deployment of a constellation of advanced tactical communications satellites for the U.S. Navy.

A United Launch Alliance (ULA) Atlas V rocket successfully launched the massive MUOS-5 satellite into clear blue skies from Space Launch Complex-41 on Cape Canaveral Air Force Station, Florida, at 10:30 a.m. EDT – on its way to a geosynchronous orbit location approximately 22,000 miles (37,586 km) above the Earth.

Note: Check back again for an expanding gallery of launch photos and videos

The Mobile User Objective System-5 (MUOS-5) satellite is the last in a five-satellite constellation that will provide military forces with significantly improved and assured communications worldwide. Lockheed Martin is the prime contractor for the MUOS system.

As launch time neared the weather odds improved to 100% GO and Atlas rumbled off the pad for on time launch that took place at the opening of a 44 minute window.

The launch was broadcast live on a ULA webcast.

The 206 foot tall Atlas rocket roared to space on an expanding plume of smoke and crackling fire from the first stage liquid and solid fueled engines generating over 2.5 million pounds of liftoff thrust.

Their contribution complete, all 5 solid rocket motors were jettisoned with seconds about 2 minutes after liftoff as the liquid fueled first stage continued firing.

The spent first stage separated about 5 minutes after liftoff, as the Centaur second stage fires up for the first of three times over almost three hours to deliver the hefty payload to orbit.

Blastoff of United Launch Alliance (ULA) Atlas V rocket on MUOS-5  mission from Space Launch Complex-41 on June 24, 2016.  Credit: Lane Hermann
Blastoff of United Launch Alliance (ULA) Atlas V rocket on MUOS-5 mission from Space Launch Complex-41 on June 24, 2016. Credit: Lane Hermann

“We are honored to deliver the final satellite in the MUOS constellation for the U.S. Navy,” said Laura Maginnis, ULA vice president, Custom Services, in a statement.

“Congratulations to our navy, air force and Lockheed Martin mission partners on yet another successful launch that provides our warfighters with enhanced communications capabilities to safely and effectively conduct their missions around the globe.”

This is the fifth satellite in the MUOS series and will provide military users up to 16 times more communications capability over existing systems, including simultaneous voice, video and data, leveraging 3G mobile communications technology.

Long plume from MUOS-5 Atlas V Launch by United Launch Alliance from Space Launch Complex-41 on June 24, 2016.  Credit: Michael Seeley
Long plume from MUOS-5 Atlas V Launch by United Launch Alliance from Space Launch Complex-41 on June 24, 2016. Credit: Michael Seeley

With MUOS-5 in orbit the system’s constellation is completed.

MUOS-5 will serve as an on orbit spare. It provides the MUOS network with near-global coverage. Communications coverage for military forces now extends further toward the North and South poles than ever before, according to Lockheed Martin officials.

“Like its predecessors, the MUOS-5 satellite has two payloads to support both new Wideband Code Division Multiple Access (WCDMA) waveform capabilities, as well as the legacy Ultra High Frequency (UHF) satellite system. On orbit, MUOS-5 will augment the constellation as a WCDMA spare, while actively supporting the legacy UHF system, currently used by many mobile forces today.”

The prior MUOS-4 satellite was launched on Sept. 2, 2015 – as I reported here.

The 20 story tall Atlas V launched in its most powerful 551 configuration and performed flawlessly.

United Launch Alliance (ULA) Atlas V rocket carrying MUOS-5 military comsat streaks to orbit atop a vast exhaust plume after liftoff from Space Launch Complex-41 on June 24, 2016.  Credit: Jillian Laudick
United Launch Alliance (ULA) Atlas V rocket carrying MUOS-5 military comsat streaks to orbit atop a vast exhaust plume after liftoff from Space Launch Complex-41 on June 24, 2016. Credit: Jillian Laudick

The vehicle includes a 5-meter diameter payload fairing and five solid rocket boosters that augment the first stage. The Atlas booster for this mission was powered by the RD AMROSS RD-180 engine and the Centaur upper stage was powered by the Aerojet Rocketdyne RL10C-1 engine.

The RD-180 burns RP-1 (Rocket Propellant-1 or highly purified kerosene) and liquid oxygen and delivers 860,200 lb of thrust at sea level.

And the rocket needed all that thrust because the huge MUOS-5 was among the heftiest payloads ever lofted by an Atlas V booster, weighing in at some 15,000 pounds.
The Centaur upper stage was fired a total of three times.

For this mission the payload fairing was outfitted with an upgraded and advanced acoustic system to beet shield the satellite from the intense vibrations during the launch sequence.

This Atlas launch had been delayed several months to rectify a shortfall in the first stage thrust that occurred during the prior mission launching the Orbital ATK OA-6 cargo freighter in March 2016 on a contract mission for NASA to resupply the International Space Station (ISS).

The launch comes just two weeks after blastoff of the ULA Delta IV Heavy, the worlds most powerful rocket, on a mission to deliver a top secret spy satellite to orbit – as I witnessed and reported on here.

“I am so proud of the team for all their hard work and commitment to 100 percent mission success,” Maginnis added.

“It is amazing to deliver our second national security payload from the Cape in just two weeks. I know this success is due to our amazing people who make the remarkable look routine.”

The 15,000 pound MUOS payload is a next-generation narrowband tactical satellite communications system designed to significantly improve ground communications for U.S. forces on the move.

Here’s a detailed mission profile video describing the launch events:

Video caption: Atlas V MUOS-5 Mission Profile launched on June 24, 2016 from Cape Canaveral Air force Station. Credit: ULA

The launch was supported by the 45th Space Wing.

“Today’s successful launch is the culmination of the 45th Space Wing, Space and Missile Systems Center, Navy and ULA’s close partnership and dedicated teamwork,” said Brig. Gen. Wayne Monteith, 45th Space Wing commander and mission Launch Decision Authority, in a statement.

“We continue our unwavering focus on mission success and guaranteeing assured access to space for our nation, while showcasing why the 45th Space Wing is the ‘World’s Premiere Gateway to Space.”

Watch this exciting launch highlights video reel from ULA – including deployment of MUOS-5!

The MUOS-5 launch marked the 63rd Atlas V mission since the vehicle’s inaugural launch in August 2002. To date seven flights have launched in the 551 configuration. These include all four prior MUOS missions as well as NASA’s New Horizons mission to Pluto and the Juno mission to Jupiter.

Watch my up close remote launch video from the pad with hurling rocks:

Video caption: The sounds and fury of a ULA Atlas V 551 rocket blast off carrying Lockheed Martin built MUOS-5 tactical communications satellite to geosynchronous orbit for US Navy on June 24, 2016 at 10:30 a.m. EDT from Space Launch Complex 41 at Cape Canaveral Air Force Station, Fl, as seen in this up close video from remote camera positioned at pad. Credit: Ken Kremer/kenkremer.com

Watch this compilation of dramatic launch videos from Jeff Seibert.

Video Caption: MUOS-5 launch compilation on ULA Atlas 5 rocket on 6/24/2016 from Pad 41 of CCAFS. Credit: Jeff Seibert

The Navy's fifth Mobile User Objective System (MUOS) is encapsulated inside an Atlas V five-meter diameter payload fairing.  Credit: ULA
The Navy’s fifth Mobile User Objective System (MUOS) is encapsulated inside an Atlas V five-meter diameter payload fairing. Credit: ULA

The next Atlas V launch is slated for July 28 with the NROL-61 mission for the National Reconnaissance Office (NRO).

Blastoff of MUOS-4 US Navy communications satellite on United Launch Alliance Atlas V rocket from pad 41 at Cape Canaveral Air Force Station, FL on Sept. 2, 2015. Credit: Ken Kremer/kenkremer.com
Blastoff of MUOS-4 US Navy communications satellite on United Launch Alliance Atlas V rocket from pad 41 at Cape Canaveral Air Force Station, FL on Sept. 2, 2015. Credit: Ken Kremer/kenkremer.com

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

United Launch Alliance (ULA) Atlas V rocket poised for launch on MUOS-5  mission from Space Launch Complex-41 on June 24, 2016.  Credit: Lane Hermann
United Launch Alliance (ULA) Atlas V rocket poised for launch on MUOS-5 mission from Space Launch Complex-41 on June 24, 2016. Credit: Lane Hermann
Artist’s concept of a MUOS satellite in orbit. Credit: Lockheed Martin
Artist’s concept of a MUOS satellite in orbit. Credit: Lockheed Martin
MUOS-5 mission logo. Credit: ULA
MUOS-5 mission logo. Credit: ULA
A United Launch Alliance (ULA) Atlas V rocket carrying the MUOS-5  mission lifts off from Space Launch Complex-41 at 10:30 a.m. EDT on June 24, 2016.  Credit:  United Launch Alliance
A United Launch Alliance (ULA) Atlas V rocket carrying the MUOS-5 mission lifts off from Space Launch Complex-41 at 10:30 a.m. EDT on June 24, 2016. Credit: United Launch Alliance

Antares Return to Flight Launch Likely Slips to August, Cygnus Completes Atmospheric Reentry

Antares rocket stands erect, reflecting off the calm waters the night before a launch from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer/kenkremer.com
Antares rocket stands erect, reflecting off the calm waters the night before the first night launch from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014.    Credit: Ken Kremer/kenkremer.com
Antares rocket stands erect, reflecting off the calm waters the night before the first night launch from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer/kenkremer.com

The long awaited maiden launch of Orbital ATK’s revamped Antares commercial rocket utilizing new first stage engines, from its Virginia launch base, will likely slip from July to August a company spokesperson confirmed to Universe Today.

The target date for the ‘Return to Flight’ launch of Antares on a cargo resupply mission for NASA to the International Space Station (ISS) is “likely to result in an updated launch schedule in the August timeframe,” Orbital ATK spokeswoman Sean Wilson told Universe Today.

The company had most recently been aiming towards an Antares launch date around July 6 from NASA’s Wallops Flight Facility – for its next NASA contracted mission to stock the ISS via the Orbital ATK Cygnus cargo freighter on a flight known as OA-5.

Meanwhile the firms most recently launched Cygnus OA-6 cargo ship departed the space station and completed its planned destructive reentry into the Earth’s atmosphere on Wednesday, June 22.

But before Orbital ATK can resume Antares/Cygnus cargo flights to the ISS, it had to successfully hurdle through a critically important milestone on the path to orbit – namely a static hot fire test of the significantly modified first stage to confirm that its qualified for launch.

Orbital ATK conducted a full-power test of the upgraded first stage propulsion system of its Antares rocket on May 31, 2016 at Virginia Space’s Mid-Atlantic Regional Spaceport (MARS) Pad 0A.  Credit: NASA/Orbital ATK
Orbital ATK conducted a full-power test of the upgraded first stage propulsion system of its Antares rocket on May 31, 2016 at Virginia Space’s Mid-Atlantic Regional Spaceport (MARS) Pad 0A. Credit: NASA/Orbital ATK

To that end the aerospace firm recently completed a successful 30 second long test firing of the re-engined first stage on May 31 at Virginia Space’s Mid-Atlantic Regional Spaceport (MARS) Launch Pad 0A – as I reported here earlier.

A thorough analysis of the hot fire test results and its implications is underway.

“Our Antares team recently completed a successful stage test and is wrapping up the test data analysis,” Wilson said.

“Final trajectory shaping work is also currently underway, which is likely to result in an updated launch schedule in the August timeframe.”

In the meantime, company engineers continue to ready the rocket and payload.

“We are continuing to prepare for the upcoming launch of the Antares rocket and Cygnus spacecraft for the OA-5 cargo logistics mission to the International Space Station from NASA’s Wallops Flight Facility,” Wilson noted.

It’s also clear that a decision on a launch date target is some weeks away and depends on the busy upcoming manifest of other ISS missions coming and going.

“A final decision on the mission schedule, which takes into account the space station traffic schedule and cargo requirements, will be made in conjunction with NASA in the next several weeks.”

And it also must take into account the launch of the intervening SpaceX ISS cargo flight that was just postponed two days to no earlier than July 18.

Another factor is the delayed launch of the next manned crew on a Russian Soyuz capsule from late June into July. Blastoff of the three person crew from Russia, the US and Japan is set for July 7. OA-5 will deliver some 3 tons of science experiments and crew supplies.

First stage of Orbital ATK Antares rocket outfitted with new RD-181 engines stands erect at Launch Pad-0A on NASA Wallops Flight Facility on May 24, 2016 in preparation for the upcoming May 31 hot fire engine test. Credit:  Ken Kremer/kenkremer.com
First stage of Orbital ATK Antares rocket outfitted with new RD-181 engines stands erect at Launch Pad-0A on NASA Wallops Flight Facility on May 24, 2016 in preparation for the May 31 hot fire engine test. Credit: Ken Kremer/kenkremer.com

Antares launches had immediately ground to a halt following a devastating launch failure 20 months ago which destroyed the rocket and its critical payload of space station science and supplies for NASA in a huge fireball just seconds after blastoff – as witnessed by this author.

As a direct result consequence of the catastrophic launch disaster, Orbital STK managers decided to outfit the Antares medium-class rocket with new first stage RD-181 engines built in Russia.

Base of Orbital Sciences Antares rocket explodes moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. Credit: Ken Kremer – kenkremer.com
Base of Orbital Sciences Antares rocket explodes moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. Credit: Ken Kremer – kenkremer.com

The RD-181 replaces the previously used AJ26 engines which failed moments after liftoff during the last launch on Oct. 28, 2014 resulting in a catastrophic loss of the rocket and Cygnus cargo freighter.

The RD-181 flight engines are built by Energomash in Russia and had to be successfully tested via the static hot fire test to ensure their readiness.

As a result of switching to the new RD-181 engines, the first stage also had to be modified to incorporate new thrust adapter structures, actuators, and propellant feed lines between the engines and core stage structure, Mike Pinkston, Orbital ATK General Manager and Vice President, Antares Program told me in a prior interview.

The new RD-181 engines are installed on the Orbital ATK Antares first stage core ready to support a full power hot fire test at the NASA Wallops Island launch pad in March 2016.  New thrust adapter structures, actuators, and propellant feed lines are incorporated between the engines and core stage.   Credit: Ken Kremer/kenkremer.com
The new RD-181 engines are installed on the Orbital ATK Antares first stage core ready to support a full power hot fire test at the NASA Wallops Island launch pad in March 2016. New thrust adapter structures, actuators, and propellant feed lines are incorporated between the engines and core stage. Credit: Ken Kremer/kenkremer.com

So the primary goal of the stage test was to confirm the effectiveness of the new engines and all the changes in the integrated rocket stage.

It’s not entirely clear at this time whether the Antares launch delay to August is due to changes in the ISS manifest scheduling or any lingering questions from the hot fire test or both.

“A final decision on the mission schedule definitely takes into account the completion of data analysis combined with the busy space station traffic schedule and NASA’s cargo requirements,” Wilson told me in a response requesting clarification.

Following a quick look immediately following the May 31 test, Orbital ATK officials initially reported that all seemed well, with the caveat that further data review is needed.

“Early indications show the upgraded propulsion system, core stage and launch complex all worked together as planned,” said Mike Pinkston, Orbital ATK General Manager and Vice President, Antares Program.

“Congratulations to the combined NASA, Orbital ATK and Virginia Space team on a successful test.”

Orbital ATK engineers will now “review test data over the next several days to confirm that all test parameters were met. ”

The test used the first stage core planned to launch the OA-7 mission from Wallops late this year.

The new RD-181 engines are installed on the Orbital ATK Antares first stage core ready to support a full power hot fire test at the NASA Wallops Island launch pad in March 2016.  Credit: Ken Kremer/kenkremer.com
The new RD-181 engines are installed on the Orbital ATK Antares first stage core ready to support a full power hot fire test at the NASA Wallops Island launch pad in March 2016. Credit: Ken Kremer/kenkremer.com

With the engine test completed, the OA-7 stage will be rolled back to the HIF processing hanger at Wallops and a new stage fully integrated with the Cygnus cargo freighter will be rolled out to the pad for the OA-5 ‘Return to Flight’ mission in August.

The mission of the OA-6 Cygnus ended on Wednesday, with a planned destructive reentry into the Earth’s atmosphere at 9:29 a.m. EDT.

Also known as the SS Rick Husband, it had spent 3 months in orbit since launching in March on a ULA Atlas V.

It departed the ISS on June 14 and continued several science experiments. Most notable was to successfully create the largest fire in space via the Spacecraft Fire Experiment-I (Saffire-I).

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

Pancaked SpaceX Falcon Pulls into Port After Trio of Spectacular Landings; Photos/Videos

Flattened SpaceX Falcon 9 first stage arrived into Port Canaveral, FL atop a droneship late Saturday, June 18 after hard landing and tipping over following successful June 15, 2016 commercial payload launch. Credit: Julian Leek
Flattened SpaceX Falcon 9 first stage arrived into Port Canaveral, FL atop a droneship late Saturday, June 18 after hard landing and tipping over following successful June 15, 2016  commercial payload launch to orbit.  Credit: Julian Leek
Flattened SpaceX Falcon 9 first stage arrived into Port Canaveral, FL atop a droneship late Saturday, June 18 after hard landing and tipping over following successful June 15, 2016 commercial payload launch to orbit. Credit: Julian Leek

CAPE CANAVERAL AIR FORCE STATION, FL — The pancaked leftovers of a SpaceX Falcon 9 first stage from last week’s successful commercial launch but hard landing at sea, pulled silently and without fanfare into its home port over the weekend – thereby ending a string of three straight spectacular and upright soft ocean landings over the past two months.

The residue of the Falcon sailed into home port at Port Canaveral, Fl under cover of darkness and covered by a big blue tarp late Saturday night, June 18, at around 9 p.m. EDT.

It arrived atop SpaceX’s ASDS drone ship landing platform known as “Of Course I Still Love You” or “OCISLY” – that had already been dispatched several days prior to the June 15 morning launch from the Florida space coast.

Pancaked SpaceX Falcon 9 first stage arrived at night into Port Canaveral, FL atop a droneship on June 18 after hard landing at sea following successful June 15, 2016  commercial payload launch to orbit.  Credit: Lane Hermann
Pancaked SpaceX Falcon 9 first stage arrived at night into Port Canaveral, FL atop a droneship on June 18 after hard landing at sea following successful June 15, 2016 commercial payload launch to orbit. Credit: Lane Hermann

And check out this exquisite hi res aerial video of the tarp ‘Blowing in the Wind’ – showing an even more revealing view of the remains of the Falcon 9 after much of the tarp was blown away by whipping sunshine state winds.

Video Caption: SpaceX booster remains from Eutelsat-ABS launch seen in Port Canaveral on 06-19-2016 the day after arrival. The wind blew off part of the tarps covering what is left of Eutelsat-ABS booster. Credit: USLaunchReport

Recovering and eventually reusing the 156 foot tall Falcon 9 first stage to loft new payloads for new paying customers lies at the heart of the visionary SpaceX CEO Elon Musk’s strategy of radically slashing future launch costs and enabling a space faring civilization.

The latest attempt to launch and propulsively land the Falcon booster on a platform a sea took place on Wednesday, June 15 after the on time liftoff at 10:29 a.m. EDT (2:29 UTC) from Space Launch Complex 40 on Cape Canaveral Air Force Station in Florida.

Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com

The 229 foot-tall (70 meter) Falcon 9 successfully accomplished its primary goal of delivering a pair of roughly 5000 pound commercial telecommunications satellites to a Geostationary Transfer Orbit (GTO) for Eutelsat based in Paris and Asia Broadcast Satellite of Bermuda and Hong Kong.

The Falcon 9 delivered the Boeing-built EUTELSAT 117 West B and ABS-2A telecommunications satellites to orbits for Latin American and Asian customers.

“Ascent phase & satellites look good,” SpaceX CEO and founder Elon Musk tweeted.

After first stage separation, SpaceX engineers attempted the secondary and experimental goal of soft landing the 15 story tall first stage booster nine minutes after liftoff, on an ocean going ‘droneship’ platform for later reuse.

OCISLY was stationed approximately 420 miles (680 kilometers) off shore and east of Cape Canaveral, Florida in the Atlantic Ocean.

However, for the first time in four tries SpaceX was not successful in safely landing and recovering the booster intact and upright.

Incredible sight of pleasure craft zooming past SpaceX Falcon 9 booster from Thaicom-8 launch on May 27, 2016 as it arrives at the mouth of Port Canaveral, FL,  atop droneship platform on June 2, 2016.  Credit: Ken Kremer/kenkremer.com
Incredible sight of pleasure craft zooming past SpaceX Falcon 9 booster from Thaicom-8 launch on May 27, 2016 as it arrives at the mouth of Port Canaveral, FL, atop droneship platform on June 2, 2016. Credit: Ken Kremer/kenkremer.com

The booster basically crashed on the drone ship because it descended too quickly due to insufficient thrust from the descent engines.

The rocket apparently ran out of fuel in the final moments before droneship touchdown.

“Looks like early liquid oxygen depletion caused engine shutdown just above the deck,” Musk explained via a twitter post.

The first stage is fueled by liquid oxygen and RP-1 propellant.

Flattened SpaceX Falcon 9 first stage arrived into Port Canaveral, FL atop a droneship late Saturday, June 18 after hard landing and tipping over following successful June 15, 2016  commercial payload launch.  Credit: Julian Leek
Flattened SpaceX Falcon 9 first stage arrived into Port Canaveral, FL atop a droneship late Saturday, June 18 after hard landing and tipping over following successful June 15, 2016 commercial payload launch to orbit. Credit: Julian Leek

A SpaceX video shows a huge cloud of black smoke enveloping the booster in the final moments before the planned touchdown – perhaps soot from the burning RP-1 propellant.

In the final moments the booster is seen tipping over and crashing with unrestrained force onto the droneship deck – crushing and flattening the boosters long round core and probably the nine Merlin 1D first stage engines as well.

“But booster rocket had a RUD on droneship,” Musk noted. RUD stands for rapid unscheduled disassembly which usually means it was destroyed on impact. Although in this case it may be more a case of being crushed by the fall instead of a fuel related explosion.

“Looks like thrust was low on 1 of 3 landing engines. High g landings v sensitive to all engines operating at max,” Musk elaborated.

SpaceX Falocn 9 streaks to orbit across the Florida skies after Eutelsat/ABS 2A comsat  launch  on June 15, 2016 from Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
SpaceX Falocn 9 streaks to orbit across the Florida skies after Eutelsat/ABS 2A comsat launch on June 15, 2016 from Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com

The June 15 crash follows three straight landing successes at sea – on April 8, May 6 and mostly recently on May 27 after the Thaicom-8 launch. See my onsite coverage here of the Thaicom-8 boosters return to Port Canaveral on the OCISLY droneship.

Yet this outcome was also not unexpected due to the high energy of the rocket required to deliver the primary payload to the GTO orbit.

“As mentioned at the beginning of the year, I’m expecting ~70% success rate on landings for the year,” Musk explains.

And keep in mind that the rocket recovery and recycling effort is truly a science experiment on a grand scale financed by SpaceX – and its aiming for huge dividends down the road.

“2016 is the year of experimentation.”

It’s a road that Musk hopes will one day lead to a human “City on Mars.”

Pancaked SpaceX Falcon 9 first stage arrived at night into Port Canaveral, FL atop a droneship on June 18 after hard landing at sea following successful June 15, 2016  commercial payload launch to orbit.  Credit: Lane Hermann
Pancaked SpaceX Falcon 9 first stage arrived at night into Port Canaveral, FL atop a droneship on June 18 after hard landing at sea following successful June 15, 2016 commercial payload launch to orbit. Credit: Lane Hermann

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Watch these incredible launch videos showing many different vantage points:

Video caption: SpaceX Falcon 9 launch video compilation – Eutelsat and ABS satellites launched on 06/15/2016 from Pad 40 CCAFS. Credit: Jeff Seibert

Video caption: SpaceX Falcon 9 lifts off with Eutelsat 117W/ABS-2A electric propulsion comsats on June 15, 2016 at 10:29 p.m. EDT from Space Launch Complex 40 at Cape Canaveral Air Force Station, Fl, as seen in this up close video from Mobius remote camera positioned at pad. Credit: Ken Kremer/kenkremer.com

Xenon Propulsion Pair of Telecom Satellites Roars Skyward from SpaceX’s Sunshine State Launch Base – Gallery

Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com
Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com

CAPE CANAVERAL AIR FORCE STATION, FL — Nearly perfect weather greeted the blastoff of a nearly identical pair of xenon propulsion commercial telecom satellites carried to orbit today, Wednesday, June 15, by an upgraded SpaceX Falcon 9 rocket from the Florida space coast.

The secondary and experimental goal of soft landing the first stage booster on an ocean going platform for later reuse was not successful – but also not unexpected due to the high energy of the rocket required to deliver the primary payload to orbit.

Note: check out the expanding gallery of launch photos and videos from my space colleagues and myself.

Liftoff of the 229 foot tall SpaceX Falcon 9 took place at the opening of Wednesday’s launch window at 10:29 a.m. EDT (2:29 UTC) under mostly sunny skies with scattered clouds, thrilling crowds along the beaches and around the coastal areas.

Wednesday’s blastoff came just 4 days after this weekends (June 11) launch from the Cape of the world’s most powerful rocket – the Delta 4 Heavy – which delivered a huge spy satellite to orbit for the NRO in support of US national defense.

Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
Successful SpaceX Falcon 9 launch of ABS/Eutelsat-2 launch on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com

The goal of the launch was to deliver the Boeing-built EUTELSAT 117 West B and ABS-2A satellites to orbits for Latin American and Asian customers.

“Ascent phase & satellites look good,” SpaceX CEO and founder Elon Musk tweeted.

However the 156 foot tall first stage booster descended too quickly due to insufficient thrust from the descent engines and crashed on the droneship.

“But booster rocket had a RUD on droneship,” Musk noted. RUD stand for rapid unscheduled disassembly” which means it exploded on impact.

“Looks like thrust was low on 1 of 3 landing engines. High g landings v sensitive to all engines operating at max,” Musk elaborated.

The crash follows three straight landing successes – mostly recently on May 27. See my onsite coverage here of the boosters return to Port Canaveral on the ICISLY droneship.

Launch of SpaceX Falcon 9 with Eutelsat/ABS 2A on June 15, 2016 from Cape Canaveral Air Force Station, Fl.   Credit: Julian Leek
Launch of SpaceX Falcon 9 with Eutelsat/ABS 2A on June 15, 2016 from Cape Canaveral Air Force Station, Fl. Credit: Julian Leek

The satellites are based on Boeing’s 702SP series program and were the first all-electric propulsion satellites when Boeing introduced it in 2012, a Boeing spokesperson Joanna Climer told Universe Today.

Liftoff occurred from Space Launch Complex 40 on Cape Canaveral Air Force Station in Florida on time at 10:29 a.m. EDT (2:29 UTC).

The crackling roar of 1.5 million pounds of thrust generated by nine Merlin 1 D engines was so load that even spectators watching some 20 miles away in Titusville, Fl heard it load and clear – eager onlookers told me with a smile of delight !

Folks enthusiastically shared experiences upon returning from my press site viewing area located less than 2 miles away from the launch pad !

Launch of SpaceX Falcon 9 with Eutelsat/ABS 2A on June 15, 2016 from Cape Canaveral Air Force Station, Fl.   Credit: Julian Leek
Launch of SpaceX Falcon 9 with Eutelsat/ABS 2A on June 15, 2016 from Cape Canaveral Air Force Station, Fl. Credit: Julian Leek

The Falcon 9 launch was carried live on a SpaceX webcast that started about 20 minutes before liftoff, at approximately 10:09 a.m. EDT at SpaceX.com/webcast

The webcast offered a detailed play by play of launch events and exquisite live views from the ground and extraordinary views of many key events of the launch in progress from the rocket itself from side mounted cameras looking up into space and back down to the ground.

SpaceX Falcon 9 blasts off carrying ABS/Eutelsat-2 satellites on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
SpaceX Falcon 9 blasts off carrying ABS/Eutelsat-2 satellites on June 15, 2016, at 10:29 a.m. EDT from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com

Falcon 9 delivered the roughly 5000 pound commercial telecommunications satellites to a Geostationary Transfer Orbit (GTO) for Eutelsat based in Paris and Asia Broadcast Satellite of Bermuda and Hong Kong.

They were deployed at about 30 minutes and 35 minutes after liftoff.

Eutelsat 117 West B will provide Latin America with video, data, government and mobile services for Paris-based Eutelsat.

ABS 2A will distribute direct-to-home television, mobile and maritime communications services across Russia, India, the Middle East, Africa, Southeast Asia and the Indian Ocean region for Asia Broadcast Satellite of Bermuda and Hong Kong.

There are only minor differences between the two satellites. They were vertically stacked for launch and encased inside the Falcon 9 nose cone, or payload fairing using a Boeing-patented and customized interface configuration – as seen in the photo herein.

The telecom sats are “very similar, but not identical,” Climer told Universe Today.

Two Boeing built satellies named Eutelsat SA 117 West B and ABS 2A are due to launch on June 15, 2015 atop a SpaceX Falcon 9 rocket  from Cape Canaveral, FL. Credit: SpaceX
Two Boeing built satellies named Eutelsat SA 117 West B and ABS 2A are due to launch on June 15, 2015 atop a SpaceX Falcon 9 rocket from Cape Canaveral, FL. Credit: SpaceX

“They vary slightly in mass, but have similar payload power. The satellite on top weighs less than the one on the bottom.”

They were tested at the Boeing Satellite Development Center in El Segundo, Calif., to ensure they could withstand the rigors of the launch environment. They have a design lifetime of a minimum of 15 years.

The satellites have no chemical thrusters. They will maneuver to their intended orbit entirely using a use xenon-based electric thruster propulsion system known as XIPS.
XIPS stands for xenon-ion propulsion system.

By using xenon electric propulsion thrusters, Boeing was able to save a lot of weight in their manufacture. This also enabled the satellites to fly together, in tandem rather than on two separate launches and at a much cheaper price to Eutelsat and ABS.

“XIPS uses the impulse generated by a thruster ejecting electrically charged particles at high velocities. XIPS requires only one propellant, xenon, and does not require any chemical propellant to generate thrust,” according to Boeing officials.

“XIPS is used for orbit raising and station-keeping for the 702SP series.”

Watch these incredible launch videos showing many different vantage points:

Close up view of the top umbilicals during the launch of the Eutelsat and ABS satellites on June 15, 2016 on SpaceX Falcon 9 booster #26 from Pad 40 of CCAFS. Credit: Jeff Seibert

Video Caption: SpaceX launch of Eutelsat and ABS Launch on 15 June 2016. Credit: USLaunchReport

Video caption: SpaceX Falcon 9 lifts off with Eutelsat 117W/ABS-2A electric propulsion comsats on June 15, 2016 at 10:29 p.m. EDT from Space Launch Complex 40 at Cape Canaveral Air Force Station, Fl, as seen in this up close video from Mobius remote camera positioned at pad. Credit: Ken Kremer/kenkremer.com

Wednesday’s launch was the sixth of this year for SpaceX.

Later this year, SpaceX hopes to relaunch one of the recovered first stage boosters that’s seems fit to fly.

Two others which landed harder will be used for long life testing.

One of my very attentive readers, Marie Bieniek, apparently spotted one of the recovered boosters being trucked back on US 19 North of Crystal River, Fl earlier this week, headed for SpaceX facilities possibly in Texas or California.

She was just driving along the Florida roads on Rt. 19 on Monday, Jun 13 when suddenly a Falcon appeared at about 11 AM! She kindly alerted me – so see her photo below.

An apparent SpaceX Falcon 9 recovered booster is spotted on US 19 North of Crystal River, Fl on June 13, 2016. Credit: Marie Bieniek
An apparent SpaceX Falcon 9 recovered booster is spotted on US 19 North of Crystal River, Fl on June 13, 2016. Credit: Marie Bieniek

The SpaceX rockets and recovery technology are all being developed so they will one day lead to establishing a ‘City on Mars’ – according to the SpaceX’s visionary CEO and founder Elon Musk.

Musk aims to radically slash the cost of launching future rockets by recycling them and using them to launch new payloads for new paying customers.

SpaceX Falocn 9 streaks to orbit across the Florida skies after Eutelsat/ABS 2A comsat  launch  on June 15, 2016 from Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
SpaceX Falocn 9 streaks to orbit across the Florida skies after Eutelsat/ABS 2A comsat launch on June 15, 2016 from Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com

Watch for Ken’s continuing on site reports direct from Cape Canaveral Air Force Station and the SpaceX launch pad.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer

Up close view of nose cone carrying two comsats atop SpaceX Falcon 9 that launched on June 15, 2016 from Cape Canaveral Air Force Station, Fl.   Credit: Lane Hermann
Up close view of nose cone carrying two comsats atop SpaceX Falcon 9 that launched on June 15, 2016 from Cape Canaveral Air Force Station, Fl. Credit: Lane Hermann
Predawn view of SpaceX Falcon 9 and Eutelsat/ABS 2A comsats pn the morning of launch on June 15, 2016 from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
Predawn view of SpaceX Falcon 9 and Eutelsat/ABS 2A comsats pn the morning of launch on June 15, 2016 from Space Launch Complex 40 on Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com
Up close view of nose cone carrying Eutelsat/ABS 2A comsats atop SpaceX Falcon 9 that launched on June 15, 2016 from Cape Canaveral Air Force Station, Fl.   Credit: Ken Kremer/kenkremer.com
Up close view of nose cone carrying Eutelsat/ABS 2A comsats atop SpaceX Falcon 9 that launched on June 15, 2016 from Cape Canaveral Air Force Station, Fl. Credit: Ken Kremer/kenkremer.com
Diagram of the Xenon propulsion system aboard the Boeing-built EUTELSAT 117 West B and ABS-2A satellites.  Credit: Boeing
Diagram of the Xenon propulsion system aboard the Boeing-built EUTELSAT 117 West B and ABS-2A satellites. Credit: Boeing

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Learn more about ULA Atlas and Delta rockets, SpaceX Falcon 9 rocket, Orbital ATK Cygnus, ISS, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:

June 16: “SpaceX launches, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

Logo for EUTELSAT 117 West B and ABS-2A satellite mission launch. Credit: SpaceX
Logo for EUTELSAT 117 West B and ABS-2A satellite mission launch. Credit: SpaceX