Bound for Bennu, OSIRIS-REx Begins Trailblazing Asteroid Sampling Sortie for Life’s Origins – Sunset Launch Gallery

United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study. Liftoff was at 7:05 p.m. EDT on September 8, 2016 in this remote camera view taken from inside the launch pad perimeter. Note the newly install crew access arm and white room for astronaut flights atop Atlas starting in early 2018. Credit: Ken Kremer/kenkremer.com
United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study.  Liftoff was at 7:05 p.m. EDT on September 8, 2016 in this remote camera view taken from inside the launch pad perimeter.  Note the newly install crew access arm and white room for astronaut flights atop Atlas starting in early 2018.   Credit: Ken Kremer/kenkremer.com
United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study. Liftoff was at 7:05 p.m. EDT on September 8, 2016 in this remote camera view taken from inside the launch pad perimeter. Note the newly installed crew access arm and white room for astronaut flights atop Atlas starting in early 2018. Credit: Ken Kremer/kenkremer.com

KENNEDY SPACE CENTER, FL – Bound for Bennu, NASA’s OSIRIS-REx robotic explorer began a trailblazing 7 year round trip sampling sortie on Sept. 8 in search of the origin of life with a spectacular sky show – thrilling spectators ringing the Florida Space Coast.

Hordes of space enthusiasts from all across the globe descended on the Kennedy Space Center and Cape Canaveral region for the chance of a lifetime to witness a once in a lifetime liftoff to the carbon rich asteroid – which could potentially bring back samples infused with the organic chemicals like amino acids that are the building blocks of life as we know it.

NASA’s Origins, Spectral Interpretation, Resource Identification, Security – Regolith Explorer (OSIRIS-REx) spacecraft departed Earth with an on time engine ignition of a United Launch Alliance Atlas V rocket under crystal clear skies on Thursday, September 8 at 7:05 p.m. EDT from Space Launch Complex 41 at Cape Canaveral Air Force Station.

Blastoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach.  Credit: Jillian Laudick
Blastoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach. Credit: Jillian Laudick

Everything went exactly according to plan for the daring mission bolding seeking to gather rocks and soil from Bennu – using an ingenious robotic arm named TAGSAM – and bring at least a 60-gram (2.1-ounce) sample back to Earth in 2023 for study by scientists using the world’s most advanced research instruments.

“We got everything just exactly perfect,” said Dante Lauretta, the principal investigator for OSIRIS-REx at the University of Arizona, at the post launch briefing at the Kennedy Space Center. “We hit all our milestone within seconds of predicts.

The space rock measures about the size of a small mountain at about a third of a mile in diameter.

And the picture perfect near sunset launch rewarded photographers from near and far with a spectacular series of richly hued photo and video recordings.

So I’ve gathered here a variety of launch imagery from multiple vantage points shot by friends, colleagues and myself – for the enjoyment of readers of Universe Today and Beyond!

Liftoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL.  Credit: Julian Leek
Liftoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL. Credit: Julian Leek

As you’ll see and hear the ULA Atlas V rocket integrated with OSIRIS-Rex on top thundered off the Cape’s pad 41 and shot skyward straight up along an equatorial path into Florida’s sun.

From every vantage point the rocket and its ever expanding vapor trail were visible for some 4 or 5 minutes or more. From my location on the roof of NASA’s Vehicle Assembly Building (VAB) the rocket finally arched over nearly straight above us and the sun produced a magnificent thin and nearly straight shadow of the vapor trail on the ground running out to the Atlantic Ocean towards Africa.

Blastoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach.  Credit: John Kraus
Blastoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach. Credit: John Kraus

It was truly an unforgettable sight to behold. And folks at Playalinda Beach, the best public viewing spot just a few miles north of pad 40 had an uninhibited view of the rocket to the base of the pad – while they waded and swam in the oceans waters with waves crashing on shore as the Atlas rocket blasted to space.

OSIRIS-REx separated as planned from the Atlas V rockets liquid oxygen and liquid hydrogen fueled second stage rocket to fly free at 8:04 p.m. on Sept. 8 – 55 minutes after launch.

The pair of solar arrays deployed as planned to provide the probes life giving power.

The spacecraft was built by prime contractor Lockheed.

“The spacecraft is healthy and functioning properly,” Richard Kuhns, Lockheed Martin OSIRIS-REx program manager, told me in an interview at the post-launch briefing.

Members of the OSIRIS-REx mission team celebrate the successful spacecraft launch on Sept. 8, 2016 atop ULA Atlas V at the post-launch briefing at the Kennedy Space Center, FL. Principal Investigator Dante Lauretta is 4th from right,  NASA Planetary Science Director Jim Green is center, 5th from left. Credit: Ken Kremer/kenkremer.com
Members of the OSIRIS-REx mission team celebrate the successful spacecraft launch on Sept. 8, 2016 atop ULA Atlas V at the post-launch briefing at the Kennedy Space Center, FL. Principal Investigator Dante Lauretta is 4th from right, NASA Planetary Science Director Jim Green is center, 5th from left. Richard Kuhns, Lockheed Martin OSIRIS-REx program manager, 2nd from right. Credit: Ken Kremer/kenkremer.com

“The primary objective of the OSIRIS-Rex mission is to bring back pristine material from the surface of the carbonaceous asteroid Bennu, OSIRIS-Rex Principal Investigator Dante Lauretta told Universe Today in a prelaunch interview in the KSC cleanroom with the spacecraft as the probe was undergoing final preparations for shipment to the launch pad.

“We are interested in that material because it is a time capsule from the earliest stages of solar system formation.”

“It records the very first material that formed from the earliest stages of solar system formation. And we are really interested in the evolution of carbon during that phase. Particularly the key prebiotic molecules like amino acids, nucleic acids, phosphates and sugars that build up. These are basically the biomolecules for all of life.”

The asteroid is 1,614-foot (500 m) in diameter and crosses Earth’s orbit around the sun every six years.

After a two year flight through space, including an Earth swing by for a gravity assisted speed boost in 2017, OSIRIS-REx will reach Bennu in Fall 2018 to begin about 2 years of study in orbit to determine the physical and chemical properties of the asteroid in extremely high resolution.

While orbiting Bennu starting in 2018 it will move in close to explore the asteroid for about two years with its suite of science instruments, scanning in visible and infrared light. After a thorough site selection, it will move carefully towards the surface and extend the 11 foot long TAGSAM robotic arm and snatch pristine soil samples containing organic materials from the surface using the TAGSAM collection dish over just 3 to 5 seconds.

Once a good sample collection is confirmed, the dish will then be placed inside the Earth return canister and be brought back to Earth for study by researchers using all of the most sophisticated science instruments available to humankind.

Using the 11 foot long TAGSAM robotic arm that functions somewhat like a pogo stick, OSIRIS-REx will gather rocks and soil and bring at least a 60-gram (2.1-ounce) sample back to Earth on Sept 24, 2023. It has the capacity to scoop up to about 2 kg or more.

ULA Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s OSIRIS-REx asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL, in this remote camera view taken from inside the launch pad perimeter.  Credit: Ken Kremer/kenkremer.com
ULA Atlas V rocket lifts off on September 8, 2016 from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s OSIRIS-REx asteroid sampling spacecraft, in this remote camera view taken from inside the launch pad perimeter. Credit: Ken Kremer/kenkremer.com

The two stage ULA Atlas V performed flawlessly and delivered OSIRIS-Rex into a hyperbolic trajectory away from Earth.

The 189 foot tall ULA Atlas V rocket launched in the rare 411 configuration for only the 3rd time on this mission – which is the 65th for the Atlas V.

The Atlas 411 vehicle includes a 4-meter diameter large Payload Fairing (PLF) and one solid rocket booster that augments the first stage. The Atlas booster for this mission is powered by the RD AMROSS RD-180 engine and the Centaur upper stage was powered by the Aerojet Rocketdyne RL10A.

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.

The strap on solid delivers approximately 348,500 pounds of thrust.

The Centaur delivers 22, 230 lbf of thrust and burns liquid oxygen and liquid hydrogen.

The solid was jettisoned at 139 seconds after liftoff.

Launch of NASA’s OSIRIS-REx on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from LC-39 Gantry.  Credit: Jen Saxby
Launch of NASA’s OSIRIS-REx on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from LC-39 Gantry. Credit: Jen Saxby

This is ULA’s eighth launch in 2016 and the 111th successful launch since the company was formed in December 2006.

NASA’s OSIRIS-REx blasts off to asteroid Bennu on ULA Atlas V rocket prior on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL, as seen from the VAB roof.  Credit: Lane Hermann/SpaceHeadNews
NASA’s OSIRIS-REx blasts off to asteroid Bennu on ULA Atlas V rocket prior on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL, as seen from the VAB roof. Credit: Lane Hermann/SpaceHeadNews

OSIRIS-REx will return the largest sample from space since the American and Soviet Union’s moon landing missions of the 1970s.

Watch these pair of up close videos (from myself and Jeff Seibert) captured directly at the pad with the sights and sounds of the fury of launch:

Video Caption: ULA Atlas V rocket lifts off on September 8, 2016 from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s OSIRIS-REx asteroid sampling spacecraft, in this remote camera view taken from inside the launch pad perimeter. Credit: Ken Kremer/kenkremer.com

Video Caption: Compilation of my launch videos from the ULA Atlas 5 launch in support of the NASA OSIRIS_REx asteroid sample return mission to the asteroid Bennu (#101955). It was launched on September 8th, 2016 from Pad 41 of CCAFS. It is scheduled to land in UTAH with asteroid samples on September 24, 2023. Credit: Jeff Seibert

OSIRIS-REx is the third mission in NASA’s New Frontiers Program, following New Horizons to Pluto and Juno to Jupiter, which also launched on Atlas V rockets.

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is responsible for overall mission management.

OSIRIS-REx complements NASA’s Asteroid Initiative – including the Asteroid Redirect Mission (ARM) which is a robotic spacecraft mission aimed at capturing a surface boulder from a different near-Earth asteroid and moving it into a stable lunar orbit for eventual up close sample collection by astronauts launched in NASA’s new Orion spacecraft. Orion will launch atop NASA’s new SLS heavy lift booster concurrently under development.

Launch of NASA’s OSIRIS-REx on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from VAB roof.  Credit:  J.Sekora/SEKORAPHOTO
Launch of NASA’s OSIRIS-REx on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from VAB roof. Credit: J.Sekora/SEKORAPHOTO

Watch for Ken’s continuing OSIRIS-REx mission and launch reporting from on site at the Kennedy Space Center and Cape Canaveral Air Force Station, FL.

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

Ken Kremer

NASA’s OSIRIS-Rex asteroid sampling spacecraft streaks to orbit on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach.  Credit: Jillian Laudick
NASA’s OSIRIS-Rex asteroid sampling spacecraft streaks to orbit on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach. Credit: Jillian Laudick
Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com
A United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study.  Liftoff was at 7:05 p.m. EDT on September 8, 2016.  Credit: Ken Kremer/kenkremer.com
A United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study. Liftoff was at 7:05 p.m. EDT on September 8, 2016. Credit: Ken Kremer/kenkremer.com
View of science instrument suite and TAGSAM robotic sample return arm on NASA’s OSIRIS-REx asteroid sampling spacecraft inside the Payloads Hazardous Servicing Facility at NASA's Kennedy Space Center.  Probe is slated for Sep. 8, 2016 launch to asteroid Bennu from Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
View of science instrument suite and TAGSAM robotic sample return arm on NASA’s OSIRIS-REx asteroid sampling spacecraft inside the Payloads Hazardous Servicing Facility at NASA’s Kennedy Space Center. Probe is slated for Sep. 8, 2016 launch to asteroid Bennu from Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

Stunning New Images Of Mars From The Curiosity Rover

Murray formation: rocks laid down by water and sculpted by wind
Finely layered rocks within the "Murray formation" layer of lower Mount Sharp on Mars. Credit: NASA

Since its deployment in 2012 to the surface of Mars, the Curiosity rover has sent back many breathtaking images of the Red Planet. In addition to snapping photos of the comet Siding Spring and Earth from the surface, not to mention some wonderful panoramic selfies, the rover has also taken countless images that show the geology and surface features of Mars’ in stunning detail.

And with the latest photos to be released by NASA, the Curiosity rover has provided us with a wonderful look at the “Murray Buttes” region, which is in the lower part of Mount Sharp. These images were taken by the Curiosity Mast Camera (Mastcam) on Sept. 8th, and provide some lovely insight into the geological history of the region.

Using these images, the Curiosity team hopes to assemble another impressive color mosaic that will give a detailed look at the region’s rocky, desert-like landscape. As you can see from the images provided, the region is characterized by mesas and buttes, which are the eroded remnants of ancient sandstone. Much like other spots around Mount Sharp, the area is of particular interest to the Curiosity team.

Sloping buttes and layered outcrops within the "Murray formation" layer of lower Mount Sharp. Credit: NASA
Sloping buttes and layered outcrops within the “Murray formation” layer of lower Mount Sharp. Credit: NASA

For years, scientists have understood that the rock layers that form the base of Mount Sharp accumulated as a result of sediment being deposited within the ancient lake bed billions of years ago. In this respect, the geological formations are similar to those found in the desert regions of the southwestern United States.

Ashwin Vasavada, the Curiosity Project Scientist of NASA’s Jet Propulsion Laboratory, told Universe Today via email:

” The Murray Buttes region of Mars is reminiscent of parts of the American southwest because of its butte and mesa landscape. In both areas, thick layers of sediment were deposited by wind and water, eventually resulting in a “layer cake” of bedrock that then began to erode away as conditions changed.  In both places, more resistant sandstone layers cap the mesas and buttes because they protect the more easily eroded, fine-grained rock underneath. 

“Like at Monument Valley near the Utah-Arizona border, at Murray Buttes there are just small remnants of these layers that once covered the surface more completely.  There were wind-driven sand dunes at both places, too, that now appear as cross-bedded sandstone layers.  There are of course many differences between Mars and the American Southwest.  For example, there were large inland seas in the Southwest, while at Gale crater there were lakes.”

These sediment layers are believed to have been laid down over the course of 2 billion years, and may have completely filled the crater at one time. Since it is widely believed that lakes and streams existed in the Gale Crater 3.3 – 3.8 billion years ago, some of the lower sediment layers may have originally been deposited on a lake bed.

A hillside outcrop with finely layered rocks within the "Murray formation" layer of lower Mount Sharp. Credit: NASA
A hillside outcrop with finely layered rocks within the “Murray formation” layer of lower Mount Sharp. Credit: NASA

For this reason, the Curiosity team also took drill samples from the Murray Buttes area for analysis. This began on Sept. 9th, after the rover was finished taking pictures of the area. As Vasavada explained:

“The Curiosity team is drilling regularly as the rover ascends Mount Sharp. We are drilling into the fine-grained rock that was deposited within lakes in order to see how the lake chemistry, and therefore the environment, changed over time. Curiosity drilled into the coarser sandstone that forms the upper layers of the buttes when the rover crossed the Naukluft Plateau earlier in 2016.”

After the drilling is completed, Curiosity will continue farther south and higher up Mount Sharp, leaving behind these spectacular formations. These pictures represent Curiosity‘s last stop in the Murray Buttes, where the rover has been spending the past month.

And as of this past September 11th, 2016, Curiosity has been on the planet Mars for a total of 4 years and 36 days (or 1497 Earth days; 1458 sols) since it landed on August 6th, 2012.

One has to wonder how the pareidolia folks are going to interpret these ones. After “seeing” a rat, a lizard, a doughnut, a coffin, and so forth, what’s left? Might I suggest that the top image kind of looks like a statue-column?

Further Reading: NASA – Solar System Exploration

SpaceX Falcon 9 Failure Investigation ‘Most Difficult’ Ever: Musk

Mangled SpaceX Falcon 9 strongback with dangling cables (at right) as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com
Mangled SpaceX Falcon 9 strongback with dangling cables as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com
Mangled SpaceX Falcon 9 strongback with dangling cables (at right) as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com

CAPE CANAVERAL AIR FORCE STATION, FL – More than a week after the catastrophic launch pad explosion that eviscerated a SpaceX Falcon 9 rocket during a fueling test, the bold and burgeoning aerospace firm is still confounded by the “most difficult and complex failure” in its history, and is asking the public for help in nailing down the elusive cause – says SpaceX CEO and Founder Elon Musk in a new series of tweets, that also seeks the public’s help in the complex investigation.

“Turning out to be the most difficult and complex failure we have ever had in 14 years,” Musk tweeted on Friday, Sept. 9 about the disaster that took place without warning on Space Launch Complex-40 at approximately 9:07 a.m. EDT on Cape Canaveral Air Force Station, Fl. on Sept. 1, 2016.

Both the $60 million SpaceX rocket and the $200 million AMOS-6 Israeli commercial communications satellite payload were completely destroyed in a massive fireball that erupted suddenly during a routine and planned pre-launch fueling and engine ignition test at pad 40 on Wednesday morning Sep. 1.

“Still working on the Falcon fireball investigation,” Musk stated.

Check out my new up close photos of launch pad 40 herein – showing dandling cables and pad damage – taken over the past few days during NASA’s OSIRIS-REx launch campaign which successfully soared to space on Sept 8. from the adjacent pad at Space Launch Complex-41.

The rocket failure originated somewhere in the upper stage during fueling test operations at the launch pad for what is known as a hot fire engine ignition test of all nine first stage Merlin 1D engines, said Musk.

However, the countdown dress rehearsal had not yet reached the point of ignition and the Merlin engines were still several minutes away from typically firing for a few seconds as the rocket was to be held down during the pre-planned hot fire test.

“Important to note that this happened during a routine filling operation. Engines were not on and there was no apparent heat source,” Musk elaborated.

Engineers were in the final stages of loading the liquid oxygen (LOX) and RP-1 kerosene propellants that power the Falcon 9 first stage for the static fire test which is a full launch dress rehearsal.

Mangled SpaceX Falcon 9 strongback with dangling cables as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com
Mangled SpaceX Falcon 9 strongback with dangling cables as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com

The explosion mystery and its root causes are apparently so deep that SpaceX is asking the public for help by sending in “any recordings of the event” which may exist, beyond what is already known.

“If you have audio, photos or videos of our anomaly last week, please send to [email protected]. Material may be useful for investigation,” Musk requested by twitter.

Indications of an initial “bang” moments before the calamity are also bewildering investigators.

“Particularly trying to understand the quieter bang sound a few seconds before the fireball goes off. May come from rocket or something else.”

The explosion is also being jointly investigated by multiple US Federal agency’s.

“Support & advice from @NASA, @FAA, @AFPAA & others much appreciated. Please email any recordings of the event to [email protected].”

The incident took place less than two days before the scheduled Falcon 9 launch on Sept. 3.

It also caused extensive damage to the rockets transporter erector, or strongback, that holds the rocket in place until minutes before liftoff, and ground support equipment (GSE) around the pad – as seen in my new photos of the pad taken a week after the explosion.

Dangling cables and gear such as pulley’s and more can clearly be seen to still be present as the strongback remains raised at pad 40. The strongback raises the rocket at the pad and also houses multiple umbilical line for electrical power, purge gases, computer communications and more.

One of the four lightning masts is also visibly burnt and blackened – much like what occurred after the catastrophic Orbital ATK Antares rocket exploded moments after liftoff from a NASA Wallops launch pad on Oct 28, 2014 and witnessed by this author.

Black soot also appears to cover some area of the pads ground support equipment in the new photos.

US Air Force personnel immediately jumped into action to assess the situation, set up roadblocks and look for signs of blast debris and “detect, dispose and render safe any possible explosive threats.”

However SpaceX has not released a full description of the damage to the pad and GSE. It cost approximately $15 Million to repair the Antares pad and flights have not yet resumed – nearly 2 years after that disaster.

Up close view of top of mangled SpaceX Falcon 9 strongback with dangling cables (at right) as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com
Up close view of top of mangled SpaceX Falcon 9 strongback with dangling cables (at right) as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com

The rocket disaster was coincidentally captured as it unfolded in stunning detail in a spectacular up close video recorded by my space journalist colleague at USLaunchReport – shown below.

Here is the full video from my space journalist friend and colleague Mike Wagner of USLaunchReport:

Video Caption: SpaceX – Static Fire Anomaly – AMOS-6 – 09-01-2016. Credit: USLaunchReport

The 229-foot-tall (70-meter) SpaceX Falcon 9 had been slated for an overnight blastoff on Saturday, September 3 at 3 a.m. from pad 40 with the 6 ton AMOS-6 telecommunications satellite valued at some $200 million.

Mangled SpaceX Falcon 9 strongback after prelaunch explosion destroyed the rocket and AMOS-6 payload. Credit: Ken Kremer/kenkremer.com
Mangled SpaceX Falcon 9 strongback after prelaunch explosion destroyed the rocket and AMOS-6 payload. Credit: Ken Kremer/kenkremer.com

The Falcon rocket and AMOS-6 satellite were swiftly consumed in a huge fireball and thunderous blasts accompanied by a vast plume of smoke rising from the wreckage that was visible for many miles around the Florida Space Coast.

“Loss of Falcon vehicle today during propellant fill operation,” Musk tweeted several hours after the launch pad explosion.

“Originated around upper stage oxygen tank. Cause still unknown. More soon.”

Aerial view of pad and strongback damage at SpaceX Launch Complex-40 as seen from the VAB roof on Sept. 8, 2016  after fueling test explosion destroyed the Falcon 9 rocket and AMOS-6 payload at Cape Canaveral Air Force Station, FL on Sept. 1, 2016. Credit: Ken Kremer/kenkremer.com
Aerial view of pad and strongback damage at SpaceX Launch Complex-40 as seen from the VAB roof on Sept. 8, 2016 after fueling test explosion destroyed the Falcon 9 rocket and AMOS-6 payload at Cape Canaveral Air Force Station, FL on Sept. 1, 2016. Credit: Ken Kremer/kenkremer.com

Thankfully there were no injuries to anyone – because the pad is always cleared of all personnel during these types of extremely hazardous launch complex operations.

“The anomaly originated around the upper stage oxygen tank and occurred during propellant loading of the vehicle. Per standard operating procedure, all personnel were clear of the pad and there were no injuries,” SpaceX reported in a statement.

“We are continuing to review the data to identify the root cause. Additional updates will be provided as they become available.”

This also marks the second time a Falcon 9 has exploded in 15 months and will call into question the rocket’s reliability. The first failure involved a catastrophic mid air explosion about two and a half minutes after liftoff, during the Dragon CRS-9 cargo resupply launch for NASA to the International Space Station on June 28, 2015 – and witnessed by this author.

All SpaceX launches are on hold until a thorough investigation is conducted, the root cause is determined, and effective fixes and remedies are identified and instituted.

After the last failure, it took nearly six months before Falcon 9 launches were resumed.

Any announcement of a ‘Return to Flight’ following this latest launch failure is likely to be some time off given the thus far inscrutable nature of the anomaly.

The planned engine test was being conducted as part of routine preparations for the scheduled liftoff of the Falcon 9 on Saturday, September 3, with an Israeli telecommunications satellite that would have also been used by Facebook.

The AMOS-6 communications satellite was built by Israel Aerospace Industries for Space Communication Ltd. It was planned to provide communication services including direct satellite home internet for Africa, the Middle East and Europe.

SpaceX is simultaneously renovating and refurbishing NASA’s former shuttle launch pad at the Kennedy Space Center at Pad 39A – from which the firm hopes to launch the new Falcon Heavy booster as well as human rated launches of the Falcon 9.

SpaceX is renovating Launch Complex 39A at the Kennedy Space Center for launches of the Falcon Heavy and human rated Falcon 9.  Credit: Ken Kremer/kenkremer.com
SpaceX is renovating Launch Complex 39A at the Kennedy Space Center for launches of the Falcon Heavy and human rated Falcon 9. Credit: Ken Kremer/kenkremer.com

Ongoing work at Pad 39A was clearly visible to this author and other media this past week during NASA’s OSIRIS-REx launch campaign.

SpaceX has indicated they hope to have the pad upgrades complete by November, but a lot of work remains to be done. For example the shuttle era Rotating Service Structure (RSS) is still standing. The timing for its demolishment has not been announced.

Damage at  SpaceX Launch Complex-40 following Sept. 1, 2016 launch pad explosion.  Credit: Lane Hermann
Damage at SpaceX Launch Complex-40 following Sept. 1, 2016 launch pad explosion. Credit: Lane Hermann

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

Ken Kremer

Up close view of mangled SpaceX Falcon 9 strongback with dangling cables as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com
Up close view of mangled SpaceX Falcon 9 strongback with dangling cables as seen on Sept. 7 after prelaunch explosion destroyed the rocket and AMOS-6 payload at Space Launch Complex-40 at Cape Canaveral Air Force Station, FL on Sept. 1, 2016 . Credit: Ken Kremer/kenkremer.com
SpaceX Falcon 9 rocket moments after catastrophic explosion destroys the rocket and Amos-6 Israeli satellite payload at launch pad 40 at Cape Canaveral Air Force Station, FL,  on Sept. 1, 2016.  A static hot fire test was planned ahead of scheduled launch on Sept. 3, 2016. Credit: USLaunchReport
SpaceX Falcon 9 rocket moments after catastrophic explosion destroys the rocket and Amos-6 Israeli satellite payload at launch pad 40 at Cape Canaveral Air Force Station, FL, on Sept. 1, 2016. A static hot fire test was planned ahead of scheduled launch on Sept. 3, 2016. Credit: USLaunchReport

Curiosity Rover’s Proximity To Possible Water Raises Planetary Protection Concerns

View from the Curiosity rover at the foot of Aeolis Mons, before the rover starts to climb the mountain. Credit: NASA

After four years on Mars, the Curiosity rover has made some pretty impressive discoveries. These have ranged from characterizing what Mars’ atmosphere was like billions of years ago to discovering organic molecules and methane there today. But arguably the biggest discovery Curiosity has made has been uncovering evidence of warm, flowing water on Mars’ surface.

Unfortunately, now faced with what could be signs of water directly in its path, NASA is forced to enact strict protocols. These signs take the form of dark streaks that have been observed along the sloping terrain of Aeolis Mons (aka. Mount Sharp), which the rover has been preparing to climb. In order to prevent contamination, the rover must avoid any contact with them, which could mean a serious diversion.

These sorts of dark streaks are known as recurring slope lineae (RSLs) because of their tendency to appear, fade away and re­appear seasonally on steep slopes. The first RSLs were reported in 2011 by the Mars Reconnaissance Orbiter in a variety of locations, and are now seen as proof that water still periodically flows on Mars (albiet in the form of salt-water).

Mosaic of the Valles Marineris hemisphere of Mars, similar to what one would see from orbital distance of 2500 km. Credit: NASA/JPL-Caltech
Mosaic of the Valles Marineris hemisphere of Mars, as it would appear from orbit. Credit: NASA/JPL-Caltech

Since that time, a total of 452 possible RSLs have been observed, mostly in Mars’s southern mid-latitudes or near the equator (particularly in Mars’ Valles Marineris). They are generally a few meters wide, and appear to lengthen at the warmest times of the year, then fade during the colder times.

These seasonal flows of salt water are believed to have come from ice trapped about a meter below the surface. Ordinarily, such features would present an opportunity to conduct research. But doing so would cause the water source to be contaminated by Earth microbes aboard Curiosity. And right now, Curiosity has bigger fish to fry (so to speak).

During its planned climb, Curiosity was supposed to pass within a few kilometers of an RSL. However, if NASA determines that the risk is too high, the rover will have to alter its course. Unfortunately, that presents a major challenge, since there is currently only one clear route between Curiosity’s current location and its next destination.

But then again, Curiosity may not have to alter its course at all. Or it could find a route that lets it still accomplish its scientific goals, depending on the circumstances. As Ashwin R. Vasavada, the Project Scientist at the Mars Science Laboratory, told Universe Today via email:

“It may depend on the distance between the rover and a potentially sensitive region, for example.  Based on that understanding, we’ll determine the right course of action. For example, it may be possible to achieve Curiosity’s science goals while maintaining a safe distance. Another possible outcome is that we determine that there are no Recurring Slope Lineae on Mount Sharp.”

MRO image of Gale Crater illustrating the landing location and trek of the Rover Curiosity. In 2 years, Curiosity traversed 3 miles to reach the base of Mount Sharp. The next two years of trekking are likely to be at least as challenging. (Credits: NASA/JPL, illustration, T.Reyes)
MRO image of Gale Crater illustrating the landing location and trek of the Rover Curiosity. Credit: NASA/JPL, illustration, T.Reyes

For years, NASA scientists have been seeking to obtain samples from different locations around Mount Sharp. By studying the sedimentary deposits in the mountainside, the rover’s science team hopes to see how Mars’ environment changed over the past 3 billion years. As Vasavada explained:

“Curiosity’s science mission has focused on understanding whether the area around 5-km high Mount Sharp ever had conditions suitable for life. We’ve already found evidence for an ancient, 3-billion-year-old habitable environment out on the plains around the mountain, and in the lowest levels of the mountain.”

“The geology indicates that a series of lakes once was present in the basin of the crater, before the mountain took shape. Curiosity will continue climbing lower Mount Sharp to see how long these habitable conditions lasted. Every step higher we go, we encounter rocks that are a bit younger, but still around 3 billion years old.”

In the end, the job of determining the risk falls to NASA’s Planetary Protection Office. In addition to reviewing the current predicament, the issue of pre-mission safety standards is also likely to come up. Prior to its deployment to Mars, the Curiosity rover was only partially sterilized, and it is currently unknown how long Earth microbes could survive in the Martian atmosphere, or how far they could be carried in Mars’ atmosphere.

These dark streaks, called recurring slope lineae, are on a sloped wall on a crater on Mars. A new study says they may have been formed by boiling water. Image: NASA/JPL-Caltech/Univ. of Arizona
These dark streaks, called recurring slope lineae (RSL), are on the sloped wall of a crater on Mars. Credit: NASA/JPL-Caltech/Univ. of Arizona

Answering these questions and coming up with new protocols that will address them in advance will come in handy for future missions – particularly the Mars 2020 Rover mission. In the course of its mission, which will include obtaining samples and leaving them behind for possible retrieval by a future crewed mission, the rover is likely to encounter several RSLs.

One of the Mars 2020 rover’s primary tasks will be finding evidence of microbial life, so ensuring that Earth microbes don’t get in the way will be of extreme importance. And with crewed missions on the horizon, knowing how we can prevent contaminating Mars with our own germs (of which there are many) is paramount!

On its currently project path, the Curiosity rover would not get closer than 2 km from the potential RSL (which it is currently 5 km from). And as Vasavada indicated, it is not known at the present time what alternate routes Curiosity could take, or if a diversion in the rover’s path will effect it’s overall mission.

“It’s unclear at this time,” he said. “But I’m optimistic that we can find a solution that protects Mars, allows us to accomplish our mission goals, and even gives us new insight into modern water on Mars, if it is there.”

Further Reading: Nature

OSIRIS-REx Blasts off on 7 Year Sampling Trek to Asteroid Bennu and Back

A United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study. Liftoff was at 7:05 p.m. EDT on September 8, 2016. Credit: Ken Kremer/kenkremer.com
Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study.  Liftoff was at 7:05 p.m. EDT on September 8, 2016.  Credit: Ken Kremer/kenkremer.com
A United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study. Liftoff was at 7:05 p.m. EDT on September 8, 2016. Credit: Ken Kremer/kenkremer.com

KENNEDY SPACE CENTER, FL – NASA’s OSIRIS-REx hi tech robotic explorer blasted off this evening in spectacular fashion from the Florida Space Coast on a ground breaking 7 year sampling trek to Asteroid Bennu and back to gather grains of 4.5 billion year old alien sand that could potentially reveal significant answers to the origins of life on Earth.

The Earth departure for NASA’s Origins, Spectral Interpretation, Resource Identification, Security – Regolith Explorer (OSIRIS-REx) spacecraft began with an on time engine ignition from Space Launch Complex 41 at Cape Canaveral Air Force Station on a United Launch Alliance Atlas V rocket shortly before a crystal clear sunset this evening, Thursday, September 8 at 7:05 p.m. EDT.

The Atlas V rocket with OSIRIS-Rex bolted on top roared off launch pad 41 and shot straight up into the sun drenched skies of the sunshine state.

The launch wowed hordes of excited spectators who gathered from near and far to witness America’s first mission to gather pristine samples of soil and rock from Bennu’s coal black and carbon rich surface – and eventually return them to Earth for analysis using the most powerful science instruments humankind has invented.

A United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study.  Liftoff was at 7:05 p.m. EDT on September 8, 2016.  Credit: Ken Kremer/kenkremer.com
A United Launch Alliance Atlas V rocket lifts off from Space Launch Complex 41 at Cape Canaveral Air Force Station carrying NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-REx spacecraft on the first U.S. mission to sample an asteroid, retrieve at least two ounces of surface material and return it to Earth for study. Liftoff was at 7:05 p.m. EDT on September 8, 2016. Credit: Ken Kremer/kenkremer.com

“This represents the hopes and dreams and blood, sweat and tears of thousands of people who have been working on this for years,” said Dante Lauretta, the principal investigator for OSIRIS-REx at the University of Arizona.

“I can’t tell you how thrilled I was this evening, thinking of the people who played a part in this.”

OSIRIS-Rex is on a totally unique 4.5 billion mile roundtrip mission to unlock the mysteries of the formation of our Solar System 4.5 Billion years ago and ourselves as Earth evolved over time.

“Today, we celebrate a huge milestone for this remarkable mission, and for this mission team,” said NASA Administrator Charles Bolden, in a statement.

“We’re very excited about what this mission can tell us about the origin of our solar system, and we celebrate the bigger picture of science that is helping us make discoveries and accomplish milestones that might have been science fiction yesterday, but are science facts today.”

Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

101955 Bennu is a near Earth asteroid discovered in 1999. It was selected specifically as the sampling because it is a carbon-rich asteroid.

It will take about 2 years for OSIRIS-Rex to reach Bennu in 2018 following a flyby of Earth in 2017.

While orbiting Bennu starting in 2018 it will move in close explore Bennu for about two years with its suite of science instruments. After a thorough site selection, it will move carefully towards the surface and extend the 11 foot long TAGSAM robotic arm and snatch pristine soil samples containing organic materials from the surface using the TAGSAM collection dish. The dish will then be placed inside the Earth return canister and be brought back to Earth for study by researchers using all of the most sophisticated science instruments available to humankind.

The asteroid is 1,614-foot (500 m) in diameter and crosses Earth’s orbit around the sun every six years.

Using the 11 foot long TAGSAM robotic arm that functions somewhat like a pogo stick, OSIRIS-REx will gather rocks and soil and bring at least a 60-gram (2.1-ounce) sample back to Earth in 2023. It has the capacity to scoop up to about 2 kg or more.

Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL.  Credit: Julian Leek
Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL. Credit: Julian Leek

The two stage ULA Atlas V performed flawlessly and delivered OSIRIS-Rex into a hyperbolic trajectory away from Earth.

The 189 foot tall ULA Atlas V rocket launched in the rare 411 configuration for only the 3rd time on this mission – which is the 65th for the Atlas V.

The Atlas 411 vehicle includes a 4-meter diameter large Payload Fairing (PLF) and one solid rocket booster that augments the first stage. The Atlas booster for this mission is powered by the RD AMROSS RD-180 engine and the Centaur upper stage was powered by the Aerojet Rocketdyne RL10A.

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.

The strap on solid delivers approximately 348,500 pounds of thrust.

The Centaur delivers 22,230 lbf of thrust and burns liquid oxygen and liquid hydrogen.

The solid was jettisoned at 139 seconds after liftoff.

This is ULA’s eighth launch in 2016 and the 111th successful launch since the company was formed in December 2006.

Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL.  Credit: Dawn Leek Taylor
Liftoff of NASA’s Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer, or OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL. Credit: Dawn Leek Taylor

OSIRIS-REx will return the largest sample from space since the American and Soviet Union’s moon landing missions of the 1970s.

OSIRIS-REx is the third mission in NASA’s New Frontiers Program, following New Horizons to Pluto and Juno to Jupiter, which also launched on Atlas V rockets.

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is responsible for overall mission management.

OSIRIS-REx complements NASA’s Asteroid Initiative – including the Asteroid Redirect Mission (ARM) which is a robotic spacecraft mission aimed at capturing a surface boulder from a different near-Earth asteroid and moving it into a stable lunar orbit for eventual up close sample collection by astronauts launched in NASA’s new Orion spacecraft. Orion will launch atop NASA’s new SLS heavy lift booster concurrently under development.

Blastoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach.  Credit: Jillian Laudick
Blastoff of NASA’s OSIRIS-Rex asteroid sampling spacecraft on September 8, 2016 from Cape Canaveral Air Force Station, FL as seen from Playalinda Beach. Credit: Jillian Laudick

Watch for Ken’s continuing OSIRIS-REx mission and launch reporting from on site at the Kennedy Space Center and Cape Canaveral Air Force Station, FL.

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

Ken Kremer

NASA’s OSIRIS-REx asteroid sampling spacecraft atop a ULA Atlas V rocket prior to launch on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Lane Hermann/SpaceHeadNews
NASA’s OSIRIS-REx asteroid sampling spacecraft atop a ULA Atlas V rocket prior to launch on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Lane Hermann/SpaceHeadNews
NASA’s OSIRIS-REx asteroid sampling spacecraft is poised for liftoff on a 7 year Journey to asteroid  Bennu and Back atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is poised for liftoff on a 7 year Journey to asteroid Bennu and Back atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com
Artist’s conception of NASA’s OSIRIS-REx sample return spacecraft collecting regolith samples at asteroid Bennu. Credits: NASA/Lockheed Martin
Artist’s conception of NASA’s OSIRIS-REx sample return spacecraft collecting regolith samples at asteroid Bennu. Credits: NASA/Lockheed Martin

Journey to Bennu – Today Sept. 8: Watch the Trailer, Watch the Earth Departure Launch Live

NASA’s OSIRIS-REx asteroid sampling spacecraft is poised for liftoff on a 7 year Journey to asteroid Bennu and Back atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is poised for liftoff on a 7 year Journey to astreroid  Bennu and Back atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is poised for liftoff on a 7 year Journey to asteroid Bennu and Back atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

KENNEDY SPACE CENTER, FL – Today is ‘Earth Departure Day’ for OSIRIS-REx, NASA’s first mission to snatch “pristine materials” from the surface of a near Earth asteroid named Bennu and deliver them back to Earth in seven years on a mission to unlock mysteries on the formation of our Solar System and ourselves 4.5 Billion years ago.

The 4.5 Billion mile roundtrip ‘Journey to Bennu and Back’ begins today. All systems are GO for a spectacular dinner-time blastoff of NASAs OSIRIS-REx spacecraft from the Florida Space Coast.

Earth departure for NASA’s Origins, Spectral Interpretation, Resource Identification, Security – Regolith Explorer (OSIRIS-REx) spacecraft from Space Launch Complex 41 at Cape Canaveral Air Force Station on a United Launch Alliance Atlas V rocket is slated for shortly before sunset this evening, Thursday, September 8 at 7:05 p.m. EDT.

Excited spectators are filling local area hotels for this once in a lifetime mission to ‘Bennu and Back.’

Bennu is a small, carbon-rich asteroid – meaning it contains significant amounts of organic molecules, the stuff of which life is made.

Bennu is only about a third of mile in diameter, measuring 500 meters or 1,614 feet across and it crosses Earth’s orbit around the sun every six years.

You can watch the sure to be a spectacular launch live in person here in sunny Florida or live via a choice of webcasts.

NASA’s OSIRIS-REx launch coverage will be broadcast on NASA TV beginning at 4:30 p.m. EDT Sept. 8, as well as on a ULA webcast.

You can watch the launch live at NASA TV at – http://www.nasa.gov/nasatv

You can watch the launch live at ULA at – www.ulalaunch.com

Today’s weather forecast remains very promising and is currently 80% GO for favorable conditions. The only concern is for cumulus clouds.

There are 3 opportunities in a row to launch OSIRIS-Rex.

In case of a delay 24 or 48 hour delay, the forecast drops only slightly to 70% GO.

Artist’s conception of NASA’s OSIRIS-REx sample return spacecraft collecting regolith samples at asteroid Bennu. Credits: NASA/Lockheed Martin
Artist’s conception of NASA’s OSIRIS-REx sample return spacecraft collecting regolith samples at asteroid Bennu. Credits: NASA/Lockheed Martin

The United Launch Alliance Atlas V rocket and OSIRIS-REx spacecraft were rolled out some 1800 feet from the Vertical Integration Facility (VIF) – where the rocket is assembled- to launch pad 41 starting at about 9 a.m. yesterday morning September 7, 2018.

Watch this OSIRIS-Rex trailer from NASA Goddard illustrating the probes Earth departure launch phase:

NASAs OSIRIS-REx spacecraft is on a mission to explore asteroid Bennu and return a sample to Earth. The OSIRIS-REx launch window opens on September 8, 2016, when the spacecraft begins its two-year journey to Bennu aboard an Atlas V rocket at Cape Canaveral, Florida. After arriving at Bennu in 2018, OSIRIS-REx will spend over a year exploring the asteroid before approaching its surface to grab a sample. This pristine material, formed at the dawn of the solar system, will be returned to Earth in 2023, providing clues to Bennus origins and our own. Credit: NASA’s Goddard Space Flight Center/David Ladd

OSIRIS-REx will gather rocks and soil and bring at least a 60-gram (2.1-ounce) sample back to Earth in 2023. It has the capacity to scoop up to about 2 kg or more.

The mission will help scientists investigate how planets formed and how life began. It will also improve our understanding of asteroids that could impact Earth by measuring the Yarkovsky effect.
Bennu is an unchanged remnant from the collapse of the solar nebula and birth of our solar system some 4.5 billion years ago.

View of science instrument suite and TAGSAM robotic sample return arm on NASA’s OSIRIS-REx asteroid sampling spacecraft inside the Payloads Hazardous Servicing Facility at NASA's Kennedy Space Center.  Probe is slated for Sep. 8, 2016 launch to asteroid Bennu from Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
View of science instrument suite and TAGSAM robotic sample return arm on NASA’s OSIRIS-REx asteroid sampling spacecraft inside the Payloads Hazardous Servicing Facility at NASA’s Kennedy Space Center. Probe is slated for Sep. 8, 2016 launch to asteroid Bennu from Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

It was chosen as the target because it is little altered over time and thus ‘pristine’ in nature.

Bennu is a near-Earth asteroid and was selected for the sample return mission because it could hold clues to the origin of the solar system and host organic molecules that may have seeded life on Earth.

NASA’s OSIRIS-REx asteroid sampling spacecraft is housed inside the payload fairing atop the  United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is housed inside the payload fairing atop the United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

The 189 foot tall ULA Atlas V rocket is launching in the rare 411 configuration for only the 3rd time on this mission – which is the 65th for the Atlas V.

The Atlas 411 vehicle includes a 4-meter diameter payload fairing and one solid rocket booster that augments the first stage. The Atlas booster for this mission is 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.

The strap on solids deliver approximately 500,000 pounds of thrust.

The solids will be jettisoned about 2 minutes after liftoff.

OSIRIS-REx will return the largest sample from space since the American and Soviet Union’s moon landing missions of the 1970s.

OSIRIS-REx is the third mission in NASA’s New Frontiers Program, following New Horizons to Pluto and Juno to Jupiter, which also launched on Atlas V rockets.

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is responsible for overall mission management.

OSIRIS-REx complements NASA’s Asteroid Initiative – including the Asteroid Redirect Mission (ARM) which is a robotic spacecraft mission aimed at capturing a surface boulder from a different near-Earth asteroid and moving it into a stable lunar orbit for eventual up close sample collection by astronauts launched in NASA’s new Orion spacecraft. Orion will launch atop NASA’s new SLS heavy lift booster concurrently under development.

Watch for Ken’s continuing OSIRIS-REx mission and launch reporting from on site at the Kennedy Space Center and Cape Canaveral Ait Force Station, FL.

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

Ken Kremer
………….

Learn more about OSIRIS-REx, InSight Mars lander, SpaceX missions, Juno at Jupiter, SpaceX CRS-9 rocket launch, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:

Sep 8-9: “OSIRIS-REx lainch, SpaceX missions/launches to ISS on CRS-9, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 40 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 40 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft atop a ULA Atlas V rocket prior to planned launch on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Julian Leek
NASA’s OSIRIS-REx asteroid sampling spacecraft atop a ULA Atlas V rocket prior to planned launch on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Julian Leek

OSIRIS-Rex Asteroid Mission Seeks to Search for Origin of Life Chemistry

NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 41 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 41 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 40 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

KENNEDY SPACE CENTER, FL – OSIRIS-Rex, NASA’s first mission to retrieve and return samples of “pristine materials” from the surface of an asteroid and return them to Earth for high powered analysis by the world’s most advanced science instruments is encapsulated in the nose cone that’s bolted atop its Atlas rocket that has just been rolled out to its Earth departure launch pad.

It’s a groundbreaking mission that could inform us about astrobiology and yield significant clues to help determine the ‘Origin of Life’ on Earth.

NASA’s Origins, Spectral Interpretation, Resource Identification, Security – Regolith Explorer (OSIRIS-REx) spacecraft will launch from Space Launch Complex 41 at Cape Canaveral Air Force Station on a United Launch Alliance Atlas V rocket on September 8 at 7:05 p.m. EDT.

The United Launch Alliance Atlas V rocket and OSIRIS-REx spacecraft were moved about 1800 feet from the Vertical Integration Facility (VIF) – where the rocket is assembled- to launch pad 41 starting at about 9 a.m. this morning September 7, 2018.

Watch this Atlas V rocket roll video:

The ULA, NASA and science team conducted a launch readiness review yesterday and gave the GO for launch with all systems passing the stringent rocket and safety review. The even search for signs of any debris from last week’s SpaceX Falcon 9 explosion at the adjacent pad 40 located about a mile south. No signs of any debris or damage were found at pad 40 or the rocket and spacecraft.

NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 40 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft is rolled out to pad 40 for launch atop a United Launch Alliance Atlas V rocket on Sept. 8, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

The weather forecast is currently 80% GO for favorable conditions. The only concern is for cumulus clouds.

There are 3 opportunities in a row to launch OSIRIS-Rex.

In case of a delay 24 or 48 hour delay, the forecast drops only slightly to 70% GO.

NASA’s OSIRIS-REx asteroid sampling spacecraft, return capsule and payload fairings inside the Payloads Hazardous Servicing Facility high bay at NASA's Kennedy Space Center  is being processed for Sep. 8, 2016 launch to asteroid Bennu from Cape Canaveral, FL.  Credit: Ken Kremer/kenkremer.com
NASA’s OSIRIS-REx asteroid sampling spacecraft, return capsule and payload fairings inside the Payloads Hazardous Servicing Facility high bay at NASA’s Kennedy Space Center is being processed for Sep. 8, 2016 launch to asteroid Bennu from Cape Canaveral, FL. Credit: Ken Kremer/kenkremer.com

OSIRIS-REx goal is to fly on a roundtrip seven-year journey of some 4.5 billion miles to the near-Earth asteroid target named Bennu and back.

Watch this mission video:

Video Caption: This video describes the seven-year journey of NASA’s OSIRIS-Rex mission from launch and cruising through space to asteroid Bennu and back. The probe will study Bennu, grab a 2 ounce or more sample from the surface and bring it back to Earth for lab study by researchers. Credit: Lockheed Martin/NASA

101955 Bennu is a near Earth asteroid discovered in 1999. It was selected specifically because it is a carbon-rich asteroid.

While orbiting Bennu starting in 2018 it will move in close and snatch pristine soil samples containing organic materials from the surface using the TAGSAM collection dish, and bring them back to Earth for study by researchers using all of the most sophisticated science instruments available to humankind.

The asteroid is 1,614-foot (500 m) in diameter and crosses Earth’s orbit around the sun every six years.

“The primary objective of the OSIRIS-Rex mission is to bring back pristine material from the surface of the carbonaceous asteroid Bennu, OSIRIS-Rex Principal Investigator Dante Lauretta told Universe Today in the PHSF, as the probe was undergoing final preparation for shipment to the launch pad.

“It records the very first material that formed from the earliest stages of solar system formation. And we are really interested in the evolution of carbon during that phase. Particularly the key prebiotic molecules like amino acids, nucleic acids, phosphates and sugars that build up. These are basically the biomolecules for all of life.”

Artist’s conception of NASA’s OSIRIS-REx sample return spacecraft collecting regolith samples at asteroid Bennu. Credits: NASA/Lockheed Martin
Artist’s conception of NASA’s OSIRIS-REx sample return spacecraft collecting regolith samples at asteroid Bennu. Credits: NASA/Lockheed Martin

OSIRIS-REx will gather rocks and soil and bring at least a 60-gram (2.1-ounce) sample back to Earth in 2023. It has the capacity to scoop up to about 1 kg or more.

The mission will help scientists investigate how planets formed and how life began. It will also improve our understanding of asteroids that could impact Earth by measuring the Yarkovsky effect.
I asked Lauretta to explain in more detail why was Bennu selected as the target to answer fundamental questions related to the origin of life ?

“We selected asteroid Bennu as the target for this mission because we feel it has the best chance of containing those pristine organic compounds from the early stage of solar system formation,” Lauretta told me.

And that information is based on our ground based spectral characterization using telescopes here on Earth. Also, space based assets like the Hubble Space Telescope and the Spitzer Space Telescope.
What is known about the presence of nitrogen containing compounds like amino acids and other elements on Bennu that are the building blocks of life?

“When we look at the compounds that make up these organic materials in these primitive asteroidal materials, we see a lot of carbon,” Lauretta explained.

“But we also see nitrogen, oxygen, hydrogen, sulfur and phosphorous. We call those the CHONPS. Those are the six elements we really focus on when we look at astrobiology and prebiotic chemistry and how those got into the origin of life.”

The OSIRIS-REx spacecraft was built for NASA by prime contractor Lockheed Martin at their facility near Denver, Colorado and flown to the Kennedy Space Center on May 20.

It will map the chemistry and mineralogy of the primitive carbonaceous asteroid. The team will initially select about 10 target areas for further scrutiny as the sampling target. This will be whittled down to two, a primary and backup, Enos told me.

After analyzing the data returned, the science team then will select a site where the spacecraft’s robotic sampling arm will grab a sample of regolith and rocks. The regolith may record the earliest history of our solar system.

Engineers will command the spacecraft to gradually move on closer to the chosen sample site, and then extend the arm to snatch the pristine samples with the TAGSAM sample return arm.

PI Lauretta will make the final decision on when and which site to grab the sample from.

“As the Principal Investigator for the mission I have responsibility for all of the key decisions during our operations,” Lauretta replied. “So we will be deciding on where we want to target our high resolution investigations for sample site evaluation. And ultimately what is the one location we want to send the spacecraft down to the surface of the asteroid to and collect that sample.”

“And then we have to decide like if we collected enough sample and are we ready to stow it in the sample return capsule. Or are we going to use one of our 2 contingency bottles of gas to go for a second attempt.”

“The primary objective is one successful sampling event. So when we collect 60 grams or 2 ounces of sample then we are done!”

“In the event that we decide to collect more, it will be intermixed with anything we collected on the first attempt.”

The priceless sample will then be stowed in the on board sample return capsule for the long journey back to Earth.

Bennu is an unchanged remnant from the collapse of the solar nebula and birth of our solar system some 4.5 billion years ago, little altered over time.

After a 7 year journey to asteroid Bennu and back, NASA’s OSIRIS-Rex sample return capsule  will land by parachute in the Utah desert on Sept. 24, 2023. Credits: NASA/Lockheed Martin
After a 7 year journey to asteroid Bennu and back, NASA’s OSIRIS-Rex sample return capsule will land by parachute in the Utah desert on Sept. 24, 2023. Credits: NASA/Lockheed Martin

Bennu is a near-Earth asteroid and was selected for the sample return mission because it could hold clues to the origin of the solar system and host organic molecules that may have seeded life on Earth.
OSIRIS-REx will return the largest sample from space since the American and Soviet Union’s moon landing missions of the 1970s.

OSIRIS-REx is the third mission in NASA’s New Frontiers Program, following New Horizons to Pluto and Juno to Jupiter, which also launched on Atlas V rockets.

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is responsible for overall mission management.

The OSIRIS-REx spacecraft, enclosed in a payload fairing, is lifted Aug. 29, 2016 at Space Launch Complex 41 at Cape Canaveral Air Force Station in Florida. The United Launch Alliance Atlas V rocket that is to lift OSIRIS-REx into space was stacked at SLC-41 so the spacecraft and fairing could be hoisted up and bolted to the rocket. Photo credit: NASA/Dimitri Gerondidakis
The OSIRIS-REx spacecraft, enclosed in a payload fairing, is lifted Aug. 29, 2016 at Space Launch Complex 41 at Cape Canaveral Air Force Station in Florida. The United Launch Alliance Atlas V rocket that is to lift OSIRIS-REx into space was stacked at SLC-41 so the spacecraft and fairing could be hoisted up and bolted to the rocket. Photo credit: NASA/Dimitri Gerondidakis

OSIRIS-REx complements NASA’s Asteroid Initiative – including the Asteroid Redirect Mission (ARM) which is a robotic spacecraft mission aimed at capturing a surface boulder from a different near-Earth asteroid and moving it into a stable lunar orbit for eventual up close sample collection by astronauts launched in NASA’s new Orion spacecraft. Orion will launch atop NASA’s new SLS heavy lift booster concurrently under development.

Watch for Ken’s continuing OSIRIS-REx mission and launch reporting from on site at the Kennedy Space Center and Cape Canaveral Ait Force Station, FL.

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

Ken Kremer

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Learn more about OSIRIS-REx, InSight Mars lander, SpaceX missions, Juno at Jupiter, SpaceX CRS-9 rocket launch, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:

Sep 7-9: “OSIRIS-REx lainch, SpaceX missions/launches to ISS on CRS-9, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

Dr Dante Lauretta, principal investigator for OSIRIS-REx at the University of Arizona, Tucson, and Dr. Ken Kremer, Universe Today point to NASA’s OSIRIS-REx asteroid sampling spacecraft inside the Payloads Hazardous Servicing Facility at the Kennedy Space Center on Aug. 20, 2016.  Credit: Ken Kremer/kenkremer.com
Dr Dante Lauretta, principal investigator for OSIRIS-REx at the University of Arizona, Tucson, and Dr. Ken Kremer, Universe Today point to NASA’s OSIRIS-REx asteroid sampling spacecraft inside the Payloads Hazardous Servicing Facility at the Kennedy Space Center on Aug. 20, 2016. Credit: Ken Kremer/kenkremer.com

Juno Captures Jupiter’s Enthralling Poles From 2,500 Miles

JunoCam captured this image of Jupiter's north pole region from a distance of 78,000 km (48,000 miles) above the planet.
JunoCam captured this image of Jupiter's north pole region from a distance of 78,000 km (48,000 miles) above the planet.

Juno is sending data from Jupiter back to us, courtesy of the Deep Space Network, and the first images are meeting our hyped-up expectations. On August 27, the Juno spacecraft came within about 4,200 km. (2,500 miles) of Jupiter’s cloud tops. All of Juno’s instruments were active, and along with some high-quality images in visual and infrared, Juno also captured the sound that Jupiter produces.

Juno has captured the first images of Jupiter’s north pole. Beyond their interest as pure, unprecedented eye candy, the images of the pole reveal things never before seen. They show storm activity and weather patterns that are seen nowhere else in our solar system. Even on the other gas giants.

“…like nothing we have seen or imagined before.”

“First glimpse of Jupiter’s north pole, and it looks like nothing we have seen or imagined before,” said Scott Bolton, principal investigator of Juno from the Southwest Research Institute in San Antonio. “It’s bluer in color up there than other parts of the planet, and there are a lot of storms. There is no sign of the latitudinal bands or zone and belts that we are used to — this image is hardly recognizable as Jupiter. We’re seeing signs that the clouds have shadows, possibly indicating that the clouds are at a higher altitude than other features.”

The iconic storm bands of Jupiter are absent in this JunoCam image of Jupiter's northern polar region. Instead, the region is dominated by swirling storm patterns reminiscent of hurricanes here on Earth. Image: NASA/JPL-Caltech/SwRI/MSSS
The iconic storm bands of Jupiter are absent in this JunoCam image of Jupiter’s northern polar region. Instead, the region is dominated by swirling storm patterns reminiscent of hurricanes here on Earth. Image: NASA/JPL-Caltech/SwRI/MSSS

The visible light images of Jupiter’s north pole are very different from our usual perception of Jupiter. People have been looking at Jupiter for a long time, and the gas giant’s storm bands, and the Great Red Spot, are iconic. But the north polar region looks completely different, with whirling, rotating storms similar to hurricanes here on Earth.

The Junocam instrument is responsible for the visible light pictures of Jupiter that we all enjoy. But the Jovian Infrared Auroral Mapper (JIRAM) is showing us a side of Jupiter that the naked eye will never see.

The Juno Infrared Auroral Mapper (JIRAM) captured this infrared image of Jupiter's south pole. This part of Jupiter cannot be seen from Earth. Image: NASA/JPL-Caltech/SwRI/MSSS
The Juno Infrared Auroral Mapper (JIRAM) captured this infrared image of Jupiter’s south pole. This part of Jupiter cannot be seen from Earth. Image: NASA/JPL-Caltech/SwRI/MSSS

“JIRAM is getting under Jupiter’s skin, giving us our first infrared close-ups of the planet,” said Alberto Adriani, JIRAM co-investigator from Istituto di Astrofisica e Planetologia Spaziali, Rome. “These first infrared views of Jupiter’s north and south poles are revealing warm and hot spots that have never been seen before. And while we knew that the first-ever infrared views of Jupiter’s south pole could reveal the planet’s southern aurora, we were amazed to see it for the first time.”

“No other instruments, both from Earth or space, have been able to see the southern aurora.”

Even when we’re prepared to be amazed by what Juno and other spacecraft show us, we are still amazed. It’s impossible to see Jupiter’s south pole from Earth, so these are everybody’s first glimpses of it.

“No other instruments, both from Earth or space, have been able to see the southern aurora,” said Adriani. “Now, with JIRAM, we see that it appears to be very bright and well-structured. The high level of detail in the images will tell us more about the aurora’s morphology and dynamics.”

Beyond the juicy images of Jupiter are some sound recordings. It’s been known since about the 1950’s that Jupiter is a noisy planet. Now Juno’s Radio/Plasma Wave Experiment (WAVE) has captured a recording of that sound.

“Jupiter is talking to us in a way only gas-giant worlds can,” said Bill Kurth, co-investigator for the Waves instrument from the University of Iowa, Iowa City. “Waves detected the signature emissions of the energetic particles that generate the massive auroras which encircle Jupiter’s north pole. These emissions are the strongest in the solar system. Now we are going to try to figure out where the electrons come from that are generating them.”

Oddly enough, that’s pretty much exactly what I expected Jupiter to sound like. Like something from an early sci-fi film.

There’s much more to come from Juno. These images and recordings of Jupiter are just the result of Juno’s first orbit. There are over 30 more orbits to come, as Juno examines the gas giant as it orbits beneath it.

Grab Your Smartphone And Become A Citizen Scientist For NASA

NASA's new app, the Globe Observer, will allow users to collect observations of clouds, and engage in a little citizen science. Image: NASA GLOBE Observer
NASA's new app, the Globe Observer, will allow users to collect observations of clouds, and engage in a little citizen science. Image: NASA GLOBE Observer

It’s long been humanity’s dream to do something useful with our smartphones. Sure, we can take selfies, and post pictures of our meals, but true smartphone greatness has eluded us. Until now, that is.

Thanks to NASA, we can now do some citizen science with our ubiquitous devices.

For over 20 years, and in schools in over 110 countries, NASA’s Global Learning and Observations to Benefit the Environment (GLOBE) program has helped students understand their local environment in a global context. Now NASA has released the GLOBE Observer app, which allows users to capture images of clouds in their local environment, and share them with scientists studying the Earth’s climate.

“With the launch of GLOBE Observer, the GLOBE program is expanding beyond the classroom to invite everyone to become a citizen Earth scientist,” said Holli Riebeek Kohl, NASA lead of GLOBE Observer. The app will initially be used to capture cloud observations and images because they’re such an important part of the global climate system. But eventually, GLOBE Observer will also be used to observe land cover, and to identify types of mosquito larvae.

GLOBE has two purposes. One is to collect solid scientific data, the other is to increase users’ awareness of their own environments. “Once you collect environmental observations with the app, they are sent to the GLOBE data and information system for use by scientists and students studying the Earth,” said Kohl. “You can also use these observations for your own investigations and interact with a vibrant community of individuals from around the world who care about Earth system science and our global environment.”

Clouds are a dynamic part of the Earth’s climate system. Depending on their type, their altitude, and even the size of their water droplets, they either trap heat in the atmosphere, or reflect sunlight back into space. We have satellites to observe and study clouds, but they have their limitations. An army of citizen scientists observing their local cloud population will add a lot to the efforts of the satellites.

“Clouds are one of the most important factors in understanding how climate is changing now and how it’s going to change in the future,” Kohl said. “NASA studies clouds from satellites that provide either a top view or a vertical slice of the clouds. The ground-up view from citizen scientists is valuable in validating and understanding the satellite observations. It also provides a more complete picture of clouds around the world.”

The observations collected by GLOBE users could end up as part of NASA's Earth Observatory, which tracks the cloud fraction around the world. Image: NASA/NASA Earth Observation.
The observations collected by GLOBE users could end up as part of NASA’s Earth Observatory, which tracks the cloud fraction around the world. Image: NASA/NASA Earth Observation.

The GLOBE team has issued a challenge to any interested citizen scientists who want to use the app. Over the next two weeks, the team is hoping that users will make ground observations of clouds at the same time as a cloud-observing satellite passes overhead. “We really encourage all citizen scientists to look up in the sky and take observations while the satellites are passing over through Sept. 14,” said Kohl.

The app makes this easy to do. It informs users when a satellite will be passing overhead, so we can do a quick observation at that time. We can also use Facebook or Twitter to view daily maps of the satellite’s path.

“Ground measurements are critical to validate measurements taken from space through remote sensing,” said Erika Podest, an Earth scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California, who is working with GLOBE data. “There are some places in the world where we have no ground data, so citizen scientists can greatly contribute to advancing our knowledge this important part of the Earth system.”

The app itself seems pretty straightforward. I checked for upcoming satellite flyovers and was notified of 6 flyovers that day. It’s pretty quick and easy to step outside and take an observation at one of those times.

I did a quick observation from the street in front of my house and it took about 2 minutes. To identify cloud types, you just match what you see with in-app photos of the different types of clouds. Then you estimate the percentage of cloud cover, or specify if the sky is obscured by blowing snow, or fog, or something else. You can also add pictures, and the app guides you in aiming the camera properly.

The GLOBE Observer app is easy to use, and kind of fun. It’s simple enough to fit a quick cloud observation in between selfies and meal pictures.

Download it and try it out.

You can download the IOS version from the App Store, and the Android version from Google Play.

Curiosity Rover Captures Full-Circle Panorama of Enticing ‘Murray Buttes’ on Mars

This 360-degree panorama was acquired by the Mast Camera (Mastcam) on NASA's Curiosity Mars rover as the rover neared features called "Murray Buttes" on lower Mount Sharp. Credit: NASA/JPL-Caltech/MSSS
This 360-degree panorama was acquired by the Mast Camera (Mastcam) on NASA's Curiosity Mars rover as the rover neared features called "Murray Buttes" on lower Mount Sharp.  Credit: NASA/JPL-Caltech/MSSS
This 360-degree panorama was acquired by the Mast Camera (Mastcam) on NASA’s Curiosity Mars rover as the rover neared features called “Murray Buttes” on lower Mount Sharp. Credit: NASA/JPL-Caltech/MSSS

Four years after a nail biting touchdown on the Red Planet, NASA’s SUV-sized Curiosity rover is at last nearing the long strived for “Murray Buttes” formation on the lower reaches of Mount Sharp.

This is a key milestone for the Curiosity mission because the “Murray Buttes” are the entry way along Curiosity’s planned route up lower Mount Sharp.

Ascending and diligently exploring the sedimentary lower layers of Mount Sharp, which towers 3.4 miles (5.5 kilometers) into the Martian sky, is the primary destination and goal of the rovers long term scientific expedition on the Red Planet.

The area features eroded mesas and buttes that are reminiscent of the U.S. Southwest.

So the team directed the rover to capture a 360-degree color panorama using the robots mast mounted Mastcam camera earlier this month on Aug. 5.

The full panorama shown above combines more than 130 images taken by Curiosity on Aug. 5, 2016, during the afternoon of Sol 1421 by the Mastcam’s left-eye camera.

In particular note the dark, flat-topped mesa seen to the left of the rover’s arm. It stands about 50 feet (about 15 meters) high and, near the top, about 200 feet (about 60 meters) wide.

Coincidentally, Aug. 5 also marks the fourth anniversary of the six wheeled rovers landing on the Red Planet via the unprecedented Sky Crane maneuver.

You can explore this spectacular Mars panorama in great detail via this specially produced 360-degree panorama from JPL. Simply move the magnificent view back and forth and up and down and all around with your mouse or mobile device.

Video Caption: This 360-degree panorama was acquired on Aug. 5, 2016, by the Mastcam on NASA’s Curiosity Mars rover as the rover neared features called “Murray Buttes” on lower Mount Sharp. The dark, flat-topped mesa seen to the left of the rover’s arm is about 50 feet (about 15 meters) high and, near the top, about 200 feet (about 60 meters) wide.

“The buttes and mesas are capped with rock that is relatively resistant to wind erosion. This helps preserve these monumental remnants of a layer that formerly more fully covered the underlying layer that the rover is now driving on,” say rover scientists.

“The relatively flat foreground is part of a geological layer called the Murray formation, which formed from lakebed mud deposits. The buttes and mesas rising above this surface are eroded remnants of ancient sandstone that originated when winds deposited sand after lower Mount Sharp had formed. Curiosity closely examined that layer — the Stimson formation — during the first half of 2016 while crossing a feature called “Naukluft Plateau” between two exposures of the Murray formation.”

Three years ago, the team informally named the site to honor Caltech planetary scientist Bruce Murray (1931-2013), a former director of NASA’s Jet Propulsion Laboratory, Pasadena, California. JPL manages the Curiosity mission for NASA.

As of today, Sol 1447, August 31, 2016, Curiosity has driven over 7.9 miles (12.7 kilometers) since its August 2012 landing, and taken over 348,500 amazing images.

Curiosity explores Red Planet paradise at Namib Dune during Christmas 2015 - backdropped by Mount Sharp.  Curiosity took first ever self-portrait with Mastcam color camera after arriving at the lee face of Namib Dune.  This photo mosaic shows a portion of the full self portrait and is stitched from Mastcam color camera raw images taken on Sol 1197, Dec. 19, 2015.  Credit: NASA/JPL/MSSS/Ken Kremer/kenkremer.com/Marco Di Lorenzo
Curiosity explores Red Planet paradise at Namib Dune during Christmas 2015 – backdropped by Mount Sharp. Curiosity took first ever self-portrait with Mastcam color camera after arriving at the lee face of Namib Dune. This photo mosaic shows a portion of the full self portrait and is stitched from Mastcam color camera raw images taken on Sol 1197, Dec. 19, 2015. Credit: NASA/JPL/MSSS/Ken Kremer/kenkremer.com/Marco Di Lorenzo

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

Ken Kremer