Space Exploration Archives

February 27, 2015December 23, 2015 by Ken Kremer

Orbital ATK Aims for March 2016 Antares Rocket Launch Restart with New Engines

Orbital Sciences Corporation Antares rocket and Cygnus spacecraft blasts off on July 13 2014 from Launch Pad 0A at NASA Wallops Flight Facility , VA, on the Orb-2 mission and loaded with over 3000 pounds of science experiments and supplies for the crew aboard the International Space Station. Credit: Ken Kremer - kenkremer.com

The newly merged company Orbital ATK is aiming to restart launches of their “upgraded Antares” rocket in March 2016 using completely new engines, following the catastrophic explosion on Oct. 28, 2014 that destroyed the rocket seconds after blastoff from a Virginia launch pad. Antares was carrying a Cygnus module loaded with supplies on a critical space station resupply mission for NASA.

The March 2016 launch date of Antares from the Wallops Island base along Virginia’s eastern shore was announced by David Thompson, Orbital ATK, President and CEO, during a recent conference call with investors and analysts regarding the formal merger of Orbital Sciences and ATK.

“The target date for that [Antares launch] is the 1st of March next year,” said Thompson.

Cygnus will be fully loaded with new supplies for the station crew.

“The first launch … will have a full cargo load on board.”

The Orbital Sciences Corp. commercial Antares rocket was destroyed in a raging inferno about 15 seconds after liftoff on Oct. 28 when one of the Soviet-era built first stage engines apparently exploded and cascaded into a spectacular aerial fireball just above the launch pad 0A at NASA’s Wallops Flight Facility on the doomed Orb-3 mission carrying the Cygnus resupply module to the International Space Station (ISS).

First stage propulsion system at base of Orbital Sciences Antares rocket appears to explode moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014, at 6:22 p.m. Credit: Ken Kremer – kenkremer.com

Orbital’s privately developed Cygnus pressurized cargo freighter was loaded with nearly 5000 pounds (2200 kg) of science experiments, research instruments, crew provisions, spare parts, spacewalk and computer equipment and gear on the Orb-3 mission. The module and all its contents were destroyed.

Orbital established an independent accident investigation review board immediately following the launch failure.

“We are about four months now into the recovery from the failure,’ said Thompson.

A turbopump failure in one of the rockets Soviet-era first stage engines has been identified as the most likely cause of the Antares destruction, according to official statements from David Thompson.

The AJ26 engines were originally manufactured some 40 years ago in the then Soviet Union as the NK-33. They were refurbished and “Americanized” by Aerojet Rocketdyne.

Antares doomed descent to incendiary destruction after first stage propulsion system of Orbital Sciences’ rocket exploded moments after blastoff from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer – kenkremer.com

“The next Cygnus will be launched on the upgraded Antares from Wallops Island. The target date for that is the 1st of March next year.”

After the launch failure Orbital, decided to ditch the trouble plagued AJ-26 and “re-engineered” the vehicle with new engines.

The Antares first stage had been powered by a pair of the aging AJ26 engines. These will now be replaced by a pair of newly manufactured Russian RD-181 engines, assembled and purchased from NPO Energomash.

“The first launch of the re-engineered vehicle in March of next year … will have a full cargo load on board.”

Thompson said the March 2016 launch target date will be preceded by a hot fire test of the first stage engines, which is currently planned to take place in January 2015. They will not conduct a demonstration launch and have opted for a full up space station resupply flight.

“We’re going to go with the cargo load on the first launch. What we are going to do in advance of that, in January of next year, is we’re going to take the first stage of Antares out to the launch pad with the new engines and do a flight readiness firing, somewhat similar to what we did back in early 2013, in advance of the first Antares flight,” said Thompson.

“But other than that, unless something came up there that was surprising, we should then be able to proceed pretty expeditiously to the first launch of the re-engineered vehicle in March of next year, and that will have a full cargo load on board.”

Orbital Sciences technicians at work on two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today at NASA Wallaps. These engines powered the successful Antares liftoff on Jan. 9, 2014 at NASA Wallops, Virginia bound for the ISS. Credit: Ken Kremer - kenkremer.com — Orbital Sciences technicians at work on two AJ26 first stage engines at the base of an Antares rocket during exclusive visit by Ken Kremer/Universe Today at NASA Wallaps. These engines powered the successful Antares liftoff on Jan. 9, 2014 at NASA Wallops, Virginia bound for the ISS. Credit: Ken Kremer – kenkremer.com

Thompson also reiterated that Orbital will fully meet its resupply services contarct with NASA and make up for the lost cargo.

The Orbital-3, or Orb-3, mission that ended in disaster on Oct 28, was to be the third of eight cargo resupply missions to the ISS through 2016 under the NASA Commercial Resupply Services (CRS) contract award valued at $1.9 Billion. Under the CRS program Orbital is to deliver 20,000 kilograms of research experiments, crew provisions, spare parts, and hardware for the eight ISS flights.

“The focus all along has been to do everything we can to fulfill our commitments to delivering cargo to the space station for NASA, and to minimize any disruption that we can to the delivery schedules.”

Towards that end Orbital ATK has contracted with United Launch Alliance (ULA) to launch at least one and up to two Cygnus cargo missions to the International Space Station (ISS) under NASA’s Commercial Resupply Services (CRS) program.

The first Cygnus mission would liftoff sometime late in the fourth quarter of 2015 aboard an Atlas V 401 vehicle from Space Launch Complex 41 (SLC-41) at Cape Canaveral Air Force Station in Florida.

I watched the unfolding disaster first hand from the media viewing site about 1.8 miles away and filed eyewitness reports at the time. Several of my launch pad remote cameras were set up at the pad. They were impounded and the images were used by investigators during the initial investigation. They were returned to me about a month later and are featured here and in my earlier Antares reports.

Watch here for Ken’s ongoing reporting about Antares and NASA Wallops.

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

Ken Kremer

February 26, 2015December 23, 2015 by Bob King

Ceres Bizarre Bright Spot Now Has a Companion

This image was taken by NASA's Dawn spacecraft of dwarf planet Ceres on Feb. 19 from a distance of nearly 29,000 miles (46,000 km). It shows that the brightest spot on Ceres has a dimmer companion, which apparently lies in the same basin. See below for the wide view. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Aliens making dinner with a solar cooker? Laser beams aimed at hapless earthlings? Whatever can that – now those – bright spots on Ceres be? The most recent images taken by the Dawn spacecraft now reveal that the bright pimple has a companion spot. Both are tucked inside a substantial crater and seem to glow with an intensity out of proportion to the otherwise dark and dusky surrounding landscape.“The brightest spot continues to be too small to resolve with our camera, but despite its size it is brighter than anything else on Ceres,” said Andreas Nathues, lead investigator for the framing camera team at the Max Planck Institute for Solar System Research, Gottingen, Germany. “This is truly unexpected and still a mystery to us.”

Tight crop of the two bright spots. Could they be ice? Volcano-related? Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA — Tight crop of the two bright spots. Could they be ice? Volcano-related? Credit:

It’s a mystery bound to stir fresh waves of online speculative pseudoscience. The hucksters better get moving. Dawn is fewer than 29,000 miles (46,000 km) away and closing fast. On March 6 it will be captured by Ceres gravity and begin orbiting the dwarf planet for a year or more. Like waking up and rubbing the sleep from your eyes, our view of Ceres and its enigmatic “twin glows” will become increasingly clear in about six weeks.

Dawn's approaches Ceres from the left (direction of the Sun) and gets captured by its gravity. The craft first gets closer as it approaches but then recedes (moves off to right) before closing in again and ultimately orbiting the asteroid. The solid lines show where Dawn is thrusting with its ion engine. As it swings to the right of Ceres, photos will show it as a crescent. Credit: NASA/Marc Rayman — Dawn approaches Ceres from the left (direction of the Sun) and gets captured by its gravity. The craft first gets closer as it approaches but then recedes (moves off to right) before closing in again and ultimately settling into orbit around the asteroid. The solid lines show where Dawn is thrusting with its ion engine. As it swings to the right, photos will show Ceres as a crescent. Credit: NASA/Marc Rayman

Why not March 6th when it enters orbit? Momentum is temporarily carrying the probe beyond Ceres. Only after a series of balletic moves to reshape its orbit to match that of Ceres will it be able to return more detailed images. You’ll recall that Rosetta did the same before finally settling into orbit around Comet 67P.

Closest approach occurred on Feb. 23 at 24,000 miles (38,600 km); at the moment the spacecraft is moving beyond Ceres at the very relaxed rate of 35 mph (55 kph).

This and the photo below were taken on Feb. 19, 2015 and processed to enhance clarity. Notice the very large but shallow crater below center. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

We do know that unlike Dawn’s first target, the asteroid Vesta, Ceres is rich in water ice. It’s thought that it possesses a mantle of ice and possibly even ice on its surface. In January 2014, ESA’s orbiting Herschel infrared observatory detected water vapor given off by the dwarf planet. Clays have been identified in its crust as well, making Ceres unique compared to many asteroids in the main belt that orbit between Mars and Jupiter.

Given the evidence for H₂0, we could be seeing ice reflecting sunlight possibly from a recent impact that exposed new material beneath the asteroid’s space-weathered skin. If so, it’s odd that the spot should be almost perfectly centered in the crater.

Chris Russell, principal investigator for the Dawn mission, offers another possible scenario, where the bright spots “may be pointing to a volcano-like origin.” Might icy volcanism in the form of cryovolcanoes have created the dual white spots? Or is the white material fresh, pale-colored rock either erupted from below or exposed by a recent impact? Ceres is a very dark world with an albedo or reflectivity even less than our asphalt-dark Moon. Freshly exposed rock or ice might stand out starkly.

An 8.8g part slice of the eucrite meteorite NWA 3147. Most eucrites are derived from lava flows on the asteroid Vesta. Credit: Bob King — A part slice of the eucrite meteorite NWA 3147. Most eucrites are derived from lava flows on the asteroid Vesta and are rich in light-toned minerals. Credit: Bob King

One of the more common forms of asteroid lava found on Earth are the eucrite achondrite meteorites. Many are rich in plagioclase and other pale minerals that are good reflectors of light. Of course, these are all speculations, but the striking contrast of bright and dark certainly piques our curiosity.

Artist’s concept of Dawn in its survey orbit at dwarf planet Ceres. Credit: NASA/JPL-Caltech

Additional higher resolutions photos streamed back by Dawn show a fascinating array of crater types from small and deep to large and shallow. On icy worlds, ancient impact craters gradually “relax” and lose relief over time, flattening as it were. We’ve seen this on the icy Galilean moons of Jupiter and perhaps the largest impact basins on Ceres are examples of same.

Questions, speculations. Our investigation of any new world seen up close for the first time always begins with questions … and often ends with them, too.

February 19, 2015December 23, 2015 by Ken Kremer

25 Years Since Voyager’s ‘Pale Blue Dot’ Images

These six narrow-angle color images were made from the first ever "portrait" of the solar system taken by Voyager 1 on Valentine’s Day on Feb. 14, 1990, which was more than 4 billion miles from Earth and about 32 degrees above the ecliptic. Venus, Earth, Jupiter, and Saturn, Uranus, Neptune are seen in these blown-up images, from left to right and top to bottom. Credit: NASA/JPL-Caltech

A quarter of a century has passed since NASA’s Voyager 1 spacecraft snapped the iconic image of Earth known as the “Pale Blue Dot” that shows all of humanity as merely a tiny point of light.

The outward bound Voyager 1 space probe took the ‘pale blue dot’ image of Earth 25 years ago on Valentine’s Day, on Feb. 14, 1990 when it looked back from its unique perch beyond the orbit of Neptune to capture the first ever “portrait” of the solar system from its outer realms.

Voyager 1 was 4 billion miles from Earth, 40 astronomical units (AU) from the sun and about 32 degrees above the ecliptic at that moment.

The idea for the images came from the world famous astronomer Carl Sagan, who was a member of the Voyager imaging team at the time.

He head the idea of pointing the spacecraft back toward its home for a last look as a way to inspire humanity. And to do so before the imaging system was shut down permanently thereafter to repurpose the computer controlling it, save on energy consumption and extend the probes lifetime, because it was so far away from any celestial objects.

Sagan later published a well known and regarded book in 1994 titled “Pale Blue Dot,” that refers to the image of Earth in Voyagers series.

This narrow-angle color image of the Earth, dubbed "Pale Blue Dot," is a part of the first ever "portrait" of the solar system taken by Voyager 1 on Valentine’s Day on Feb. 14, 1990. Credit: NASA/JPL-Caltech — This narrow-angle color image of the Earth, dubbed “Pale Blue Dot,” is a part of the first ever “portrait” of the solar system taken by Voyager 1 on Valentine’s Day on Feb. 14, 1990. Credit: NASA/JPL-Caltech

“Twenty-five years ago, Voyager 1 looked back toward Earth and saw a ‘pale blue dot,’ ” an image that continues to inspire wonderment about the spot we call home,” said Ed Stone, project scientist for the Voyager mission, based at the California Institute of Technology, Pasadena, in a statement.

Six of the Solar System’s nine known planets at the time were imaged, including Venus, Earth, Jupiter, and Saturn, Uranus, Neptune. The other three didn’t make it in. Mercury was too close to the sun, Mars had too little sunlight and little Pluto was too dim.

Voyager snapped a series of images with its wide angle and narrow angle cameras. Altogether 60 images from the wide angle camera were compiled into the first “solar system mosaic.”

Voyager 1 was launched in 1977 from Cape Canaveral Air Force Station in Florida as part of a twin probe series with Voyager 2. They successfully conducted up close flyby observations of the gas giant outer planets including Jupiter, Saturn, Uranus and Neptune in the 1970s and 1980s.

Both probes still operate today as part of the Voyager Interstellar Mission.

“After taking these images in 1990, we began our interstellar mission. We had no idea how long the spacecraft would last,” Stone said.

Hurtling along at a distance of 130 astronomical units from the sun, Voyager 1 is the farthest human-made object from Earth.

Solar System Portrait - 60 Frame Mosaic. The cameras of Voyager 1 on Feb. 14, 1990, pointed back toward the sun and took a series of pictures of the sun and the planets, making the first ever "portrait" of our solar system as seen from the outside. Missing are Mercury, Mars and Pluto Credit: NASA/JPL-Caltech — Solar System Portrait – 60 Frame Mosaic. The cameras of Voyager 1 on Feb. 14, 1990, pointed back toward the sun and took a series of pictures of the sun and the planets, making the first ever “portrait” of our solar system as seen from the outside. Missing are Mercury, Mars and Pluto. Credit: NASA/JPL-Caltech

Voyager 1 still operates today as the first human made instrument to reach interstellar space and continues to forge new frontiers outwards to the unexplored cosmos where no human or robotic emissary as gone before.

Here’s what Sagan wrote in his “Pale Blue Dot” book:

“That’s here. That’s home. That’s us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. … There is perhaps no better demonstration of the folly of human conceits than this distant image of our tiny world.”

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

Ken Kremer

February 18, 2015December 23, 2015 by Nancy Atkinson

Why Can’t We Design the Perfect Spacesuit?

The MIT BioSuit, a skintight spacesuit that offers improved mobility and reduced mass compared to modern gas-pressurized spacesuits. Credit: MIT.

So far, every spacesuit humans have utilized has been designed with a specific mission and purpose in mind. As of yet, there’s been no universal or “perfect” spacesuit that would fit every need. For example, the US ACES “pumpkin” suits and the Russian Sokol are only for launch and reentry and can’t be used for spacewalks. And the Apollo A7L suits were designed with hard soled boots for astronauts to walk on the Moon, while the current NASA EMU and the Russian Orlan are designed for use in space, but with soft soled booties so as not to damage the exterior of the space station.

What would constitute the perfect spacesuit that could be used for any mission? It would have to be lightweight while being impervious to rips, impacts and radiation, but also be flexible, fit multiple sizes, and be comfortable enough to be worn for long periods of time.

With those specifications in mind, is it possible to create the perfect spacesuit?

Spacesuit and Spacewalk History — An astronaut using NASA’s current EMU spacewalking suit, outside the International Space Station. Credit: NASA

“Designing a spacesuit turns into a battle between protection and mobility,” said NASA astronaut trainer Robert Frost in an article on Quora. “The more we try to protect the wearer, the less mobile they become. The more mobile we make them, the less protected they are.”

The perfect spacesuit would be, to quote Elon Musk, “badass.”

That’s the terminology the SpaceX used in negotiations with suit-making companies to create the pressure suit for SpaceX’s future commercial passengers. SpaceX is now designing their own suit, and Musk said SpaceX is looking for not just utility but esthetics, too.

“It needs to both look like a 21st-century space suit and work well,” he said during a reddit AMA.

But even with SpaceX’s ‘badass’ suit, they are designing with one purpose in mind.

And there are obstacles to having a “badass space suit design,” wrote Eric Sofge in an article in Popular Science. “A launch-entry suit is ungainly, an oversize one-piece embedded with rigid interfaces for the helmet and gloves, and enough room to inflate, basketball-like, when pressurized—especially in the seat, so an astronaut isn’t forced to stand up.”

New Ideas

One of the best hopes on the horizon is a “shrink-wrap” type of spacesuit that MIT has been developing. It is a lightweight, form-fitting, flexible spacesuit — a la Seven of Nine on Star Trek: Voyager— lined with tiny, muscle like coils.

Dava Newman wearing the biosuit. Image credit: Donna Coveney

“With conventional spacesuits, you’re essentially in a balloon of gas that’s providing you with the necessary one-third of an atmosphere [of pressure,] to keep you alive in the vacuum of space,” said one of the developers, Dava Newman. “We want to achieve that same pressurization, but through mechanical counterpressure — applying the pressure directly to the skin, thus avoiding the gas pressure altogether. We combine passive elastics with active materials. … Ultimately, the big advantage is mobility, and a very lightweight suit for planetary exploration.”

MIT is using a nickel-titanium shape-memory alloy and they are continuing to test ideas. Some problems with this suit include the difficulty of putting on such a tight suit in a zero-gravity environment and how a gas-pressurized helmet can be connected to the compression-pressurized suit.

The NASA Z-2 suit will incorporate the "technology" design the public voted on. Credit: NASA — The NASA Z-2 suit will incorporate the “technology” design the public voted on. Credit: NASA

NASA recently revealed the winner of a public-voted spacesuit design called the Z-2. While it looks a bit like Buzz Lightyear’s fictional suit, it has bearings in the joints that make more flexible than NASA’s current EMU. It also has a rear-entry port, allowing it to be docked to the side of a mobile transporter or habitat, essentially turning the suit into its own air lock. This helps to avoid bringing in abrasive soil and dust such as lunar regolith Martian soil. NASA is currently testing the Z-2 prototype with plans to develop a better suit, the Z-3. If it works well, the Z-3 might be used in a space walk from the International Space Station by 2017.

So, still, the perfect spacesuit eludes us.

But here are some other additions that would make the perfect spacesuit:

Self-healing: Currently, having multiple layers is the best way to defend against rips or tears, which can be fatal in the vacuum of space. But MIT’s body suit would utilize mechanical counterpressure to counteract a rip, and engineers at ILC Dover are looking into integrating self-healing materials, such as polymers embedded with microencapsulated chemicals that would create a foam to heal a torn suit.

Spacesuit Glove. Courtesy of Johnson Space Center

Better gloves: gloves have been one of the hardest things to design in spacesuits. Making a glove that is both flexible and protective is a challenge. Astronaut Duane Carey compared spacewalks to trying to fix your car while wearing winter mittens. Astronauts have had skin rubbed until it bleeds and have lost fingernails because of how the current gloves wear. NASA is constantly working on better gloves.

Augmented Vision: Currently, NASA’s polycarbonate helmets could be confused with fishbowls. One material that could be used for future helmets is a clear ceramic called ALON, which is thinner than bulletproof glass and three times as strong. Another addition could be an internal heads-up display — like ones used by F-16 pilots – to provide data and information.

The cooling undergarment used under NASA's EMU spacesuit. Credit: NASA. — The cooling undergarment used under NASA’s EMU spacesuit. Credit: NASA.

A better cooling system: Current suits have “underwear” with about 300 feet of plastic tubing that circulate waters to draw away body heat. Purdue University engineers are developing a polymer using glass fibers coated with thermoelectric nanocrystals that absorb heat and discharge electricity.

Artificial Gravity: Remember the magnetic boots worn in Star Trek: The Undiscovered Country and Star Trek: Insurrection? The University of Massachusetts is developing a dry adhesive that could help astronauts and those pesky floating tools to “stick” to surfaces. It is made of a carbon fiber weave and mimics the skin and tendon structure of gecko feet. Another idea — while not quite the same – is a way to counter muscle and bone atrophy in zero-G: Draper Labs are developing gyroscopes the could be attached to the arms and legs of spacesuits that could provide resistance similar to the force of gravity on Earth.

Long-life Battery Power: One issue for long spacewalks is having enough battery power. Michigan Tech is developing units that can convert movement into electricity. Also, Elon Musk might have some ideas for long-lasting batteries…

So, while many entities are working on ideas and concepts, the perfect spacesuit has yet to be developed. If humans are going to go to an asteroid, back to the Moon, to Mars or on a mission to deep space, we’ll need a suit as close to perfect as possible.

Further reading:
MIT’s ‘shrink-wrapped’ spacesuit
The Deep Space Suit: Popular Science
Factors Considered in the Design of a Spacesuit: Quora
NASA’s Z-2 Suit

February 12, 2015December 23, 2015 by Ken Kremer

Space Weather Storm Monitoring Satellite Blasts off for Deep Space on SpaceX Rocket

NOAA's DSCOVR satellite launches from Cape Canaveral Air Force Station on Feb. 11, 2015. DSCOVR will provide NOAA space weather forecasters more reliable measurements of solar wind conditions, improving their ability to monitor potentially harmful solar activity. Credit: Alan Walters/AmericaSpace

After a 17 year long wait, a new American mission to monitor intense solar storms and warn of impeding space weather disruptions to vital power grids, telecommunications satellites and public infrastructure was launched atop a SpaceX Falcon 9 on Wednesday, Feb. 11, from Cape Canaveral, Florida, to start a million mile journey to its deep space observation post.

The third time proved to be the charm when the Deep Space Climate Observatory, or DSCOVR science satellite lifted off at 6:03 p.m. EST Wednesday from Space Launch Complex 40 at Cape Canaveral Air Force Station in Florida.

The spectacular sunset blastoff came after two scrubs this week forced by a technical problem with the Air Force tracking radar and adverse weather on Sunday and Tuesday.

The $340 million DSCOVR has a critical mission to monitor the solar wind and aid very important forecasts of space weather at Earth at an observation point nearly a million miles from Earth. It will also take full disk color images of the sunlit side of Earth at least six times per day that will be publicly available and “wow” viewers.

Launch of NOAA DSCOVR satellite from Cape Canaveral Air Force Station on Feb. 11, 2015 to monitor solar storms and space weather. Credit: Julian Leek

The couch sized probe was targeted to the L1 Lagrange Point, a neutral gravity point that lies on the direct line between Earth and the sun located 1.5 million kilometers (932,000 miles) sunward from Earth. At L1 the gravity between the sun and Earth is perfectly balanced and the satellite will orbit about that spot just like a planet.

L1 is a perfect place for the science because it lies outside Earth’s magnetic environment. The probe will measure the constant stream of solar wind particles from the sun as they pass by.

The DSCOVR spacecraft (3-axis stabilized, 570 kg) will be delivered to the Sun-Earth L1 point, 1.5 million km (1 million miles) from the Earth, directly in front of the Sun. A Halo (Lissajous) orbit will stabilize the craft's position around the L1 point while keeping it outside the radio noise emanating from the Sun. (Illustratin Credit: NASA) — The DSCOVR spacecraft (3-axis stabilized, 570 kg) will be delivered to the Sun-Earth L1 point, 1.5 million km (1 million miles) from the Earth, directly in front of the Sun. A Halo (Lissajous) orbit will stabilize the craft’s position around the L1 point while keeping it outside the radio noise emanating from the Sun. (Illustratin Credit: NASA)

DSCOVR is a joint mission between NOAA, NASA, and the U.S Air Force (USAF) that will be managed by NOAA. The satellite and science instruments are provided by NASA and NOAA. The rocket was funded by the USAF.

The mission is vital because its solar wind observations are crucial to maintaining accurate space weather forecasts to protect US infrastructure such as power grids, aviation, planes in flight, all types of Earth orbiting satellites for civilian and military needs, telecommunications, ISS astronauts and GPS systems.

It will take about 150 days to reach the L1 point and complete satellite and instrument checkouts.

DSCOVR will then become the first operational space weather mission to deep space and function as America’s primary warning system for solar magnetic storms.

It will replace NASA’s aging Advanced Composition Explorer (ACE) satellite which is nearly 20 years old and far beyond its original design lifetime.

“DSCOVR is the latest example of how NASA and NOAA work together to leverage the vantage point of space to both understand the science of space weather and provide direct practical benefits to us here on Earth,” said John Grunsfeld, associate administrator of NASA’s Science Mission Directorate in Washington.

DSCOVR was first proposed in 1998 by then US Vice President Al Gore as the low cost ‘Triana’ satellite to take near continuous views of the Earth’s entire globe to feed to the internet as a means of motivating students to study math and science. It was eventually built as a much more capable Earth science satellite that would also conduct the space weather observations.

But Triana was shelved for purely partisan political reasons and the satellite was placed into storage at NASA Goddard and the science was lost until now.

DSCOVR mission logo. Credit: NOAA/NASA/U.S. Air Force

DSCOVR is equipped with a suite of four continuously operating solar science and Earth science instruments from NASA and NOAA.

It will make simultaneous scientific observations of the solar wind and the entire sunlit side of Earth.

The 750-kilogram (1250 pound) DSCOVR probe measures 54 inches by 72 inches.

Technician works on NASA Earth science instruments and Earth imaging EPIC camera (white circle) housed on NOAA/NASA Deep Space Climate Observatory (DSCOVR) inside NASA Goddard Space Flight Center clean room in November 2014. Credit: Ken Kremer/kenkremer.com/AmericaSpace

The two Earth science instruments from NASA are the Earth Polychromatic Imaging Camera (EPIC) and the National Institute of Standards and Technology Advanced Radiometer (NISTAR).

EPIC will provide true color spectral images of the entire sunlit face of Earth at least six times per day, as viewed from an orbit around L1. They will be publically available within 24 hours via NASA Langley.

It will view the full disk of the entire sunlit Earth from sunrise to sunset and collect a variety of science measurements including on ozone, aerosols, dust and volcanic ash, vegetation properties, cloud heights and more.

Listen to my post launch interview with the BBC about DSCOVR and ESA’s successful IXV launch on Feb. 11.

A secondary objective by SpaceX to recover the Falcon 9 first stage booster on an ocean going barge had to be skipped due to very poor weather and very high waves in the Atlantic Ocean making a safe landing impossible. The stage did successfully complete a soft landing in the ocean.

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

Ken Kremer

NOAA/NASA Deep Space Climate Observatory (DSCOVR) undergoes processing in NASA Goddard Space Flight Center clean room. Solar wind instruments at right. DSCOVER will launch in February 2015 atop SpaceX Falcon 9 rocket. Credit: Ken Kremer/kenkremer.com/AmericaSpace

Launch of NOAA DSCOVR satellite from Cape Canaveral Air Force Station on Feb. 11, 2015 to monitor solar storms and space weather. Credit: John Studwell

Prelaunch view of SpaceX rocket on Cape Canaveral launch pad taken from LC-39 at the Kennedy Space Center. Credit: Chuck Higgins

February 11, 2015December 23, 2015 by David Dickinson

The Number of Asteroids We Could Visit and Explore Has Just Doubled

There’s a famous line from Shakespeare’s Hamlet that says “There are more things in heaven and Earth, Horatio, than are dreamt of in your philosophy,” and the same now holds true for brave new worlds for humans to explore.

This result was published earlier this week courtesy of the NASA/JPL Near-Earth Program Office. The study found that the number of possible asteroid targets for human exploration has now doubled from the 666 known in the first study, completed in late 2010.

NHATS NEO asteroid discoveries by year. Credit: NASA/GFSC/Brent Barbee

This information comes from NHATS, which stands for the Near Earth Object Human Spaceflight Accessible Targets Study. Yes, it’s an acronym containing acronyms. NHATS is an automated system based out of Greenbelt, Maryland which monitors and periodically updates its list of potential target candidates for accessibility. The NHATS system data is readily accessible to the public online, and as of February 11^th 2015, 1346 NHATS compliant asteroids are known.

NEO orbit types. — NEA orbit types. Credit: Brent Barbee/NASA/GSFC

This is the Holy Grail for the future of manned spaceflight, and will represent a good stepping stone (bad pun intended) for future crewed missions to Mars. Several hundred NHATS asteroids require less time and energy to reach than the Red Planet, and a few dozen even require less energy to reach than it does to enter lunar orbit.

Relative delta-V and return velocity is crucial. Apollo astronauts were subject to a blistering 11 kilometre per second reentry velocity on their return from the Moon, and future asteroid missions would be subject to the same style of trajectory on return to Earth from a solar orbit.

Mission to an NEO: a typical orbital profile. Credit: Brent Barbee/NASA/GSFC

The test of the Orion heat shield on reentry during last year’s EFT-1 flight was a step in this direction, and the next test will be an uncrewed launch atop an SLS rocket in September 2018. If all goes according to schedule — and NASA can successfully weather the ever-shifting political winds of multiple future changes of administration — expect to see astronauts exploring an NHATS asteroid placed in lunar orbit sometime around late 2023.

I know. “When I was a kid back in the 70’s…” we expected to be vacationing on Callisto by 2015, as well.

Brent Barbee at NASA’s Goddard Space Flight Center designed the automated NHATS system. It pulls data from a source that many comet and asteroid hunters are familiar with: JPL’s Small Bodies Database. The NHATS system then makes trajectory calculations and patches in conical solutions for possible spacecraft trajectories and actually gives potential launch window dates for future missions. Seriously, its fun to play with… you can even tailor and filter these by target dates versus maximum velocity constraints and the length of stays.

The orbit of asteroid 1943 Anteros. Credit: NASA/JPL.

The first discovered NHATS-compliant NEO was 2.3 kilometre 1943 Anteros way back in 1973, and famous alumni on the NHATS list also include 10 metre asteroid 2011 MD, which passed 12,000 kilometres from the Earth on June 27^th, 2011. 2011 MD is on NASA’s short list of asteroids ideal for human exploration. Another famous asteroid on the NHATS list is 99942 Apophis which — triskaidekaphobics take note — will safely miss the Earth by 31,300 kilometres on Friday the 13^th, April 2029. More are added every day, and the growing curve of discoveries also closely mirrors the rise of automated all-sky surveys such as LINEAR, PanSTARRS and the Catalina Sky Survey, though dedicated amateurs do get in on the act occasionally as well.

To date, over 12,000 NEA asteroids are now known, and you can expect future surveys such as the Large Synoptic Survey Telescope set to see first light in 2021 to add to their ranks. The Sentinel space telescope set to launch in 2017 will also boost the known number of NEOs as it covers our sunward blind spot from an orbit interior to the Earth’s. Remember Chelyabinsk? That could actually be a great rallying cry for Sentinel’s cause, as the asteroid came at the Earth from a sunward direction and avoided the sky sweeping robotic eyes of astronomers.

Sometimes, NEOs turn out to be returning space junk from the early Space Age (a low relative velocity and low orbital inclination is often a dead giveaway). Earth has also been known to capture an NEO as an occasional temporary second Moon, as occurred in 2006 in the case of asteroid 2006 RH120.

The LSST mirror in the Tuscon Mirror Lab. Photo by author.

But beyond just creating a database, the NHATS system also presents key opportunities for astronomers to perform follow-up observations of NEO asteroids, which is vital for precisely characterizing their orbits. Two future missions are also planned to return samples from NHATS asteroids: Hayabusa 2, which launched on December 3^rd 2014 headed for asteroid 1999 JU₃ in July 2018, and the OSIRIS-REx mission, set to launch in late 2016 headed for asteroid 101955 Bennu in 2018.

NHATS is providing a crucial target list for that day when first human footfall on an asteroid occurs… or should we say docking?

February 11, 2015December 23, 2015 by Nancy Atkinson

All the World’s Rockets, Past, Present and Future

The world's greatest rockets, past, present and future. Credit and copyright: Alex Brown.

MOAR rockets! As a followup to our recent post about the Rockets of the World (to scale), here’s another graphic posted on imgur, created by Alex Brown. While the earlier graphic only included rockets that had flown, this one has rockets that are also in development, such as the SLS, Falcon Heavy and the Long March 9. It’s also a great look back at the history of rocket development, including the V-2 ballistic, England’s Black Arrow and Korolyov’v wide-body Sputnik. All are shown to scale, as compared with an average human being.

As noted, this graphic is as of the present, February 2015.

February 8, 2015December 23, 2015 by Ken Kremer

Gorgeous Sunrises, Auroras, Landscapes, and More from Space Station Crew

Almost disappearing behind the solar panels before sunrise: the US East coast from DC to Boston. #HelloEarth. Credit: NASA/ESA/Samantha Cristoforetti

The Expedition 42 crew aboard the International Space Station (ISS) continues to delight us with stunning views of ‘Our Beautiful Earth from Space.’

Here’s a collection of a few of the newest sunrises, auroras, landscapes, nightlights, and more snapshots from the multinational crew of six astronauts and cosmonauts living and working aboard the ISS orbiting some 250 miles (400 kilometers) overhead.

And don’t forget that at sunset tonight (Feb. 8), a SpaceX Falcon 9 rocket is due to blastoff at 6:10 p.m., EST, if all goes well carrying the DSCOVR space weather satellite about a million miles (1.5 million kilometers) away to the L1 Lagrange point.

The Falcon 9 will blastoff from Cape Canaveral, Florida, pictured below:

From Key West to the Gulf of Mexico and #Atlanta, a very nice, clear, half moonlit night. Credit: NASA/Terry Virts. KSC and Cape Canaveral launch pads along Florida east coast at right. — From Key West to the Gulf of Mexico and #Atlanta, a very nice, clear, half moonlit night. Credit: NASA/Terry Virts.
KSC and Cape Canaveral launch pads along Florida east coast at right.

Tens of millions of you are included in the lead sunrise photo of the U.S. East Coast – taken by ESA astronaut Samantha Cristoforetti perched aboard the orbiting lab complex.

And here’s a “speechless sunrise” taken today by NASA astronaut Terry Virts. We agree!

#speechless from this #sunrise. Credit: NASA/Terry Virts

Always happy to see this lovely sight that has become familiar in #Patagonia. Credit: NASA/ESA/Samantha Cristoforetti

This, on the contrary, I've seen only once: the Strait of Magellan and la Tierra del Fuego free of clouds! Credit: NASA/ESA/Samantha Cristoforetti — This, on the contrary, I’ve seen only once: the Strait of Magellan and la Tierra del Fuego free of clouds! Credit: NASA/ESA/Samantha Cristoforetti

#Moscow shining like a bright star under the aurora. Credit: NASA/Terry Virts

#aurora over Anchorage and Fairbanks #Alaska. Credit: NASA/Terry Virts

The current six person crew includes astronauts and cosmonauts from three nations; America, Russia and Italy including four men and two women serving aboard the massive orbiting lab complex.

They comprise Expedition 42 Commander Barry “Butch” Wilmore and Terry Virts from NASA, Samantha Cristoforetti from the European Space Agency (ESA) and cosmonauts Aleksandr Samokutyayev, Yelena Serova, and Anton Shkaplerov from Russia.

Brazilian clouds showing off their #majesty. Credit: NASA/Terry Virts

L+72/73: Logbook. Wow, this has been a busy week! But we can still catch up a little bit… ESA astronaut Samantha Cristoforetti
….https://plus.google.com/app/basic/stream/z12iczzoqovhfdo2z23odnbwmz3cir0ox04?cbp=1hmsp4t51xmr3&sview=27&cid=5&soc-app=115&soc-platform=1&spath=%2Fapp%2Fbasic%2F%2BSamanthaCristoforetti%2Fposts …

Soyuz- everyone’s ride to space and back!

#soyuz #earth #beauty. Credit: NASA/Terry Virts

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

Ken Kremer

'I wish I could bring all of you up to see this!' Credit: NASA/Terry Virts — ‘I wish I could bring all of you up to see this!’ Credit: NASA/Terry Virts

ISS Expedition 42. Credit: NASA/ESA/Roscosmos

February 6, 2015December 23, 2015 by David Dickinson

You’ve Never Seen the Phases of the Moon from This Perspective: The Far Side

Sometimes, it seems to be a cosmic misfortune that we only get to view the universe from a singular vantage point.

Take the example of our single natural satellite. As the Moon waxes and wanes through its cycle of phases, we see the familiar face of the lunar nearside. This holds true from the day we’re born until the day we die. The Romans and Paleolithic man saw that same face, and until less than a century ago, it was anyone’s guess as to just what was on the other side.

Enter the Space Age and the possibility to finally get a peek at the universe from different perspective via our robotic ambassadors. This week, the folks over at NASA’s Scientific Visualization Studio released a unique video simulation that utilized data from NASA’s Lunar Reconnaissance Orbiter to give us a view unseen from Earth. This perspective shows just what the phases of the Moon would look like from the vantage point of the lunar farside:

You can see the Moon going through the synodic 29.5 day period a familiar phases, albeit with an unfamiliar face. Note that the Sun zips by, as the lunar farside wanes towards New. And in the background, the Earth can be seen, presenting an identical phase and tracing out a lazy figure eight as it appears and disappears behind the lunar limb.

What’s with the lunar-planetary game of peek-a-boo? Well, the point of view for the video assumes that your looking at down at the lunar farside from a stationary point above the Moon. Note that the disk of the Moon stays fixed in place. The Moon actually ‘rocks’ or nods back and forth and side-to-side in motions referred to as libration and nutation, and you’re seeing these expressed via the motion of the Earth in the video. This assures that we actually get a peek over the lunar limb and see a foreshadowed extra bit of the lunar farside, with grand 59% of the lunar surface visible from the Earth. Such is the wacky motion of our Moon, which gave early astronomers an excellent crash course in celestial mechanics 101.

Now, to dispel some commonly overheard lunar myths:

Myth #1: The moon doesn’t rotate. Yes, it’s tidally locked from our perspective, meaning that it keeps one face turned Earthward. But it does turn on its axis in lockstep as it does so once every 27.3 days, known as a sidereal month.

Myth #2: The Farside vs. the Darkside. (Cue Pink Floyd) We do in fact see the dark or nighttime side of the Moon just as much as the daytime side. Despite popular culture, the farside is only synonymous with the darkside of the Moon during Full phase.

Humanity got its first glimpse of the lunar farside in 1959, when the Soviet Union’s Luna 3 spacecraft looked back as it flew past the Moon and beamed us the first blurry image. The Russians got there first, which is why the lunar farside now possesses names for features such as the “Mare Moscoviense”.

Think we’ve explored the Moon? Thus far, no mission – crewed or otherwise – has landed on the lunar farside. The Apollo missions were restricted to nearside landing sites at low latitudes with direct line of sight communication with the Earth. The same goes for the lunar poles: the Moon is still a place begging for further exploration.

Why go to the lunar farside? Well, it would be a great place to do some radio astronomy, as you have the bulk of the Moon behind you to shield your sensitive searches from the now radio noisy Earth. Sure, the dilemmas of living on the lunar farside might forever outweigh the benefits, and abrasive lunar dust will definitely be a challenge to lunar living… perhaps an orbiting radio astronomy observatory in a Lissajous orbit at the L2 point would be a better bet?

And exploration of the Moon continues. Earlier this week, the LRO team released a finding suggesting that surface hydrogen may be more abundant on the poleward facing slopes of craters that litter the lunar south pole region. Locating caches of lunar ice in permanently shadowed craters will be key to a ‘living off of the land’ approach for future lunar colonists… and then there’s the idea to harvest helium-3 for nuclear fusion (remember the movie Moon?) that’s still science fiction… for now.

Perhaps the Moonbase Alpha of Space: 1999 never came to pass… but there’s always 2029!

February 5, 2015December 23, 2015 by Ken Kremer

SpaceX Prepares for Crucial Crew Dragon Capsule Pad Abort Test

SpaceX Dragon V2 pad abort test flight vehicle. Credit: SpaceX

SpaceX is preparing for the first of two critical abort tests for the firm’s next generation human rated Dragon V2 capsule as soon as March.

The purpose of the pair of abort tests is to demonstrate a crew escape capability to save the astronauts’ lives in case of a rocket failure, starting from the launch pad and going all the way to orbit.

The SpaceX Dragon V2 and Boeing CST-100 vehicles were selected by NASA last fall for further funding under the auspices of the agency’s Commercial Crew Program (CCP) as the world’s privately developed spaceships to ferry astronauts back and forth to the International Space Station (ISS).

Both SpaceX and Boeing plan to launch the first manned test flights to the ISS with their respective transports in 2017.

During the Sept. 16, 2014, news briefing at the Kennedy Space Center, NASA Administrator Charles Bolden announced that contracts worth a total of $6.8 Billion were awarded to SpaceX to build the manned Dragon V2 and to Boeing to build the manned CST-100.

The first abort test involving the pad abort test is currently slated to take place soon from the company’s launch pad on Cape Canaveral Air Force Station in Florida, according to Gwynne Shotwell, president of SpaceX.

“First up is a pad abort in about a month,” said Shotwell during a media briefing last week at NASA’s Johnson Space Center in Houston, Texas.

SpaceX engineers have been building the pad abort test vehicle for the unmanned test for more than a year at their headquarters in Hawthorne, California.

Dragon V2 builds on and significantly upgrades the technology for the initial cargo version of the Dragon which has successfully flown five operational resupply missions to the ISS.

“It took us quite a while to get there, but there’s a lot of great technology and innovations in that pad abort vehicle,” noted Shotwell.

First look at the SpaceX Crew Dragon’s pad abort vehicle set for flight test in March 2014. Credit: SpaceX.

The pad abort demonstration will test the ability of a set of eight SuperDraco engines built into the side walls of the crew Dragon to pull the vehicle away from the launch pad in a simulated emergency.

The SuperDraco engines are located in four jet packs around the base. Each engine can produce up to 120,000 pounds of axial thrust to carry astronauts to safety, according to a SpaceX description.

Here is a SpaceX video of SuperDraco’s being hot fire tested in Texas:

Video caption: Full functionality of Crew Dragon’s SuperDraco jetpacks demonstrated with hotfire test in McGregor, TX. Credit: SpaceX

For the purpose of this test, the crew Dragon will sit on top of a facsimile of the unpressurized trunk portion of the Dragon. It will not be loaded on top of a Falcon 9 rocket for the pad abort test.

The second abort test involves a high altitude abort test launching atop a SpaceX Falcon 9 rocket from Vandenberg Air Force Base in California.

“An in-flight abort test [follows] later this year,” said Shotwell.

“The Integrated launch abort system is critically important to us. We think it gives incredible safety features for a full abort all the way through ascent.”

“It does also allow us the ultimate goal of fully propulsive landing.”

Both tests were originally scheduled for 2014 as part of the firm’s prior CCiCAP development phase contract with NASA, SpaceX CEO Elon Musk told me in late 2013.

“Assuming all goes well, we expect to conduct [up to] two Dragon abort tests next year in 2014,” Musk explained.

Last year, NASA granted SpaceX an extension into 2015 for both tests under SpaceX’s CCiCAP milestones.

SpaceX founder and CEO Elon Musk briefs reporters, including Universe Today, in Cocoa Beach, FL, during prior SpaceX Falcon 9 rocket blastoff from Cape Canaveral, FL. Credit: Ken Kremer/kenkremer.com — SpaceX founder and CEO Elon Musk briefs reporters, including Universe Today, in Cocoa Beach, FL, during a prior SpaceX Falcon 9 rocket blastoff from Cape Canaveral, FL. Credit: Ken Kremer/kenkremer.com

The SpaceX Dragon V2 will launch atop a human rated Falcon 9 v1.1 rocket from Space Launch Complex 40 at Cape Canaveral.

“We understand the incredible responsibility we’ve been given to carry crew. We should fly over 50 Falcon 9’s before crewed flight,” said Shotwell.

To accomplish the first manned test flight to the ISS by 2017, the US Congress must agree to fully fund the commercial crew program.

“To do this we need for Congress to approve full funding for the Commercial Crew Program,” Bolden said at last week’s JSC media briefing.

Severe budget cuts by Congress forced NASA into a two year delay in the first commercial crew flights to the ISS from 2015 to 2017 – and also forced NASA to pay hundreds of millions of more dollars to the Russians for crews seats aboard their Soyuz instead of employing American aerospace workers.

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

Ken Kremer