Berth of a Dragon after Thruster Failure Recovery Establishes American Lifeline to ISS

SpaceX Dragon berthing at ISS on March 3, 2013. Credit: NASA

Kennedy Space Center – After overcoming a frightening thruster failure that could have spelled rapid doom on the heels of a breathtakingly beautiful launch, the privately developed Dragon spacecraft successfully berthed at the International Space Station (ISS) a short while ago, at 8:56 a.m. EST Sunday morning, March 3, 2013 – thereby establishing an indispensable American Lifeline to the massive orbiting lab complex.

Hearts sank and hopes rose in the span of a few troubling hours following Friday’s (Mar. 1) flawless launch of the Dragon cargo resupply capsule atop the 15 story tall Falcon 9 rocket from Cape Canaveral Air Force Station, Florida and the initial failure of the life giving solar arrays to deploy and failure of the maneuvering thrusters to fire.

“Congrats to the @NASA/@SpaceX team. Great work getting #Dragon to the #ISS…our foothold for future exploration!” tweeted NASA Deputy Administrator Lori Garver.

Space station Expedition 34 crew members Kevin Ford and Tom Marshburn of NASA used the station’s 58 foot long Canadian supplied robotic arm to successfully grapple and capture Dragon at 5:31 a.m. Sunday as the station was flying 253 miles above northern Ukraine. See the grappling video – here.

SpaceX Dragon holding at 10m capture point. ISS crew standing by for "go" to perform grapple. Credit: NASA
SpaceX Dragon holding at 10m capture point. ISS crew standing by for “go” to perform grapple. Credit: NASA

“The vehicle’s beautiful, space is beautiful, and the Canadarm2 is beautiful too”, said station commander Kevin Ford during the operation.

The capsule pluck from free space came one day, 19 hours and 22 minutes after the mission’s launch.

Ground controllers at NASA’s Johnson Space Center in Houston then commanded the arm to install Dragon onto the Earth-facing port of the Harmony module – see schematic.

Schematic shows location of Dragon docking port for CRS-2 mission and ISS modules. Credit: NASA
Schematic shows location of Dragon docking port for CRS-2 mission and ISS modules. Credit: NASA

Originally, Dragon capture was slated only about 20 hours after launch. But that all went out the window following the serious post-launch anomalies that sent SpaceX engineers desperately scrambling to save the flight from a catastrophic finale.

The $133 million mission dubbed CRS-2 is only the 2nd contracted commercial resupply mission ever to berth at the ISS under NASA’s Commercial Resupply Services (CRS) contract. The contract is worth $1.6 Billion for at least a dozen resupply flights.

Following the forced retirement of NASA’s space shuttle orbiters in July 2011, American was left with zero capability to launch either cargo or astronauts to the primarily American ISS. NASA astronauts are 100% reliant on Russian Soyuz capsules for launch to the ISS.

Both the Falcon 9 rocket and Dragon spacecraft were designed and built by SpaceX Corporation based in Hawthorne, Calif., and are entirely American built.

The Falcon 9/Dragon commercial system restores America’s unmanned cargo resupply capability. But the time gap will be at least 3 to 5 years before American’s can again launch to the ISS aboard American rockets from American soil.

And continuing, relentless cuts to NASA’s budget are significantly increasing that human spaceflight gap and consequently forces more payments to Russia.

“Today we marked another milestone in our aggressive efforts to make sure American companies are launching resupply missions from U.S. shores,” said NASA Admisistrator Charles Bolden in a NASA statement.

“Our NASA-SpaceX team completed another successful berthing of the SpaceX Dragon cargo module to the International Space Station (ISS) following its near flawless launch on the Falcon-9 booster out of Cape Canaveral, Florida Friday morning. Launching rockets is difficult, and while the team faced some technical challenges after Dragon separation from the launch vehicle, they called upon their thorough knowledge of their systems to successfully troubleshoot and fully recover all vehicle capabilities. Dragon is now once again safely berthed to the station.”

“I was pleased to watch the launch from SpaceX’s facility in Hawthorne, CA, and I want to congratulate the SpaceX and NASA teams, who are working side by side to ensure America continues to lead the world in space.”

“Unfortunately, all of this progress could be jeopardized with the sequestration ordered by law to be signed by the President Friday evening. The sequester could further delay the restarting of human space launches from U.S. soil, push back our next generation space vehicles, hold up development of new space technologies, and jeopardize our space-based, Earth observing capabilities,” said Bolden.

ISS crew given GO for second stage capture of SpaceX Dragon with ISS on March 3, 2013.  Credit: NASA
ISS crew given GO for second stage capture of SpaceX Dragon with ISS on March 3, 2013. Credit: NASA

Dragon is loaded with about 1,268 pounds (575 kilograms) of vital supplies and provisions to support the ongoing science research by the resident six man crew, including more than a ton of vital supplies, science gear, research experiments, spare parts, food, water and clothing.

NASA says that despite the one-day docking delay, the Dragon unberthing will still be the same day as originally planned on March 25 – followed by a parachute assisted splashdown in the Pacific Ocean off the coast of Baja California.

Dragon will spend 22 days docked to the ISS. The station crew will soon open the hatch and unload all the up mass cargo and research supplies. Then they will pack the Dragon with about 2,668 pounds (1,210 kilograms) of science samples from human research, biology and biotechnology studies, physical science investigations, and education activities for return to Earth.

Canadian built robotic arm grapples SpaceX Dragon on March 3, 2013.  Credit:
Canadian built robotic arm grapples SpaceX Dragon on March 3, 2013. Credit:

Dragon is the only spacecraft in the world today capable of returning significant amounts of cargo to Earth.

Orbital Sciences Corp also won a $1.9 Billion cargo resupply contract from NASA to deliver cargo to the ISS using the firm’s new Antares rocket and Cygnus capsule.

NASA hopes the first Antares/Cygnus demonstration test flight from NASA’s Wallops Island Facility in Virginia will follow in April. Cygnus cargo transport is one way – to orbit only.

“SpaceX is proud to execute this important work for NASA, and we’re thrilled to bring this capability back to the United States,” said Gwynne Shotwell, President of SpaceX.

“Today’s launch continues SpaceX’s long-term partnership with NASA to provide reliable, safe transport of cargo to and from the station, enabling beneficial research and advancements in technology and research.”

The SpaceX CRS-3 flight is slated to blast off in September 2013.

Ken Kremer

Falcon 9 SpaceX CRS-2 launch on March 1, 2013 ISS - shot from the roof of the Vehicle Assembly Building.  .  Credit: Ken Kremer/www.kenkremer.com
Falcon 9 SpaceX CRS-2 launch on March 1, 2013 to the ISS – shot from the roof of the Vehicle Assembly Building. Credit: Ken Kremer/www.kenkremer.com

SpaceX Dragon Recovers from Frightening Propulsion System Failure – Sunday Docking Set

Launch of SpaceX Falcon 9 on CRS-2 mission on March 1, 2013 from Cape Canaveral, Florida. Credit: Jeff Seibert

Kennedy Space Center – Barely 11 minutes after the spectacular Friday morning, March 1 launch of the SpaceX Falcon 9 rocket and unmanned Dragon capsule bound for the International Space Station (ISS), absolute glee suddenly threatened to turn to total gloom when the mission suffered an unexpected failure in the critical propulsion system required to propel the Dragon to the Earth orbiting outpost.

An alarming issue with the Dragons thrust pods prevented three out of four from initializing and firing.

For several hours the outlook for the $133 million mission appeared dire, but gradually began to improve a few hours after launch.

“It was a little frightening,” said SpaceX CEO Elon Musk at a Friday afternoon media briefing for reporters gathered at the Kennedy Space Center, commenting on the moments after the glitch appeared out of nowhere.

“We noticed after separation that only one of the four thruster pods engaged or was ready to engage,” Musk explained. “And then we saw that the oxidizer pressure in three of the four tanks was low.”

Launch of SpaceX Falcon 9 on CRS-2 mission on March 1, 2013 from Cape Canaveral, Florida. Credit: Jeff Seibert
Launch of SpaceX Falcon 9 on CRS-2 mission on March 1, 2013 from Cape Canaveral, Florida. Credit: Jeff Seibert/Wired4Space.com

The situation progressed onto the road to recovery after SpaceX engineers immediately sprang into action and frantically worked to troubleshoot the thruster problems in an urgent bid to try and bring the crucial propulsion systems back on line and revive the mission.

By late Saturday afternoon sufficient recovery work had been accomplished to warrant NASA, ISS and SpaceX managers to give the go-ahead for the Dragon to rendezvous with the station early Sunday morning, March 3.

“The station’s Mission Management Team unanimously agreed that Dragon’s propulsion system is operating normally along with its other systems and ready to support the rendezvous two days after Friday’s launch on a Falcon 9 rocket from the Cape Canaveral Air Force Station in Florida,” NASA announced in a statement on Saturday, March 2.

A failure to ignite the thrusters within 1 or 2 days would have resulted in unacceptable orbital decay and a quick and unplanned fiery reentry into the earth’s atmosphere, said Musk.

Reentry would cause a total loss of the mission – carrying more than a ton of vital supplies, science gear, research experiments, spare parts, food, water and provisions to orbit for the stations six man crew.

Shortly after the Dragon achieved orbit and separated from the second stage, the solar arrays failed to deploy and the live webcast stopped prematurely.

Falcon 9 SpaceX CRS-2 launch on March 1, 2013 ISS - shot from the roof of the Vehicle Assembly Building.  .  Credit: Ken Kremer/www.kenkremer.com
Falcon 9 SpaceX CRS-2 launch on March 1, 2013 to the ISS – shot from the roof of the Vehicle Assembly Building. Credit: Ken Kremer/www.kenkremer.com

During the course of the Friday afternoon briefing, Musk and NASA officials received continuous updates indicating the situating was changing and slowly improving.

Musk confirmed that SpaceX was able to bring all four of Dragon’s thruster pods back up and running. Engineers were able to identify and correct the issue, normalizing the pressure in the oxidation tanks.

The problem may have been caused by stuck valves or frozen oxidizer in the lines. Dragon has four oxidizer tanks and four fuel tanks.

“We think there may have been a blockage of some kind or stuck check valves going from the helium pressure tank to the oxidizer tank,” Musk hypothesized. “Whatever that blockage is seems to have alleviated.”

Three of the four thruster pods must be active before the Dragon would be permitted to dock, said Mike Suffredini, NASA program manager for the ISS. There are a total of 18 Draco thrusters.

SpaceX and the ISS partners conducted a thorough review process to assure that the thrusters will work as advertised and allow the Dragon to safely enter the stations keep out zone and physically dock at the berthing port onto the Earth-facing port of the Harmony module.

“SpaceX said it has high confidence there will be no repeat of the thruster problem during rendezvous, including its capability to perform an abort, should that be required,” NASA said in a statement.

Dragon is now slated to be grappled early Sunday morning at 6:31 a.m. by NASA Expedition 34 Commander Kevin Ford and NASA Flight Engineer Tom Marshburn – that’s one day past the originally planned Saturday morning docking.


Video: Falcon 9 SpaceX CRS-2 launch on March 1, 2013 bound for the ISS – shot from the roof of the Vehicle Assembly Building. Credit: Matthew Travis/Spacearium

NASA says that despite the one-day docking delay, the Dragon unberthing and parachute assisted return to Earth will still be the same day as originally planned on March 25.

There are numerous docking opportunities available in the coming days if SpaceX and NASA determined that more time was needed to gain confidence that Dragon could safely carry out an attempt.

Musk said the Dragon could stay on orbit for several additional months if needed.

We have to review the data with NASA before docking to make sure it’s safe, Musk emphasized on Friday.

Falcon 9 SpaceX CRS-2 launch on March 1, 2013.  Credit: Mike Killian/www.zerognews.com
Falcon 9 SpaceX CRS-2 launch on March 1, 2013. Credit: Mike Killian/www.zerognews.com

The mission dubbed CRS-2 will be only the 2nd commercial resupply mission ever to berth at the ISS. SpaceX is under contract to NASA to conduct a dozen Dragon resupply flight to the ISS over the next few years at a cost of about $1.6 Billion.

NASA TV coverage of rendezvous and grapple on Sunday, March 3 will begin at 3:30 a.m. EST. Coverage of berthing operations on NASA TV will begin at 8 a.m.

SpaceX’s live coverage at http://www.spacex.com/webcast begins at 6:00 a.m. Eastern.

Ken Kremer

Falcon 9 SpaceX CRS-2 launch on March 1, 2013.  Credit: Mike Killian/www.zerognews.com
Falcon 9 SpaceX CRS-2 launch on March 1, 2013. Credit: Mike Killian/www.zerognews.com

SpaceX Commercial Rocket Poised for March 1 Blast Off to ISS

SpaceX Falcon 9 rocket before May 2012 blast off from Cape Canaveral Air Force Station, Florida on historic maiden private commercial launch to the ISS. Credit: Ken Kremer/www.kenkremer.com

Kennedy Space Center – All systems are GO and the weather outlook looks spectacular for the March 1 blast off of the privately developed SpaceX Falcon 9 rocket to the International Space Station (ISS).

The Falcon 9 is slated to lift off at 10:10 AM EST with a Dragon capsule loaded with fresh supplies and science gear to continued full up operation and utilization of the ISS.

Right now the weather forecast is at 80% GO on March 1 – with superbly beautiful, clear blue skies here in sunny and comfortably warm Florida from Space Launch Complex 40 at Cape Canaveral Air Force Station.

Large crowds of eager tourists, sightseers and space enthusiasts are already gathering in local hotels – most are sold out including at my hotel where I have been holding well attended ISS star parties during excellent evening viewing opportunities this week.

NASA TV will provide live launch coverage starting at 8 30 AM. SpaceX will also provide a separate feed starting about 40 minutes prior to launch.

The two stage Falcon 9 rocket was rolled out horizontally to the pad late this afternoon (Thursday, Feb. 28) in anticipation of a Friday morning launch. Myself and Dave Dickinson are on-site for Universe Today

The mission dubbed CRS-2 will be only the 2nd commercial resupply mission ever to the ISS.

There are no technical concerns at this time. Saturday March 2 is the back-up launch date in case of a last second scrub. Weather is projected as 80% favorable.

SpaceX President Gwynne Shotwell and NASA officials told me that additional launch opportunities are available Sunday, Monday and Tuesday, if needed, and later until about March 11. After that, the launch team would have to stand down to make way for the next eventual departure of a docked Soyuz and launch of a manned Russian Soyuz capsule with a new three man crew.

SpaceX Falcon 9 rocket liftoff on May 22, 2012 from Space Launch Complex-40 at Cape Canaveral Air Force Station, Fla., on the first commercial mission to the International Space Station.  Credit: Ken Kremer
SpaceX Falcon 9 rocket liftoff on May 22, 2012 from Space Launch Complex-40 at Cape Canaveral Air Force Station, Fla., on the first commercial mission to the International Space Station. Credit: Ken Kremer

The SpaceX Dragon capsule is carrying about 1,200 pounds of vital supplies and research experiments for the six man international crew living aboard the million pound orbiting outpost.

SpaceX is under contract to NASA to deliver over 44,000 pounds of cargo to the ISS during a dozen flights over the next few years at a cost of about $1.6 Billion.

The capsule is fully loaded Shotwell told me. An upgraded Falcon 9 will be used in the next launch that will allow for a significant increase in the cargo up mass, Shotwell elaborated.

The Dragon is due to dock with the ISS in record time some 20 hours after blast off.

Ken Kremer

How Will Sequestration Affect NASA?

NASA Administrator Charles Bolden addresses the media at SpaceX's main hangar in Cape Canaveral, FL. The sequester will affect both NASA and SpaceX. Credit: NASA.

It seems the US in not going to avoid the sequester — the $85 billion worth of federal spending cuts due to kick in March 1, 2013. There will be across the board cuts to government agencies, applying equally to defense and non-defense spending, and will affect services from meat inspections to air traffic control. In some cases, federal workers will be furloughed or could stand to lose as much as 20 percent of their pay. One question no one can answer is how long it will take for Congress and the Obama administration to come to an agreement on a package that would reduce the deficit.

But in the near term, how will it affect NASA?

“Sequestration would significantly set back the ambitious space exploration plan the President and Congress have asked NASA to carry out,” NASA Administrator Charlie Bolden said in a message to NASA employees this week. “These damaging cuts would slash roughly 5 percent from the agency’s current annual budget during the remaining seven months of the 2013 fiscal year, a loss of about $726 million from the President’s budget request. This could further delay the restarting of human space launches from U.S. soil, push back our next generation space vehicles, and hold up development of new space technologies.

In hard numbers, NASA’s overall budget would drop to $16.9 billion, down from the $17.8 billion Congress approved last year.

NASA civil servants are safe from furloughs, but NASA contractors will see cuts in their contracts.

In a press conference on Feb. 28, preceding the scheduled March 1 launch of the SpaceX Dragon capsule to the ISS, NASA’s Space Station Manager Mike Suffredini said the ISS would not be impacted very much. With humans on board the ISS, there can be no cuts in operations that would endanger the crew. While Sufferdini didn’t say so, if the cuts continue long-term to NASA, there likely would be an impact to science being done, and perhaps eventually crew size.

Spending on the commercial crew program might take one of the biggest hits, and would be reduced to $388 million, which is $18 million less than it is currently spending and $441.6 million less than the agency had been planning to spend in 2013. Boeing, Sierra Nevada, and SpaceX are all under contract to meet performance milestones to deliver cargo and ultimately crew (by 2017) to the International Space Station.

In a separate letter to Senate Appropriations Committee Chairwoman Barbara Mikulski, (D-MD) Bolden said NASA’s commercial crew partners would be affected by this summer, as NASA would no longer be able to fund upcoming events such as a test of Boeing’s CST-100 orbital maneuvering and attitude control engine in July, a September review of an in-flight abort test SpaceX plans to conduct in April 2014, and an October integrated system and safety analysis review of Sierra Nevada’s DreamChaser space plane.

Also at the SpaceX press conference on Feb. 28, SpaceX President Gwynne Shotwell said the specifics of how the sequestration will affect her company is not yet known, but it will likely impact some of their milestones if the budget issues aren’t resolved soon.

Howard Bloom, founder of the Space Development Steering Committee, said these cuts to commercial crew would be a disaster, delaying when US astronauts could launch on US rockets, and would just “shovel” money to Russia.

“This nip and tuck may result in a period of an additional one to two years in which America cannot get astronauts to the International Space Station on our own launch vehicles,” he said in a statement sent to Universe Today. “But we are committed to manning the Space Station. How will we do it? Using Russian Soyuz capsules. At a price of $63 million paid to the Russians for each American passenger– a total of $350-400 million per year.”

Even worse, Bloom said, sequestration could eliminate one of more of the companies working on American launch vehicles, and the result would be “less competition and a potentially higher cost per launch once a new vehicle comes into service.”

Science and research will also be affected, with reductions of $51.1 million below the FY 2013 budget request for astrophysics and science, meaning funding for new missions such as Explorer and Earth Venture Class will be cut, decreasing mission selections by 10 to 15 percent, resulting in lower funding levels for new activities and causing some launch delays. There will also be a reduction in the number of science flight opportunities such as those for college and high school students, and the elimination of Centennial Challenges funding to for any new prizes.

NASA’s Space Technology Program would be cut by $24 million to $550 million instead of $699 million, and any updates or construction at NASA facilities would be centers would be canceled. This may impact updates at Kennedy Space Center for infrastructure needed for NASA’s Space Launch System (SLS), the Orion Multi-Purpose Crew Vehicle, and other programs.

As far as other science programs in the US there are reports that at least 1,000 National Science Foundation grants will be cut, and the National Institute of Health will lose $3.1 billion.

“We will continue to keep you informed as we learn more about issues surrounding the potential sequestration,” Bolden said in his email to NASA employees. Dr. Elizabeth Robinson, Agency Chief Financial Officer, and her staff in the Office of the Chief Financial Officer here at NASA HQ will be following up with the Officials in Charge regarding our plans for implementing sequestration and how those plans will affect NASA’s day-to-day operations. Please feel free to contact her or her staff with questions or concerns.”

Sources: NBC, AeroNews, Space Industry News.

A New Look at Saturn’s Northern Hexagon

Raw Cassini image captured on 26 Feb. 2013 (NASA/JPL/SSI)

Freshly delivered from Cassini’s wide-angle camera, this raw image gives us another look at Saturn’s north pole and the curious hexagon-shaped jet stream that encircles it, as well as the spiraling vortex of clouds at its center.

Back in November we got our first good look at Saturn’s north pole in years, now that Cassini’s orbit is once again taking it high over the ringplane. With spring progressing on Saturn’s northern hemisphere the upper latitudes are getting more and more sunlight — which stirs up storm activity in its atmosphere.

The bright tops of upper-level storm clouds speckle Saturn’s skies, and a large circular cyclone can be seen near the north pole, within the darker region contained by the hexagonal jet stream. This could be a long-lived storm, as it also seems to be in the images captured on November 27.

About 25,000 km (15,500 miles) across, Saturn’s hexagon is wide enough to fit nearly four Earths inside!

The Saturn hexagon as seen by Voyager 1 in 1980 (NASA)
The Saturn hexagon as seen by Voyager 1 in 1980 (NASA)

The hexagon was originally discovered in images taken by the Voyager spacecraft in the early 1980s. It encircles Saturn at about 77 degrees north latitude and is estimated to whip around the planet at speeds of 354 km/h (220 mph.)

Watch a video of the hexagon in motion here.

The rings can be seen in the background fading into the shadow cast by the planet itself. A slight bit of ringshine brightens Saturn’s nighttime limb.

Cassini was approximately 579,653 kilometers (360,180 miles) from Saturn when the raw image above (W00079643) was taken.

Image credit: NASA/JPL/Space Science Institute

 

Curiosity Mars Rover Eats 1st Sample of Gray Rocky Powder

NASA's Mars rover Curiosity took this image of Curiosity's sample-processing and delivery tool just after the tool delivered a portion of powdered rock into the rover's Sample Analysis at Mars (SAM) instrument. This Collection and Handling for In-situ Martian Rock Analysis (CHIMRA) tool delivered portions of the first sample ever acquired from the interior of a rock on Mars into both SAM and the rover's Chemistry and Mineralogy (CheMin) instrument. Credit: NASA/JPL-Caltech/MSSS

NASA’s Curiosity rover has eaten the 1st ever samples of gray rocky powder cored from the interior of a Martian rock.

The robotic arm delivered aspirin sized samples of the pulverized powder to the rover’s Chemistry and Mineralogy (CheMin) and Sample Analysis at Mars (SAM) instruments this past weekend on Feb. 22 and 23, or Sols 195 and 196 respectively.

Both of Curiosity’s chemistry labs have already begun analyzing the samples – but don’t expect results anytime soon because of the complexity of the operation involved.

“Analysis has begun and could take weeks,’ NASA JPL spokesman Guy Webster told Universe Today.

The samples were collected from the rover’s 1st drilling site known as ‘John Klein’ – comprised of a red colored slab of flat, fine-grained, sedimentary bedrock shot through with mineral veins of Calcium Sulfate that formed in water.

“Data from the instruments have confirmed the deliveries,” said Curiosity Mission Manager Jennifer Trosper of NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

On Feb. 8, 2013 (mission Sol 182), Curiosity used the rotary-percussion drill mounted on the tool turret at the end of the 7 foot (2.1 meter) long robotic arm to bore a circular hole about 0.63 inch (16 mm) wide and about 2.5 inches (64 mm) deep into ‘John Klein’ that produced a slurry of gray tailings

Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals - dramatically back dropped with  her ultimate destination; Mount Sharp.  Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals – dramatically back dropped with her ultimate destination; Mount Sharp. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

The gray colored tailings give a completely fresh insight into Mars that offers a stark contrast to the prevailing views of reddish-orange rusty, oxidized dust.

The eventual results from SAM and CheMin may give clues about what exactly does the color change mean. One theory is that it might be related to different oxidations states of iron that could potentially inform us about the habitability of Mars insides the rover’s Gale Crater landing site.

“The rock drilling capability is a significant advancement. It allows us to go beyond the surface layer of the rock, unlocking a time capsule of evidence about the state of Mars going back 3 or 4 Billion years,” said Louise Jandura of JPL and Curiosity’s chief engineer for the sampling system.

Additional portions of the first John Klein sample could be delivered to SAM and CheMin if the results warrant. The state-of-the-art instruments are testing the gray powder to elucidate the chemical composition and search for simple and complex organic molecules based on carbon, which are the building blocks of life as we know it.

Curiosity’s Mastcam camera snapped this photo mosaic of 1st drill holes into Martian rock at John Klein outcrop inside Yellowknife Bay basin where the robot is currently working. Notice the gray powdery tailings from the rocks interior. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
Curiosity’s Mastcam camera snapped this photo mosaic of 1st drill holes into Martian rock at John Klein outcrop inside Yellowknife Bay basin where the robot is currently working. Notice the gray powdery tailings from the rocks interior. Credit: NASA/JPL-Caltech/MSSS/Ken Kremer/Marco Di Lorenzo

The Curiosity science team believes that this work area inside Gale Crater called Yellowknife Bay, experienced repeated percolation of flowing liquid water long ago when Mars was warmer and wetter – and therefore was potentially more hospitable to the possible evolution of life.

Curiosity is nearly 7 months into her 2 year long primary mission. So far she has snapped over 45,000 images.

“The mission is discovery driven,” says John Grotzinger, the Curiosity mission’s chief scientist of the California Institute of Technology.

The rover will likely remain in the John Klein area for several more weeks to a month or more to obtain a more complete scientific characterization of the area which has seen repeated episodes of flowing water.

Eventually, the six-wheeled mega rover will set off on a nearly year long trek to her main destination – the sedimentary layers of the lower reaches of the 3 mile (5 km) high mountain named Mount Sharp – some 6 miles (10 km) away.

Ken Kremer

European Asteroid Smasher Could Bolster Planetary Defense

US-European Asteroid Impact and Deflection mission – AIDA.

Planetary Defense is a concept very few people heard of or took seriously – that is until last week’s humongous and totally unexpected meteor explosion over Russia sent millions of frightened residents ducking for cover, followed just hours later by Earth’s uncomfortably close shave with the 45 meter (150 ft) wide asteroid named 2012 DA14.

This ‘Cosmic Coincidence’ of potentially catastrophic space rocks zooming around Earth is a wakeup call that underscores the need to learn much more about the ever present threat from the vast array of unknown celestial debris in close proximity to Earth and get serious about Planetary Defense from asteroid impacts.

The European Space Agency’s (ESA) proposed Asteroid Impact and Deflection Assessment mission, or AIDA, could significantly bolster both our basic knowledge about asteroids in our neighborhood and perhaps even begin testing Planetary Defense concepts and deflection strategies.

After two years of work, research teams from the US and Europe have selected the mission’s target – a so called ‘binary asteroid’ named Didymos – that AIDA will intercept and smash into at about the time of its closest approach to Earth in 2022 when it is just 11 million kilometers away.

“AIDA is not just an asteroid mission, it is also meant as a research platform open to all different mission users,” says Andres Galvez, ESA studies manager.

Asteroid Didymos could provide a great platform for a wide variety of research endeavors because it’s actually a complex two body system with a moon – and they orbit each other. The larger body is roughly 800 meters across, while the smaller one is about 150 meters wide.

Didymos with its Moon
Didymos with its Moon. Credit: ESA

So the smaller body is some 15 times bigger than the Russian meteor and 3 times the size of Asteroid 2012 DA14 which flew just 27,700 km (17,200 mi) above Earth’s surface on Feb. 15, 2013.

The low cost AIDA mission would be comprised of two spacecraft – a mother ship and a collider. Two ships for two targets.

The US collider is named the Double Asteroid Redirection Test, or DART and would smash into the smaller body at about 6.25 km per second. The impact should change the pace at which the objects spin around each other.

ESA’s mothership is named Asteroid Impact Monitor, or AIM, and would carry out a detailed science survey of Didymos both before and after the violent collision.

“The project has value in many areas,” says Andy Cheng, AIDA lead at Johns Hopkins’ Applied Physics Laboratory, “from applied science and exploration to asteroid resource utilisation.” Cheng was a key member of NASA’s NEAR mission that first orbited and later landed on the near Earth Asteroid named Eros back in 2001.

Recall that back in 2005, NASA’s Deep Impact mission successfully lobbed a projectile into Comet Tempel 1 that unleashed a fiery explosion and spewing out vast quantities of material from the comet’s interior, including water and organics.

NASA’s Deep Impact images Comet Tempel 1 alive with light after colliding with the impactor spacecraft on July 4, 2005.  ESA and NASA are now proposing the AIDA mission to smash into Asteroid Didymos.  CREDIT: NASA/JPL-Caltech/UMD
NASA’s Deep Impact images Comet Tempel 1 alive with light after colliding with the impactor spacecraft on July 4, 2005. ESA and NASA are now proposing the AIDA mission to smash into Asteroid Didymos. CREDIT: NASA/JPL-Caltech/UMD

ESA has invited researchers to submit AIDA experiment proposals on a range of ideas including anything that deals with hypervelocity impacts, planetary science, planetary defense, human exploration or innovation in spacecraft operations. The deadline is 15 March.

“It is an exciting opportunity to do world-leading research of all kinds on a problem that is out of this world,” says Stephan Ulamec from the DLR German Aerospace Center. “And it helps us learn how to work together in international missions tackling the asteroid impact hazard.”

The Russian meteor exploded without warning in mid air with a force of nearly 500 kilotons of TNT, the equivalent of about 20–30 times the atomic bombs detonated at Hiroshima and Nagasaki.

Over 1200 people were injured in Russia’s Chelyabinsk region and some 4000 buildings were damaged at a cost exceeding tens of millions of dollars. A ground impact would have decimated cities like New York, Moscow or Beijing with millions likely killed.

ESA’s AIDA mission concept and NASA’s approved Osiris-REx asteroid sample return mission will begin the path to bolster our basic knowledge about asteroids and hopefully inform us on asteroid deflection and Planetary Defense strategies.

Ken Kremer

Near-Earth asteroid Eros imaged from NASA’s orbiting NEAR spacecraft. Credit: NASA
Near-Earth asteroid Eros imaged from NASA’s orbiting NEAR spacecraft. Credit: NASA

Historic Mars Rock Drilling Sample Set for Analysis by Curiosity Robot in Search of Organics

First Curiosity Drilling Sample in the Scoop. This image shows the first sample of powdered rock extracted by the rover's drill after transfer from the drill to the rover's scoop. The sample will now be sieved and portions delivered to the Chemistry and Mineralogy instrument and the Sample Analysis at Mars instrument. The scoop is 1.8 inches (4.5 centimeters) wide. The image was taken by Curiosity's Mastcam 34 camera on Feb. 20, or Sol 193.The image has been white-balanced to show what the sample would look like if it were on Earth. Credit: NASA/JPL-Caltech/MSSS

Newly received images from the surface of Mars confirm that NASA’s Curiosity rover successfully extracted the 1st ever samples collected by drilling down inside a rock on another planet and transferred the pulverized alien powder to the robots processing scoop, thrilled mission scientists announced just hours after seeing visual corroboration.

Collecting the 1st particles bored from the interior of a rock on a planet beyond Earth marks a historic feat in humankind’s exploration of the cosmos – and is crucial for achieving Curiosity’s goal to determine whether Mars ever could have supported microbial life, past or present.

The essential next step is to feed carefully sieved portions of the precious gray colored material into the high powered duo of miniaturized analytical chemistry labs (CheMin & SAM) inside the rover, for thorough analysis and scrutiny of their mineral content and to search for signatures of organic molecules – the building blocks of life as we know it.

Curiosity is drilling into ancient bedrock and hunting for clues to the planet’s habitability over the eons and that preserve the historical record – perhaps including organics.

The rover team believes that this work area inside Gale Crater called Yellowknife Bay, experienced repeated percolation of flowing liquid water long ago when Mars was warmer and wetter – and therefore was potentially more hospitable to the possible evolution of life. See our Yellowknife Bay worksite and drill hole photo mosaics below by Ken Kremer & Marco Di Lorenzo, created from rover raw images.

Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals - dramatically back dropped with  her ultimate destination; Mount Sharp.  Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo
Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals – dramatically back dropped with her ultimate destination; Mount Sharp. Credit: NASA/JPL-Caltech/Ken Kremer (kenkremer.com)/Marco Di Lorenzo

“We collected about a tablespoon of powder, which meets our expectations and is a great result,” said JPL’s Scott McCloskey, drill systems engineer for Curiosity, at a NASA media briefing on Feb. 20. “We are all very happy and relieved that the drilling was a complete success.”

The gray colored tailings from the rocky interior offer a startlingly fresh sight of Mars compared to the red-orangey veneer of rusty, oxidized dust we are so accustomed to seeing globally across what we humans have referred to for centuries as the “Red Planet”.

“For the first time we are examining ancient rocks that have not been exposed to the Martian surface environment, and weathering, and preserve the environment in which they formed,” said Joel Hurowitz, Curiosity sampling system scientist of JPL.

This is a key point because subsequent oxidation reactions can destroy organic molecules and thereby potential signs of habitability and life.

“The tailings are gray. All things being equal it’s better to have a gray color than red because oxidation is something that can destroy organic compounds,” said John Grotzinger, the Curiosity mission’s chief scientist of the California Institute of Technology.

On Feb. 8, 2013 (mission Sol 182), Curiosity used the rotary-percussion drill mounted on the tool turret at the end of the 7 foot (2.1 meter) long robotic arm to bore a circular hole about 0.63 inch (16 mm) wide and about 2.5 inches (64 mm) deep into a red colored slab of flat, fine-grained, veiny sedimentary bedrock named “John Klein” that formed in water.

“Curiosity’s first drill hole at the John Klein site is a historic moment for the MSL mission, JPL, NASA and the United States. This is the first time any robot, fixed or mobile, has drilled into a rock to collect a sample on Mars,” said Louise Jandura, Curiosity’s chief engineer for the sampling system.

“In fact, this is the first time any rover has drilled into a rock to collect a sample anywhere but on Earth. In the five decade history of the space age this is indeed a rare event.”

“The rock drilling capability is a significant advancement. It allows us to go beyond the surface layer of the rock, unlocking a time capsule of evidence about the state of Mars going back 3 or 4 Billion years.”

“Using our roving geologist Curiosity, the scientists can choose the rock, get inside the rock and deliver the powdered sample to instruments on the rover for analysis.”

“We couldn’t all be happier as Curiosity drilled her first hole on Mars,” said Jandura.

Over the next few days, the powdery gray scoop material will be shaken and moved through Curiosity’s sample processing device known as CHIMRA, or Collection and Handling for In-Situ Martian Rock Analysis and sieved through ultra fine screens that filter out particles larger than 150 microns (0.006 inch) across – about the width of a human strand of hair.

Figure shows the location of CHIMRA on the turret of NASA's Curiosity rover, together with a cutaway view of the device. The CHIMRA, short for Collection and Handling for In-situ Martian Rock Analysis, processes samples from the rover's scoop or drill and delivers them to science instruments. Credit: NASA/JPL-Caltech
Figure shows the location of CHIMRA on the turret of NASA’s Curiosity rover, together with a cutaway view of the device. The CHIMRA, short for Collection and Handling for In-situ Martian Rock Analysis, processes samples from the rover’s scoop or drill and delivers them to science instruments. Credit: NASA/JPL-Caltech

Drilling goes to the heart of the mission. It is absolutely indispensable for collecting and conveying pristine portions of Martian rocks and soil to a trio of inlet ports on top of the rover deck leading into the Chemistry and Mineralogy (CheMin) instrument and Sample Analysis at Mars (SAM) instrument .

The sieving process is designed to prevent clogging downstream into the chemistry labs.

The pair of state-of-the-art instruments will then test the gray rocky powder for a variety of inorganic minerals as well as both simple and complex organic molecules.

Samples will be dropped off first to CheMin and then SAM over the next few days. Results are expected soon.

The data so far indicate the drilled rock is either siltstone or mudstone with a basaltic bulk composition, said Hurowitz. The CheMin and SAM testing will be revealing.

The high powered drill was the last of Curiosity 10 instruments still to be checked out and put into full operation and completes the robots commissioning phase.

“This is a real big turning point for us as we had a passing of the key for the rover [from the engineering team] to the science team,” said Grotzinger.

Curiosity has discovered that Yellowknife Bay is loaded with hydrated mineral veins of calcium sulfate that precipitated from interaction with aqueous environments.

I asked how was the drill target hole selected?

“We wanted to be well centered in a large plate of bedrock where we knew we could place the drill into a stable location on an interesting rock,” Hurowitz told Universe Today.

“The drill did not specifically target the veins or nodular features visible in this rock. But these rocks are so shot through with these features that it’s hard to imagine that we would have been missed them somewhere along the travel of the drill.”

“We will find out what’s in the material once we get the materials analyzed by SAM and CheMin.

“We will consider additional drill targets if we think we missed a component of the rock.”

“We believe the white vein material is calcium sulfate based on data from ChemCam and APXS but we don’t yet know the hydration state.” Hurowitz told me.

Regarding the prospects for conducting additional sample drilling and soil scooping at Yellowknife Bay, Grotzinger told me, “We have to take it one step at a time.”

“We have to see what we find in the first sample. We are discovery driven and that will determine what we do next here,” Grotzinger said. “We have no quotas.”

The long term mission goal remains to drive to the lower reaches of Mount Sharp some 6 miles away and look for habitable environments in the sedimentary layers.

Curiosity executed a flawless and unprecedented nail-biting, pinpoint touchdown on Aug. 5, 2012 to begin her 2 year long primary mission inside Gale Crater. So far she has snapped over 45,000 images, traveled nearly 0.5 miles, conducted 25 analysis with the APXS spectrometer and fired over 12,000 laser shots with the ChemCam instrument.

Ken Kremer

Image collage show Curiosty’s first bore hole drilled on Feb. 8, 2013 (Sol 182). Credit: NASA/JPL-Caltech/MSSS/Marco Di Lorenzo/KenKremer (kenkremer.com)
Image collage show Curiosty’s first bore hole drilled on Feb. 8, 2013 (Sol 182). Credit: NASA/JPL-Caltech/MSSS/Marco Di Lorenzo/KenKremer (kenkremer.com)
Curiosity's First Sample Drilling hole is shown at the center of this image in a rock called "John Klein" on Feb. 8, 2013, or Sol 182 operations. The image was obtained by Curiosity’s Mars Hand Lens Imager (MAHLI). The sample-collection hole is 0.63 inch (1.6 centimeters) in diameter and 2.5 inches (6.4 centimeters) deep. The “mini drill” test hole near it is the same diameter, with a depth of 0.8 inch (2 centimeters). Credit: NASA/JPL-Caltech/MSSS
Curiosity’s First Sample Drilling hole is shown at the center of this image in a rock called “John Klein” on Feb. 8, 2013, or Sol 182 operations. The image was obtained by Curiosity’s Mars Hand Lens Imager (MAHLI). The sample-collection hole is 0.63 inch (1.6 centimeters) in diameter and 2.5 inches (6.4 centimeters) deep. The “mini drill” test hole near it is the same diameter, with a depth of 0.8 inch (2 centimeters). Credit: NASA/JPL-Caltech/MSSS

Scientist Who Studied Famous Martian Meteorite Passes Away

NASA scientists David. S. McKay. Credit: NASA

NASA scientist, Dr. David S. McKay has passed away. He may be best known for his paper about a Martian meteorite, ALH84001, which presented an argument that it contained evidence for life on Mars. McKay had been battling serious cardiac health problems for some time, according to an announcement from Johnson Space Center, and he died peacefully in his sleep in the early morning hours of February 20, 2013.

McKay had been the Chief Scientist For Astrobiology at NASA and searched for evidence of past life on Mars using Martian meteorites and terrestrial analogs. He performed original research on lunar soils, lunar pyroclastics, and space weathering.

McKay joined NASA in June of 1965 and participated extensively in astronaut training up until the Apollo 11 mission. He was named a Principal Investigator to study the first returned lunar samples and continued as a lunar sample PI for the next 20 years. He started many of the laboratories for the Lunar Sample Facility at Johnson Space Center and managed the NASA space resources program out of JSC during much of the 1980s.

McKay published more than 200 peer-reviewed papers on lunar samples, space resource utilization, cosmic dust, meteorites, astrobiology and Mars topics, and NASA said his “body of work includes many contributions to our understanding of the development and evolution of the lunar regolith and space weathering processes.”

Most notably, he was the lead author on the 1996 paper in Science on the ALH84001 Martian meteorite that was found in Antarctica and argued that it contains evidence for life on Mars.

“Although that claim was highly controversial, there can be no question that the appearance of that paper sparked significant changes in martian and planetary science, shaped the direction of the Mars Exploration Program to the present day, and prompted the establishment of the NASA Astrobiology Institute,” said the JSC announcement. “Whether one accepts their arguments or not, it has led, directly or indirectly, to investigations seeking and finding signs of life in the most extreme environments. History will judge the value of that rather serendipitous outcome, but it seems clear that its significance is, and will remain, great.”

Read more about McKay here.

Take a Spin Around Mercury

Color map of Mercury's varied surface. The 1,550-km-wide Caloris Basin can be seen at upper right.

Created by the MESSENGER mission team at the Johns Hopkins University Applied Physics Laboratory and the Carnegie Institution of Washington, this animation gives us a look at the spinning globe of Mercury, its surface color-coded to reflect variations in surface material reflectance.

Thousands of Wide Angle Camera images of Mercury’s surface were stitched together to create the full-planet views.

While the vibrant colors don’t accurately portray Mercury as our eyes would see it, they are valuable to scientists as they highlight the many different types of materials that make up the planet’s surface. Young crater rays surrounding fresh impact craters appear light blue or white. Medium- and dark-blue “low-reflectance material” (LRM) areas are thought to be rich in a dark, opaque mineral. Tan areas are plains formed by eruption of highly fluid lavas. Small orange spots are materials deposited by explosive volcanic eruptions.

At this point, over 99% of the Solar System’s innermost planet has been mapped by MESSENGER. Read more about the ongoing mission here.

Image/video credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington