The International Space Station. Credit: NASA
Thursday, March 28, 2013
Tuesday, March 26, 2013
Monday, March 25, 2013
Sunday, March 24, 2013
AIRCRAFT TO SURVEY POLAR ICE
FROM: NASA
P-3B Starts the Day
On March 21, 2013, the P-3B waits outside the hangar at Thule Air Base with the Greenland Ice sheet in the background.
IceBridge, a six-year NASA mission, is the largest airborne survey of Earth's polar ice ever flown. It will yield an unprecedented three-dimensional view of Arctic and Antarctic ice sheets, ice shelves and sea ice. These flights will provide a yearly, multi-instrument look at the behavior of the rapidly changing features of the Greenland and Antarctic ice.
Data collected during IceBridge will help scientists bridge the gap in polar observations between NASA's Ice, Cloud and Land Elevation Satellite (ICESat) -- in orbit since 2003 -- and ICESat-2, planned for early 2016. ICESat stopped collecting science data in 2009, making IceBridge critical for ensuring a continuous series of observations.
IceBridge will use airborne instruments to map Arctic and Antarctic areas once a year. IceBridge flights are conducted in March-May over Greenland and in October-November over Antarctica. Other smaller airborne surveys around the world are also part of the IceBridge campaign.
Image Credit: NASA/Goddard/Michael Studinger
Saturday, March 23, 2013
STATE DEPARTMENT REMARKS ON U.S.-INDIA SPACE COOPERATION
FROM: U.S. STATE DEPARTMENT
U.S.-India Space Cooperation
Remarks
Geoffrey Pyatt
Principal Deputy Assistant Secretary, Bureau of South and Central Asian Affairs
U.S.-India Civil Space Joint Working Group
Washington, DC
March 21, 2013
Good morning everyone. It’s an enormous privilege to welcome Administrator Bolden, Ambassador Rao, the Indian delegation, and our colleagues from the Indian Embassy, NASA, NOAA, and the State Department here in Washington to this Joint Working Group.
The United States and India are leaders in earth observation. We’re excited to see how this working group can build on joint activities using U.S. and Indian earth observation satellites to better understand earth systems and provide information to improve economies and lives.
We also should seek to increase our commercial space cooperation and create opportunities for U.S. and Indian companies.
And our very capable space science communities have much to offer each other through collaboration. India’s first Indian Mars Orbiter Mission, slated for October 2013, is an exciting opportunity for U.S.-India collaboration.
Being here at this working group this morning is a particular pleasure for me, as I’ve been working for many years on helping make this sort of cooperation possible. Thanks to visionary, bipartisan U.S. and Indian leadership, we’ve recognized how much we have to offer each other and have made great strides in the past decade in bringing our scientific and technical communities together.
The hard work on both sides in transforming our interactions with each other has allowed successes such as including U.S. instruments on India’s Chandrayaan-1 lunar mission -- a path-finding step to show our two systems how to work together, as well as a fruitful scientific endeavor pointing out the promise of this cooperation. More recently, the removal of ISRO subordinate entities from the Entity List at the 2011 Civil Space Joint Working Group meeting and additional measures taken since have further expanded the possibilities for trade and cooperation in civil space.
In January, President Obama signed into law the National Defense Authorization Act, which includes satellite export reform measures expected to expedite trade in space technology.
U.S.-India science and technology builds on a relationship that is robust and vibrant. The U.S.-India Science and Technology Endowment Fund, established in 2009 and with an annual budget of $2 to $3 million, is a landmark in our belief to work together to promote commercialization of innovative technologies.
This collaboration on innovation across a wide range of disciplines is generating new jobs for our people and helping to address many of the globe’s big challenges.
Our space cooperation has become a signature aspect of this science, technology, and innovation cooperation, highlighting both the constancy of our mutual respect and appreciation for each others’ capabilities through the decades, as well as the vast potential – dare I say universal? -- opened up by the changes in our relationship.
I congratulate all of you – the experts and practitioners from both our countries – for your participation in building closer ties in space exploration, space science, earth observation, and launch and ensuring the safety and security of outer space activities. I know your efforts this week will further the cooperation that expands our collective knowledge, brings practical benefits to our citizens, and helps us plan for our future. I wish you all the best in this meeting of the Civil Space Joint Working Group.
U.S.-India Space Cooperation
Remarks
Geoffrey Pyatt
Principal Deputy Assistant Secretary, Bureau of South and Central Asian Affairs
U.S.-India Civil Space Joint Working Group
Washington, DC
March 21, 2013
Good morning everyone. It’s an enormous privilege to welcome Administrator Bolden, Ambassador Rao, the Indian delegation, and our colleagues from the Indian Embassy, NASA, NOAA, and the State Department here in Washington to this Joint Working Group.
The United States and India are leaders in earth observation. We’re excited to see how this working group can build on joint activities using U.S. and Indian earth observation satellites to better understand earth systems and provide information to improve economies and lives.
We also should seek to increase our commercial space cooperation and create opportunities for U.S. and Indian companies.
And our very capable space science communities have much to offer each other through collaboration. India’s first Indian Mars Orbiter Mission, slated for October 2013, is an exciting opportunity for U.S.-India collaboration.
Being here at this working group this morning is a particular pleasure for me, as I’ve been working for many years on helping make this sort of cooperation possible. Thanks to visionary, bipartisan U.S. and Indian leadership, we’ve recognized how much we have to offer each other and have made great strides in the past decade in bringing our scientific and technical communities together.
The hard work on both sides in transforming our interactions with each other has allowed successes such as including U.S. instruments on India’s Chandrayaan-1 lunar mission -- a path-finding step to show our two systems how to work together, as well as a fruitful scientific endeavor pointing out the promise of this cooperation. More recently, the removal of ISRO subordinate entities from the Entity List at the 2011 Civil Space Joint Working Group meeting and additional measures taken since have further expanded the possibilities for trade and cooperation in civil space.
In January, President Obama signed into law the National Defense Authorization Act, which includes satellite export reform measures expected to expedite trade in space technology.
U.S.-India science and technology builds on a relationship that is robust and vibrant. The U.S.-India Science and Technology Endowment Fund, established in 2009 and with an annual budget of $2 to $3 million, is a landmark in our belief to work together to promote commercialization of innovative technologies.
This collaboration on innovation across a wide range of disciplines is generating new jobs for our people and helping to address many of the globe’s big challenges.
Our space cooperation has become a signature aspect of this science, technology, and innovation cooperation, highlighting both the constancy of our mutual respect and appreciation for each others’ capabilities through the decades, as well as the vast potential – dare I say universal? -- opened up by the changes in our relationship.
I congratulate all of you – the experts and practitioners from both our countries – for your participation in building closer ties in space exploration, space science, earth observation, and launch and ensuring the safety and security of outer space activities. I know your efforts this week will further the cooperation that expands our collective knowledge, brings practical benefits to our citizens, and helps us plan for our future. I wish you all the best in this meeting of the Civil Space Joint Working Group.
Thursday, March 21, 2013
Tuesday, March 19, 2013
Monday, March 18, 2013
THE CHEMISTRY OF LIFE ON MARS
 |
| Credit: NASA, JPL, Caltech. |
NASA Rover Finds Conditions Once Suited for Ancient Life on Mars
WASHINGTON -- An analysis of a rock sample collected by NASA's Curiosity rover shows ancient Mars could have supported living microbes.
Scientists identified sulfur, nitrogen, hydrogen, oxygen, phosphorus and carbon -- some of the key chemical ingredients for life -- in the powder Curiosity drilled out of a sedimentary rock near an ancient stream bed in Gale Crater on the Red Planet last month.
"A fundamental question for this mission is whether Mars could have supported a habitable environment," said Michael Meyer, lead scientist for NASA's Mars Exploration Program at the agency's headquarters in Washington. "From what we know now, the answer is yes."
Clues to this habitable environment come from data returned by the rover's Sample Analysis at Mars (SAM) and Chemistry and Mineralogy (CheMin) instruments. The data indicate the Yellowknife Bay area the rover is exploring was the end of an ancient river system or an intermittently wet lake bed that could have provided chemical energy and other favorable conditions for microbes. The rock is made up of a fine grain mudstone containing clay minerals, sulfate minerals and other chemicals. This ancient wet environment, unlike some others on Mars, was not harshly oxidizing, acidic, or extremely salty.
The patch of bedrock where Curiosity drilled for its first sample lies in an ancient network of stream channels descending from the rim of Gale Crater. The bedrock also is fine-grained mudstone and shows evidence of multiple periods of wet conditions, including nodules and veins.
Curiosity's drill collected the sample at a site just a few hundred yards away from where the rover earlier found an ancient streambed in September 2012.
"Clay minerals make up at least 20 percent of the composition of this sample," said David Blake, principal investigator for the CheMin instrument at NASA's Ames Research Center in Moffett Field, Calif.
These clay minerals are a product of the reaction of relatively fresh water with igneous minerals, such as olivine, also present in the sediment. The reaction could have taken place within the sedimentary deposit, during transport of the sediment, or in the source region of the sediment. The presence of calcium sulfate along with the clay suggests the soil is neutral or mildly alkaline.
Scientists were surprised to find a mixture of oxidized, less-oxidized, and even non-oxidized chemicals providing an energy gradient of the sort many microbes on Earth exploit to live. This partial oxidation was first hinted at when the drill cuttings were revealed to be gray rather than red.
"The range of chemical ingredients we have identified in the sample is impressive, and it suggests pairings such as sulfates and sulfides that indicate a possible chemical energy source for micro-organisms," said Paul Mahaffy, principal investigator of the SAM suite of instruments at NASA's Goddard Space Flight Center in Greenbelt, Md.
An additional drilled sample will be used to help confirm these results for several of the trace gases analyzed by the SAM instrument.
"We have characterized a very ancient, but strangely new 'gray Mars' where conditions once were favorable for life," said John Grotzinger, Mars Science Laboratory project scientist at the California Institute of Technology in Pasadena, Calif. "Curiosity is on a mission of discovery and exploration, and as a team we feel there are many more exciting discoveries ahead of us in the months and years to come."
Scientists plan to work with Curiosity in the Yellowknife Bay area for many more weeks before beginning a long drive to Gale Crater's central mound, Mount Sharp. Investigating the stack of layers exposed on Mount Sharp, where clay minerals and sulfate minerals have been identified from orbit, may add information about the duration and diversity of habitable conditions.
NASA's Mars Science Laboratory Project has been using Curiosity to investigate whether an area within Mars' Gale Crater ever has offered an environment favorable for microbial life. Curiosity, carrying 10 science instruments, landed seven months ago to begin its two-year prime mission. NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the project for NASA's Science Mission Directorate in Washington.
Sunday, March 17, 2013
THE GULLYS OF MARS
Landforms on Mars
This image was taken by the High Resolution Imaging Science Experiment (HiRISE) flying onboard the Mars Reconnaissance Orbiter mission.
Gully landforms like those in this image are found in many craters in the mid-latitudes of Mars. Changes in gullies were first seen in images from the Mars Orbiter Camera in 2006, and studying such activity has been a high priority for HiRISE. Many examples of new deposits in gullies are now known.
This image shows a new deposit in Gasa Crater, in the Southern mid-latitudes. The deposit is distinctively blue in enhanced-color images. This image was acquired in southern spring, but the flow that formed the deposit occurred in the preceding winter.
Current gully activity appears to be concentrated in winter and early spring, and may be caused by the seasonal carbon dioxide frost that is visible in gully alcoves in the winter.
Written by: Colin Dundas
Image Credit-- NASA-JPL-University of Arizona
Friday, March 15, 2013
Monday, March 11, 2013
Sunday, March 10, 2013
LOOKING FOR ORGANICS ON MARS
 |
| Mars Rover On Earth. Credit: NASA. |
Organics are carbon-based molecules – key ingredients to life. If Curiosity finds organics in ancient rocks, thereʼs a better chance Mars once had good conditions for small life forms called microbes.
But, finding organics is hard! Thatʼs because organics easily break down when exposed to harsh things like extreme radiation and chemical oxidants that gave the Martian surface its rusty color.
A great place to look for ancient organics today is in rock layers. Organics that were quickly trapped and buried in layers of mud or in sediments that sank to the bottom of a body of water could have an especially good chance of being preserved.
Scientists think Curiosityʼs landing site, Gale Crater, contains those special layers, created in ancient times when water was present. The water dried up long ago, but rock layers that remain today could still preserve organics inside.
If Curiosity finds organics, it wouldnʼt prove life existed, but it sure would improve the odds that Mars once had the right ingredients for life!
Saturday, March 9, 2013
NASA RESEARCHES ALTERNATIVE JET FUEL
FROM: NASA
NASA Begins Flight Research Campaign Using Alternate Jet Fuel
WASHINGTON -- NASA researchers have begun a series of flights using the agency's DC-8 flying laboratory to study the effects of alternate biofuel on engine performance, emissions and aircraft-generated contrails at altitude.
The Alternative Fuel Effects on Contrails and Cruise Emissions (ACCESS) research involves flying the DC-8 as high as 40,000 feet while an instrumented NASA Falcon HU-25 aircraft trails behind at distances ranging from 300 feet to more than 10 miles.
"We believe this study will improve understanding of contrails formation and quantify potential benefits of renewable alternate fuels in terms of aviation's impact on the environment," said Ruben Del Rosario, manager of NASA's Fixed Wing Project.
ACCESS flight operations are being staged from NASA's Dryden Aircraft Operations Facility in Palmdale, Calif., and will take place mostly within restricted airspace over Edwards Air Force Base, Calif.
During the flights, the DC-8's four CFM56 engines will be powered by conventional JP-8 jet fuel, or a 50-50 blend of JP-8 and an alternative fuel of hydroprocessed esters and fatty acids that comes from camelina plants.
More than a dozen instruments mounted on the Falcon jet will characterize the soot and gases streaming from the DC-8, monitor the way exhaust plumes change in composition as they mix with air, and investigate the role emissions play in contrail formation.
Also, if weather conditions permit, the Falcon jet will trail commercial aircraft flying in the Southern California region, in coordination with air traffic controllers, to survey the exhaust emissions from a safe distance of 10 miles.
The flight campaign began Feb. 28 and is expected to take as long as three weeks to complete.
ACCESS follows a pair of Alternative Aviation Fuel Experiment studies conducted in 2009 and 2011 in which ground-based instruments measured the DC-8's exhaust emissions as the aircraft burned alternative fuels while parked on the ramp at the Palmdale facility.
A second phase of ACCESS flights is planned for 2014. It will capitalize on lessons learned from the 2013 flights and include a more extensive set of measurements.
The ACCESS study is a joint project involving researchers at Dryden, NASA's Glenn Research Center in Cleveland and NASA's Langley Research Center in Hampton, Va.
The Fixed Wing Project within the Fundamental Aeronautics Program of NASA's Aeronautics Research Mission Directorate manages ACCESS.
NASA Begins Flight Research Campaign Using Alternate Jet Fuel
WASHINGTON -- NASA researchers have begun a series of flights using the agency's DC-8 flying laboratory to study the effects of alternate biofuel on engine performance, emissions and aircraft-generated contrails at altitude.
The Alternative Fuel Effects on Contrails and Cruise Emissions (ACCESS) research involves flying the DC-8 as high as 40,000 feet while an instrumented NASA Falcon HU-25 aircraft trails behind at distances ranging from 300 feet to more than 10 miles.
"We believe this study will improve understanding of contrails formation and quantify potential benefits of renewable alternate fuels in terms of aviation's impact on the environment," said Ruben Del Rosario, manager of NASA's Fixed Wing Project.
ACCESS flight operations are being staged from NASA's Dryden Aircraft Operations Facility in Palmdale, Calif., and will take place mostly within restricted airspace over Edwards Air Force Base, Calif.
During the flights, the DC-8's four CFM56 engines will be powered by conventional JP-8 jet fuel, or a 50-50 blend of JP-8 and an alternative fuel of hydroprocessed esters and fatty acids that comes from camelina plants.
More than a dozen instruments mounted on the Falcon jet will characterize the soot and gases streaming from the DC-8, monitor the way exhaust plumes change in composition as they mix with air, and investigate the role emissions play in contrail formation.
Also, if weather conditions permit, the Falcon jet will trail commercial aircraft flying in the Southern California region, in coordination with air traffic controllers, to survey the exhaust emissions from a safe distance of 10 miles.
The flight campaign began Feb. 28 and is expected to take as long as three weeks to complete.
ACCESS follows a pair of Alternative Aviation Fuel Experiment studies conducted in 2009 and 2011 in which ground-based instruments measured the DC-8's exhaust emissions as the aircraft burned alternative fuels while parked on the ramp at the Palmdale facility.
A second phase of ACCESS flights is planned for 2014. It will capitalize on lessons learned from the 2013 flights and include a more extensive set of measurements.
The ACCESS study is a joint project involving researchers at Dryden, NASA's Glenn Research Center in Cleveland and NASA's Langley Research Center in Hampton, Va.
The Fixed Wing Project within the Fundamental Aeronautics Program of NASA's Aeronautics Research Mission Directorate manages ACCESS.
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