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LCROSS Lunar Impact Data Shows ‘Significant Amount’ of Water on Moon

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Preliminary data from NASA’s Lunar Crater Observation and Sensing Satellite, or LCROSS, indicates the mission successfully uncovered water in a permanently shadowed lunar crater. The discovery opens a new chapter in our understanding of the moon.

The LCROSS spacecraft and a companion rocket stage made twin impacts in the Cabeus crater Oct. 9 that created a plume of material from the bottom of a crater that has not seen sunlight in billions of years. The plume traveled at a high angle beyond the rim of Cabeus and into sunlight, while an additional curtain of debris was ejected more laterally.

“We’re unlocking the mysteries of our nearest neighbor and, by extension, the solar system,” said Michael Wargo, chief lunar scientist at NASA Headquarters in Washington. “The moon harbors many secrets, and LCROSS has added a new layer to our understanding.”

Scientists long have speculated about the source of significant quantities of hydrogen that have been observed at the lunar poles. The LCROSS findings are shedding new light on the question with the discovery of water, which could be more widespread and in greater quantity than previously suspected. If the water that was formed or deposited is billions of years old, these polar cold traps could hold a key to the history and evolution of the solar system, much as an ice core sample taken on Earth reveals ancient data. In addition, water and other compounds represent potential resources that could sustain future lunar exploration.

Since the impacts, the LCROSS science team has been analyzing the huge amount of data the spacecraft collected. The team concentrated on data from the satellite’s spectrometers, which provide the most definitive information about the presence of water. A spectrometer helps identify the composition of materials by examining light they emit or absorb.

“We are ecstatic,” said Anthony Colaprete, LCROSS project scientist and principal investigator at NASA’s Ames Research Center in Moffett Field, Calif. “Multiple lines of evidence show water was present in both the high angle vapor plume and the ejecta curtain created by the LCROSS Centaur impact. The concentration and distribution of water and other substances requires further analysis, but it is safe to say Cabeus holds water.”

The team took the known near-infrared spectral signatures of water and other materials and compared them to the impact spectra the LCROSS near infrared spectrometer collected.

“We were able to match the spectra from LCROSS data only when we inserted the spectra for water,” Colaprete said. “No other reasonable combination of other compounds that we tried matched the observations. The possibility of contamination from the Centaur also was ruled out.”

Additional confirmation came from an emission in the ultraviolet spectrum that was attributed to hydroxyl, one product from the break-up of water by sunlight. When atoms and molecules are excited, they release energy at specific wavelengths that can be detected by the spectrometers. A similar process is used in neon signs. When electrified, a specific gas will produce a distinct color. Just after impact, the LCROSS ultraviolet visible spectrometer detected hydroxyl signatures that are consistent with a water vapor cloud in sunlight.

Data from the other LCROSS instruments are being analyzed for additional clues about the state and distribution of the material at the impact site. The LCROSS science team and colleagues are poring over the data to understand the entire impact event, from flash to crater. The goal is to understand the distribution of all materials within the soil at the impact site.

“The full understanding of the LCROSS data may take some time. The data is that rich,” Colaprete said. “Along with the water in Cabeus, there are hints of other intriguing substances. The permanently shadowed regions of the moon are truly cold traps, collecting and preserving material over billions of years.”

LCROSS was launched June 18 from NASA’s Kennedy Space Center in Florida as a companion mission to the Lunar Reconnaissance Orbiter, or LRO. Moving at a speed of more than 1.5 miles per second, the spent upper stage of its launch vehicle hit the lunar surface shortly after 4:31 a.m. PDT Oct. 9, creating an impact that instruments aboard LCROSS observed for approximately four minutes. LCROSS then impacted the surface at approximately 4:36 a.m.

LRO observed the impact and continues to pass over the site to give the LCROSS team additional insight into the mechanics of the impact and its resulting craters. The LCROSS science team is working closely with scientists from LRO and other observatories that viewed the impact to analyze and understand the full scope of the LCROSS data.


SPACE WALLPAPER: Apollo 11 Bootprint

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(Above) One of the first steps taken on the Moon, this is an image of Buzz Aldrin’s bootprint from the Apollo 11 mission. Neil Armstrong and Buzz Aldrin walked on the Moon on July 20, 1969.

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SPACE WALLPAPER: 1963 Lunar Lander Model

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(Above) This 1963 model depicts an early Apollo lunar lander concept, called a “bug.” Engineers designed several possible vehicle shapes for both manned and unmanned landers. In 1961, Bruce Lundin, former director of NASA’s Lewis Research Center (now Glenn), chaired a NASA study group that assessed a variety of ways to accomplish a lunar landing mission.

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NASA/DOE Developing Surface Nuclear Fission Power

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(Above) An artist’s concept of a fission surface power system on the surface of the moon. The nuclear reactor has been buried below the lunar surface to make use of lunar soil as additional radiation shielding. The power system would transmit a steady 40 kW of electric power, enough for about eight houses on Earth, to the lunar outpost.

NASA and the Department of Energy have completed tests on several fission surface power components within the last few weeks. The agencies are researching technologies that could enable possible use of nuclear power on the surface of the moon and Mars. Nuclear power is part of the range of options that are being examined for potential human missions on the moon and Mars.

A fission surface power system could use a small nuclear reactor, about the size of an office trash can, and Stirling power generators to produce 40 kilowatts of energy, enough electricity to power a future lunar or Mars outpost. The electricity produced could be used for life support, performing experiments, recharging rovers and mining resources.

Don Palac, NASA Glenn Research Center’s fission surface power system project manager, observed, “This recent string of technology development successes confirms that the fission surface power project is on the right path.”

One successful test occurred at Glenn in Cleveland, where a lightweight composite radiator panel was successfully tested in a vacuum chamber that replicates the hard vacuum and extreme cold temperatures that would be seen in space, with temperatures as low as minus 125 degrees C. The radiator, approximately 6 feet by 9 feet, represents one of 20 panels that would be needed to cool the notional fission surface power system. By performing this test, the team showed the radiator panel could reject the required heat at the proper temperature under realistic lunar conditions.

The radiator panel was designed and built by Material Innovations, Inc., Huntington Beach, Calif., with help from Thermacore, Inc., Lancaster, Pa. and Materials Research and Design, Inc., Wayne, Pa.

According to Glenn lead engineer David Ellis, “This was a tremendous accomplishment and a giant step toward proving out the radiator technology. We can now proceed toward a system-level technology demonstration with confidence.”

A second achievement occurred at NASA’s Marshall Space Flight Center, Huntsville, Ala. For the first time, Stirling engines were heated with a pumped liquid metal, replicating how heat could be delivered from a reactor to the converter. This was a major accomplishment on the road to demonstrating technical feasibility of fission surface power.

Glenn developed the data and control system for the Stirling engines, which were designed and built by Sunpower, Inc., Athens, Ohio. Glenn also designed the Stirling heat exchangers that were fabricated by Mound Advanced Technology Center in Miamisburg, Ohio. The test loop at Marshall included an electrically heated reactor simulator designed by Los Alamos National Laboratory, Los Alamos, NM and an electromagnetic pump supplied by Idaho National Laboratory, Idaho Falls, Idaho.

Steve Geng was the Glenn lead for the test. He said, “The engines performed flawlessly producing over 2 kilowatts of electricity at a gross thermal efficiency of about 32 per cent with liquid metal temperatures as high as 550 degrees C.”

At Sandia National Laboratories in Albuquerque, NM, a Stirling alternator was operated while being exposed to radiation levels similar to those that would be experienced with a reactor. The alternator survived a cumulative radiation dose 20 times the current fission surface power surface design requirement, during 26 hours of radiation exposure in the DOE Gamma Irradiation Facility at Sandia. There was no change in electrical power input required to maintain alternator operation, which would have been a possible indication of radiation damage.

The Stirling alternator was developed by Sunpower, Inc., Athens, Ohio. The diagnostics and control rack was assembled by Glenn. Testing was conducted by a team that included Sandia, Glenn and a University of Florida doctoral student.

“The pace of progress exhibited by these three achievements in the same time period is exciting,” said Lee Mason, Glenn’s principal investigator for the fission surface power project. “It has built the team’s confidence and prepared them for challenges that lay ahead.”

The next major step is a non-nuclear system level technology demonstration where all of the major elements will be combined in one test. This test is scheduled to begin in 2012.

The Fission Surface Power Project is managed by Glenn for NASA’s Exploration Technology Development Program Office at NASA’s Langley Research Center, Hampton, Va.


NASA Oxygen Production Technology Tested in Hawaii

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(Above) ROxygen could produce two thirds of the oxygen needed to sustain a crew of four on the moon.

In November of 2008, NASA concluded nearly two weeks of tests on equipment and lunar rover concepts in Hawaii. The islands’ volcanic terrain, rock distribution and soil materials provide a high-quality simulation of the moon’s polar region. One of many field demonstrations developed by NASA’s Exploration Technology Development Program, these tests provides valuable information and help engineers and scientists spot complications that might not be obvious in laboratories.

The agency’s In Situ Resource Utilization Project, which studies ways astronauts can use resources found at landing sites, demonstrated how people might prospect for resources on the moon and make their own oxygen from lunar rocks and soil. NASA’s lunar exploration plan currently projects that on-site lunar resources could generate one to two metric tons of oxygen annually. This is roughly the amount of oxygen that four to six people living at a lunar outpost might breathe in a year.

ROxygen and PILOT, or Precursor ISRU Lunar Oxygen Testbed were two technologies that were tested. The two large, complementary systems might produce oxygen from soil on an outpost-sized scale.

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(Above) The PILOT system is shown with Lockheed Martin’s Bucketwheel on a lander the size of the Phoenix spacecraft currently on Mars. PILOT could produce up to one quarter of the oxygen needed to sustain a crew of four on the moon.

A prototype system combines a polar prospecting rover and a drill specifically designed to penetrate the harsh lunar soil. The rover’s system demonstrates small-scale oxygen production from regolith. A similar rover could search for water ice and volatile gases such as hydrogen, helium, and nitrogen, in the permanently shadowed craters of the moon’s poles. Carnegie Mellon University of Pittsburgh built the rover, which carries equipment known as the Regolith and Environment Science and Oxygen and Lunar Volatile Extraction (RESOLVE).

Other tested concepts include a NASA-developed robotic excavator known as Cratos; a new lunar wheel developed by Michelin North America of Greenville, S.C.; a lunar sample coring drill the Northern Centre for Advanced Technology in Canada developed for NASA with support from the Canadian Space Agency, or CSA; an excavator developed by Lockheed Martin of Denver; and a night vision camera called TriDAR for the rover’s navigation and drill site selection. Neptec in Canada developed the camera with support from CSA. The tests were hosted by The Pacific International Space Center for Exploration Systems, or PISCES, headquartered at the University of Hawaii, Hilo.

Additional instruments that were field tested will be used to improve understanding of minerals found on the moon. They include a Mossbauer spectrometer from NASA’s Johnson Space Center in Houston and the University of Mainz in Germany; an X-ray diffraction unit called mini CheMIN from NASA’s Ames Research Center at Moffett Field, Calif., and the Los Alamos National Laboratory in New Mexico; and a handheld Raman spectrometer CSA provided.


NASA’s Moon Mapper Captures Earth

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This false-color image of Earth was taken from 124 miles above the lunar surface by the Moon Mineralogy Mapper, one of two NASA instruments onboard the Indian Space Research Organization’s Chandrayaan-1 spacecraft.

This image of Earth taken from 200 kilometers (124 miles) above the lunar surface was taken by the Moon Mineralogy Mapper, one of two NASA instruments onboard the Indian Space Research Organization’s Chandrayaan-1 spacecraft. Australia is visible in the lower center of the image. The image is presented as a false-color composite with oceans a dark blue, clouds white, and vegetation an enhanced green. The image data were acquired on July 22, 2009.

The Moon Mineralogy Mapper instrument is a state-of-the-art imaging spectrometer designed to provide the first map of the entire lunar surface at high spatial and spectral resolution. Scientists will use this information to answer questions about the moon’s origin and development and the evolution of terrestrial planets in the early solar system. Future astronauts will use it to locate resources, possibly including water, that can support exploration of the moon and beyond.


New Spring Tire for Lunar Rovers That Won’t Go Flat

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The National Aeronautics and Space Administration (NASA) and The Goodyear Tire & Rubber Company have developed an airless tire to transport large, long-range vehicles across the surface of the moon.

The new “Spring Tire” with 800 load bearing springs is designed to carry much heavier vehicles over much greater distances than the wire mesh tire previously used on the Apollo Lunar Roving Vehicle (LRV). The new tire will allow for broader exploration and the eventual development and maintenance of a lunar outpost.

According to Vivake Asnani, NASA’s principal investigator at the Glenn Research Center in Cleveland, this was a significant change in requirements that required innovation. “With the combined requirements of increased load and life, we needed to make a fundamental change to the original moon tire,” he said. “What the Goodyear-NASA team developed is an innovative, yet simple network of interwoven springs that does the job. The tire design seems almost obvious in retrospect, as most good inventions do.”

The Spring Tire was installed on NASA’s Lunar Electric Rover test vehicle and put through its paces at the Johnson Space Center’s “Rock Yard” in Houston where it performed successfully.

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“This tire is extremely durable and extremely energy efficient,” noted Jim Benzing, Goodyear’s lead innovator on the project. “The spring design contours to the surface on which it’s driven to provide traction. But all of the energy used to deform the tire is returned when the springs rebound. It doesn’t generate heat like a normal tire.

According to Goodyear engineers, development of the original Apollo lunar mission tires, and the new Spring Tire were driven by the fact that traditional rubber, pneumatic (air-filled) tires used on Earth have little utility on the moon. This is because rubber properties vary significantly between the extreme cold and hot temperatures experienced in the shaded and directly sunlit areas of the moon. Furthermore, unfiltered solar radiation degrades rubber, and pneumatic tires pose an unacceptable risk of deflation.

According to Asnani, the Spring Tire does not have a “single point failure mode. What that means,” he said, “is that a hard impact that might cause a pneumatic tire to puncture and deflate would only damage one of the 800 load bearing springs. Along with having this ultra-redundant characteristic, the tire has a combination of overall stiffness yet flexibility that allows off-road vehicles to travel fast over rough terrain with relatively little motion being transferred to the vehicle.”

NASA has been so impressed with the tire that it decided to highlight the project during NASA’s recent “Day on the Hill” exhibit at the Rayburn House Office Building in Washington, DC. “I spoke with 10 to 15 members of Congress and about sixty staffers,” noted NASA’s Asnani. “Virtually everyone I spoke with was blown away by the idea that this technology may one day be used, not only for extraterrestrial vehicles, but also, perhaps, for vehicles here on Earth.”


Iconic Images: First U.S. Image of the Moon

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Ranger 7 took this image, the first picture of the Moon by a U.S. spacecraft about 17 minutes before impacting the lunar surface. The large crater at center right is the 108 km diameter Alphonsus. Above it is Ptolemaeus and below it Arzachel. Mare Nubium is at center and left. The Ranger 7impact site is off the frame, to the left of the upper left corner.

Ranger spacecraft were designed solely to take high-quality pictures of the Moon for scientific study and to scout landing sites for Apollo astronauts. Ranger 7 was the first true success in the series and represents a turning point in the American space program. It transmitted 4,308 high-quality images in its final 17 minutes of flight.

Ranger 7 was launched July 28, 1964 and arrived at the Moon on July 31, 1964.


Apollo 11 Moon Rock on the International Space Station

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(Above) A moon rock brought to Earth by Apollo 11, humans’ first landing on the moon in July 1969, is shown as it floats aboard the International Space Station. Part of Earth can be seen through the window.

The 3.6 billion year-old lunar sample was flown to the station aboard Space Shuttle mission STS-119 in April 2009 in honor of the July 2009 40th anniversary of the historic first moon landing. The rock, lunar sample 10072, was flown to the station to serve as a symbol of the nation’s resolve to continue the exploration of space. It will be returned on shuttle mission STS-128 to be publicly displayed.


Chandrayaan-1 spacecraft completes 3000 Lunar Orbits

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(Above) This artist’s concept shows the Indian lunar mission Chandrayaan 1

Chandrayaan-1, India’s first mission to the Moon, launched on October 22, 2008 from Satish Dhawan Space Centre, Sriharikota, has completed eight months of successful operation and has made 3,000 revolutions around the Moon.

Besides sending more than 70,000 images of the lunar surface which provide breathtaking views of lunar mountains and craters, especially craters in the permanently shadowed areas of the Moon’s polar region, Chandrayaan-1 spacecraft is also collecting valuable data pertaining to the chemical and mineral content of the Moon.

Chandrayaan-1’s orbit was raised from 100 km to 200 km circular on May 19, 2009. The high orbital altitude of Chandrayaan-1 reduces the resolution of the imagery but provides a wider swath and the data is of good quality.

The onboard star sensor used for determining the orientation of the spacecraft started malfunctioning on April 26, 2009.

To overcome this anomaly, ISRO devised an innovative technique of using redundant sensors – gyroscopes – along with antenna pointing information and images of specific location on the surface of the moon, for determining the orientation of the spacecraft.

This method has been validated and based on this information, mission operations are being carried out satisfactorily. Other than the failure of the star sensor and one of the Bus Management Units, health of the spacecraft is normal.

Recent review by scientists has confirmed that all primary mission objectives of Chandrayaan-1 have been successfully realised during the eight months of its operation.

The spacecraft continues to send high quality data as per planned sequence to its ground station at Byalalu near Bangalore. Detailed review of the scientific objectives and the performance results on the Chandrayaan-1 mission is scheduled within three months after which further operational procedures will be worked out.

The primary mission objectives of Chandrayaan-1 are:

  • To realise the complex spacecraft with 11 scientific instruments
  • To launch the spacecraft in near earth orbit and to carry out orbit raising manoeuvres of the spacecraft from 22,000 km to 3,84,000 km and place the spacecraft in a circular orbit around the moon
  • To place the Indian Tricolour on the moon
  • To carry out the imaging operation of the lunar surface and collect data on the mineral content of the lunar surface
  • To realise the deep space tracking network and implement the operational procedures for travel into deep space

With the successful realisation of these objectives, additional data that will be derived during the remaining part of Chandrayaan-1’s life will be complementary to already derived information.

The data collected from Chandrayaan-1 instruments have been disseminated to the Indian scientists and also the partners from Europe and USA. The scientific community is extremely happy with the already obtained data and the results of analysis could be expected in about 6 months to 1 year period.


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