NASA's LCROSS Impacts Confirm Water in Lunar Crater

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Nov. 13, 2009

Grey Hautaluoma/Ashley Edwards 
Headquarters, Washington 
202-358-0668/1756 
grey.hautaluoma-1@xxxxxxxx, ashley.edwards-1@xxxxxxxx 

Jonas Dino 
Ames Research Center, Moffett Field, Calif. 
650-604-5612 
jonas.dino@xxxxxxxx 

RELEASE: 09-265

NASA'S LCROSS IMPACTS CONFIRM WATER IN LUNAR CRATER

MOFFETT FIELD, Calif. -- 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. 

For information about LCROSS, visit: 



http://www.nasa.gov/lcross 

	
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