Blair Kuykendall
The Daily Beacon | A team of scientists, including Lawrence A. Taylor, professor in the Department of Earth and Planetary Sciences, has discovered the existence of water on the lunar surface.
Previously, the idea of water on the moon has been viewed with great skepticism, resulting from the assumption that the moon rock samples brought back from the Apollo mission were contaminated.
Trace amounts of water were found in the sample boxes, but scientists believed that the samples were contaminated by the presence of air from Earth.
Forty years have passed, and new satellite technology has aided scientists in discovering the composition of lunar soil. The soil contained chemical bonds between hydrogen and oxygen -- the molecular make-up of water.
This information was found through the analysis of data collected by a NASA craft known as the Moon Mineralogy Mapper, or M3. Carried by an Indian satellite, this tool processes the information conveyed by light rays the sun reflects off the moon.
Since light is reflected by varying wavelengths after contact with different minerals, scientists are able to use this method to determine which minerals are present in a thin layer of soil.
The M3 searched for traces of bonds between hydrogen and oxygen in the top few centimeters of lunar soil. Scientists were shocked to discover the presence of water within this soil, Taylor said.
“There is a special spectra given off by compounds and molecules containing OH (hydroxyl) and HOH (water),” he said. “These signals are very pronounced and caused our M3 team to argue and discuss this finding for five months, until we were all agreeable to the presence of the water and its probable cause.”
Researchers have decided that this probable cause is solar wind.
When the sun generates nuclear fusion, it creates protons that are positively charged hydrogen atoms. Lacking the protection of an atmosphere similar to the Earth, the moon’s surface is constantly being attacked by this fast-moving hydrogen.
Since the moon’s soil is largely composed of oxygen, the impact of these hydrogen particles is thought to be strong enough to break apart oxygen bonds present in the soil. Thus, water is formed on the moon.
“What we have discovered is a type of water that has a most unusual origin, being the result of solar-wind bombardment of the highly reactive lunar soil,” Taylor said.
The results of these findings by scientists from the U.S. and India were reported in the online journal Scientific Express. The findings could prove extremely valuable in the future as NASA plans to return to the moon. Maps created with this research data could help astronauts locate useful water within the lunar soil.
“The ability of utilizing in-situ resources greatly facilitates our space exploration,” Yang Liu, a research associate working with Taylor on planetary sciences and lunar exploration, said. “The finding of ‘water’ on the lunar surface opens doors for more economical space exploration.”
Further implications for this research could be even more extensive in the future.
“The NASA crash lander, LCROSS, on October 9 will bring more supporting evidence for our find,” Taylor said. “We would hope that all this will lead to humans returning to the moon to establish a launching point, away from Earth’s gravity, from which to refuel and go onward to Mars and beyond into the solar system.”
This discovery was made possible by a partnership between NASA and UT to fund Taylor’s work.
“This has supplied funding for beaucoup students, postdocs, instrumentation, etc. that the university would not otherwise have been able to afford,” Taylor said. “This is but one example of what we do as professors to help the university, as they provide the best education for the money for all the students.”
Related: NASA Prepares To Bomb The Moon
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Telltale signs
T.S. Subramanian
Frontline | SCIENTISTS of the Space Physics Laboratory (SPL), Vikram Sarabhai Space Centre (VSSC), Thiruvananthapuram, the lead institute for one of the experiments on the Moon Impact Probe (MIP) of Chandrayaan-1, obtained “very clear signature of H2O (18 atomic mass unit, or amu) intensifying” in the thin atmosphere of the moon as the MIP, carrying a very sensitive mass spectrometer called ChACE (Chandra’s Altitudinal Composition Explorer), “raced towards the lunar surface” for more than 20 minutes on November 14, 2008, according to Professor Dr R. Sridharan, Director of the SPL. “Our conclusion is that there is water present in the thin atmosphere of the moon,” he asserted. Consistent signature was revealed by ChACE, which was developed as a payload by the SPL. “We got the spectrum covering a mass range of 1 to 100 amu all through…. For us, the finding of water vapour in the moon’s thin atmosphere is very important,” he added.
The MIP was one of the 11 scientific instruments on board Chandrayaan-1, India’s first scientific mission to the moon. The MIP sat like “a hat” on top of the spacecraft. A Polar Satellite Launch Vehicle (PSLV) of the Indian Space Research Organisation (ISRO) lifted off from the spaceport at Sriharikota on October 22, 2008, and put Chandrayaan-1 in its initial orbit. A series of tricky manoeuvres saw the spacecraft reaching the lunar orbit at an altitude of 100 km on November 14.
After Chandrayaan-1 reached its lunar orbit, the MIP, with the Indian flag painted on its sides, hived itself away from the orbiter, raced towards the moon and crashed near the Shackleton Crater. Its journey towards the moon lasted more than 20 minutes. It had three instruments on board: ChACE, to “sniff” the moon’s very thin atmosphere as it descended towards the moon’s surface; a video camera (VIS) to take pictures of the lunar surface during its descent; and a radar altimeter to measure instantaneously the MIP’s altitude from the moon as the payload flew towards the lunar surface.
Sridharan dispelled misconceptions that the mass spectrometer detected water on the surface of the moon. It found water vapour in the moon’s thin atmosphere, he said. The purpose of the mass spectrometer was to analyse the gaseous constituents of the moon’s tenuous atmosphere. It was capable of analysing “how much [of gas] was present and what it is composed of,” he said. It did this in latitude and altitude after the MIP split away from Chandrayaan-1 and raced towards the moon’s surface. “The mass spectrometer was sensitive enough to analyse the presence of H2O in the form of gas – in the form of water vapour. It provided this data on November 14, [2008],” the SPL Director said.
Scientists of the SPL went ahead and analysed the constituents of the lunar atmosphere from the data given by the mass spectrometer. Sridharan said, “This was the first time that any composition measurement was done on the ‘sunlit’ side of the moon as the earlier attempts by the Apollo missions did not succeed owing to saturation effects. Any sensitive instrument such as the mass spectrometer is vulnerable to contamination, especially water vapour. So it becomes extremely important to glean out the signatures that belong exclusively to the lunar ambience.” The SPL scientists, therefore, went about differentiating the water vapour present in the latitude and altitude in the lunar atmosphere from possible instrument degassing.
Sridharan further explained: “That is why we took time to announce that there was water vapour present in the thin atmosphere of the moon. But there was one clue and we had to use it judiciously. If the water vapour was of instrument origin, it would have continued all through. But it cannot show the variations in latitude and altitude as the source itself is within. However, we had seen very clear signatures of H2O intensifying as the MIP raced towards the lunar surface…. The Moon Mineralogy Mapper [M3] of NASA, on board Chandrayaan-1, has also inferred [water molecules on the moon’s top surface]. There is a consistency [in the findings of the mass spectrometer and the Moon Mineralogy Mapper]. Our conclusion is that there is water vapour present in the thin lunar atmosphere…. We got the signatures all through.”
Any substance exists in three phases: solid, liquid and vapour. If a substance has one of these phases, the other phases will coexist depending on the ambient conditions. Further, owing to the large thermal cycling of the lunar surface, the lunar atmosphere went through cycles as it “breathed” in and out, Sridharan said. But the moon’s atmosphere is so thin that the breathing effect turns out to be phenomenal. While it breathed out, all gases get released owing to desorption, said the SPL Director.
Asked how significant the success of the MIP’s mass spectrometer and the finding of water on the moon by M3 were, Sridharan said: “As a person who was involved in this mission, it was a phenomenal success. For us, the whole experiment was a phenomenal success.”
The SPL team was on the job of analysing the data from the mass spectrometer. The team had to publish its findings and the world should accept it, he said. “The MIP mission was over long ago. While the world might have forgotten about it, we cannot. We are on the job of analysing the data. Maybe we will be working on the data for several years to come. For us, detecting water vapour in the moon’s thin atmosphere is very, very important.”
Y. Ashok Kumar, Project Director of the MIP, is also thrilled about the success of the MIP. The video camera on board the probe took about 3,000 pictures of the lunar surface right from the time it separated from the orbiter and crashed on the Shackleton Crater, he said. The video camera clicked away all through its descent. In fact, the MIP was switched on soon after the spacecraft entered the lunar orbit and the camera took pictures when the spacecraft was in this orbit itself, he said.
On whether it was true that it was A.P.J. Abdul Kalam, rocket engineer and former President, who suggested that ISRO keep MIP on board Chandrayaan-1, Ashok Kumar replied that “in a way, it was the brainchild of Mr. Kalam.” The former President suggested that since ISRO was sending a spacecraft all the way to the moon, “why not we have something that can crash on the moon”. An instrument, with India’s flag painted on its side, could “drop” on the moon and it would convey the message that “India has arrived on the moon”, Kalam had said.
The MIP landing on the moon was “both symbolic and significant”, Ashok Kumar said. It was significant because both the M3 and ChACE had revealed the presence of water on the moon. India, in its very first attempt, could put a spacecraft in the lunar orbit; it could land a payload on the moon’s surface; and the mass spectrometer was able to detect water vapour in the moon’s atmosphere. “All these are unique successes of the Chandrayaan-1 mission,” Ashok Kumar said. The 3,000 pictures of the lunar surface taken by the MIP’s video camera would help ISRO determine where the lander-cum-rover of Chandrayaan-2 mission should soft-land on the moon, he added.
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