Moon Mineralogy Mapper
Left side of the Moon Mineralogy Mapper
|Instrument Type||Imaging spectrometer|
|Mission duration||712 days (planned)
|Began operations||November 12, 2008|
|Ceased operations||September 20, 2009|
|Mass||8.2 kg (18 lb)|
|Resolution||40 km (25 mi) (field of view)
140 m (460 ft) (global)
70 m (230 ft) (targeted)
|Launch date||00:52, October 22, 2008|
|Launch Site||Satish Dhawan Space Centre|
The Moon Mineralogy Mapper (M3) is one of two instruments that NASA contributed to India's first mission to the Moon, Chandrayaan-1, launched October 22, 2008. The instrument is led by principal investigator Carle Pieters of Brown University, and managed by NASA's Jet Propulsion Laboratory.
M3 is an imaging spectrometer that has provided the first high-resolution spatial and spectral map of the entire lunar surface, revealing the minerals of which it is made. This information will both provide clues to the early development of the solar system and guide future astronauts to stores of precious resources.
This instrument is a Discovery Program "Mission of Opportunity" (a NASA-designed instrument on board another space agency's spacecraft).
Chandrayaan-1 operated for 312 days as opposed to the intended two years but the mission achieved 95 percent of its planned objectives, including mapping over 95% of the lunar surface with the M3 instrument.  After suffering from several technical issues including failure of the star sensors and poor thermal shielding, Chandrayaan-1 stopped sending radio signals at 1:30 AM IST on 29 August 2009 shortly after which, the ISRO officially declared the mission over.
- Carle M. Pieters, Brown University - PI (principal investigator)
- Joe Boardman, Analytical Imaging and Geophysics, LLC
- Bonnie Buratti, JPL
- Roger Clark, USGS
- Robert Green, JPL
- Jim Head, Brown University
- Sarah Lundeen, JPL - Instrument Ground Data System
- Erick Malaret, ACT
- Tom McCord, University of Hawaii
- Jack Mustard, Brown University
- Cass Runyon, College of Charleston
- Matt Staid, Planetary Science Institute
- Jessica Sunshine, University of Maryland
- Larry Taylor, University of Tennessee
- Stefanie Tompkins, SAIC
- Padma Varanasi, JPL - Mission Operations
Water discovered on moon
On September 24, 2009, the Science Magazine reported that NASA's Moon Mineralogy Mapper (M3) on Chandrayaan-1 had detected water on the moon. But, on 25 September 2009, ISRO announced that the MIP, another instrument on-board Chandrayaan-1 also had discovered water on the moon just before impact and had discovered it before M3. The announcement of this discovery was not made until NASA confirmed it.
M3 detected absorption features near 2.8-3.0 µm on the surface of the Moon. For silicate bodies, such features are typically attributed to OH- and/or H2O-bearing materials. On the Moon, the feature is seen as a widely distributed absorption that appears strongest at cooler high latitudes and at several fresh feldspathic craters. The general lack of correlation of this feature in sunlit M3 data with neutron spectrometer H abundance data suggests that the formation and retention of OH and H2O is an ongoing surficial process. OH/H2O production processes may feed polar cold traps and make the lunar regolith a candidate source of volatiles for human exploration.
The Moon Mineralogy Mapper (M3), an imaging spectrometer, was one of the 11 instruments on board Chandrayaan-I that came to a premature end on August 29. M3 was aimed at providing the first mineral map of the entire lunar surface.
Lunar scientists have for decades contended with the possibility of water repositories. They are now increasingly “confident that the decades-long debate is over,” a report says. “The moon, in fact, has water in all sorts of places; not just locked up in minerals, but scattered throughout the broken-up surface, and, potentially, in blocks or sheets of ice at depth.” The results from the NASA’s Lunar Reconnaissance Orbiter are also “offering a wide array of watery signals.” 
Mg-spinel-rich rock discovered
M3 found a rock dominated by Mg-spinel with no detectable pyroxene or olivine present (<5%) occurring along the western inner ring of Moscoviense Basin (as one of several discrete areas). The occurrence of this spinel does not easily fit with current lunar-crustal evolution models.
- Boardman, Joe. "A New Lunar Globe as Seen by the Moon Mineralogy Mapper: Image Coverage, Spectral Dimensionality and Statistical Anomalies." (PDF). LPI. Retrieved 12 April 2011.
- "Chandrayaan first discovered water on moon, but?". DNA. Bangalore. DNA. Sep 25, 2009. Retrieved 2013-06-09.
- Bagla, Pallav (September 25, 2009). "Did India beat NASA to find water on moon?". NDTV. Bangalore. Retrieved 2013-06-09.
- "Water discovered on moon?: "A lot of it actually"". The Hindu. Chennai, India. 23 September 2009.
- Pieters, Carle. "Identification of a new spinel-rich lunar rock type by the Moon Mineralogy Mapper (M3)" (PDF). LPI. Retrieved 12 April 2011.