Discovery of Water
On the 25 September 2009, ISRO announced that the MIP had discovered water on the moon just before impact. This announcement was made after the discovery of water was announced on September 24, 2009 by Science magazine by the NASA payload Moon Mineralogy Mapper carried on board Chandrayaan-1. MIP discovered water on moon before NASA's Moon Mineralogy Mapper. The announcement of this discovery was not made until NASA confirmed it.
It gifted the answer to the millennia-old question whether water is there in Earth’s moon when it led to the discovery of water in its vapour phase by the CHACE (CHandra’s Altitudinal Composition Explorer) payload on board the Moon Impact Probe (MIP) and complementarily in its solid phase by the Moon Mineralogy Mapper (M3) payload on board the main orbiter in the Chandrayaan I mission. This ‘discovery-class-of-finding’ by CHACE was achieved by direct in situ measurement of the lunar atmosphere during the descend journey of the MIP to the Lunar South Pole, while M3 discovered water in ice form by remote sensing techniques. As water cannot retain its liquid phase in the lunar environment because of its own vapour pressure and the ultra-high vacuum prevailing there, it can be found in solid (ice) and gaseous (vapour) phases. While the Moon Mineralogy Mapper (M3), a payload by NASA, on board Chandrayaan I lunar orbiter has detected, by mapping almost 97% of the lunar surface using remote sensing techniques, the presence of water in ice form in higher latitudes especially in the polar caps, the CHACE payload in the lunar impactor (MIP) has directly detected water in its gaseous form along 14 degree E meridian from 45 degree N to 90 degree S latitude, with a latitudinal resolution of around 0.10 and altitudinal resolution of ~ 250 m from 98 km altitude till impact .
Read more about this topic: Moon Impact Probe
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