The Chandra’s Atmospheric Composition Explorer-2 (CHACE-2) payload aboard the Chandrayaan-2 orbiter has detected Argon-40 from an altitude of approximately 100 km said ISRO on Thursday. Planetary scientists prefer to call the thin gaseous envelope around the Moon as the ‘Lunar exosphere’ since it is so tenuous that the gas atoms very rarely collide with each other. ISRO also released a schematic of how Argon-40 is formed.
#ISRO— ISRO (@isro) October 31, 2019
The CHACE-2 payload aboard the #Chandrayaan2 orbiter has detected Argon-40 from an altitude of approximately 100 km.
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Here's the schematic of the origin and dynamics of Argon-40 in lunar exosphere pic.twitter.com/xrFDblq2Mt
Argon-40 (40Ar), which is one of the isotopes of the noble gas Argon, is an important constituent of the lunar exosphere. It originates from the radioactive disintegration of Potassium-40 (40K), which has a half-life of ~1.2 X 109 years. The radioactive 40K nuclide, which is present deep below the lunar surface, disintegrates to 40Ar, which, in turn, diffuses through the intergranular space and makes way up to the lunar exosphere through seepages and faults.
The Chandra’s Atmospheric Composition Explorer-2 (CHACE-2) payload aboard the Chandrayaan-2 orbiter, is a neutral mass spectrometer-based payload which can detect constituents in the lunar neutral exosphere in the range of 1-300 amu (atomic mass unit). As part of its early operation, it has detected 40Ar in the lunar exosphere from an altitude of ~100 km, capturing the day-night variations of concentration. 40Ar being a condensable gas at the temperatures and pressures that prevail on the lunar surface, condenses during lunar night. After lunar dawn, the 40Ar starts getting released to the lunar exosphere.
On October 22, ISRO released the pictures of the impact craters on the south polar region of the moon clicked by the orbiter of Chandrayaan 2. These pictures show the observations made by the Synthetic Aperture Radar on the lunar surface. Moon’s surface has a lot of impact craters owing to the continuous bombardment of celestial bodies, these craters are usually studied by a powerful remote sensing instrument to know more about the moon’s surface.
#ISRO#Chandrayaan2’s DF-SAR is designed to produce greater details about the morphology and ejecta materials of impact craters on the lunar surface. Have a look of initial images and observations made by DF-SAR— ISRO (@isro) October 22, 2019
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