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Evidences of Relatively New Volcanic Flows on the Moon


Affiliations
1 Department of Earth Sciences, Indian Institute of Technology-Roorkee, Roorkee 247 667, India
2 Planetary Sciences and Exploration Programme, Physical Research Laboratory, Ahmedabad 380 009, India
 

It is generally believed that the Moon became inter-nally dead ∼1 b.y. from the present, and only old ( 1 b.y.) volcanic flows forming largely the mare basins are known to occur. The old volcanic land-forms stand largely obliterated and flows studded with impact craters. However, recent findings have indicated global presence of young thrust faults on the Moon, escape of gases from the interior and also pre-dicted the presence of partially molten lower lunar mantle and core. Here, we have used high-resolution datasets from NASA's LRO, Kaguya of JAXA and ISRO's Chandrayan-1 missions to examine the char-acteristics and origin of multiple relatively fresh, coaxial, superposed viscous flows spotted inside the Lowell crater on the far side of the Moon. Various considerations apparently rule out the possibility of these melts being derived from nearby areas. An asso-ciated likely source crater and tectonic structures (a fault and a fracture) of two different ages but emanat-ing from the same crater and affecting different flows have also been located - exhibiting tectono-volcanic relationship. These features provide evidences of like-ly volcanic activity in the region not too far in the past, are consistent with recent results that the Moon may not be internally dead, and thus have implica-tions to the thermal history and present-day geologic nature of the Moon.

Keywords

Craters, Moon, Tectonic Features, Volcanic Flows.
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  • Evidences of Relatively New Volcanic Flows on the Moon

Abstract Views: 335  |  PDF Views: 140

Authors

R. P. Gupta
Department of Earth Sciences, Indian Institute of Technology-Roorkee, Roorkee 247 667, India
N. Srivastava
Planetary Sciences and Exploration Programme, Physical Research Laboratory, Ahmedabad 380 009, India
R. K. Tiwari
Department of Earth Sciences, Indian Institute of Technology-Roorkee, Roorkee 247 667, India

Abstract


It is generally believed that the Moon became inter-nally dead ∼1 b.y. from the present, and only old ( 1 b.y.) volcanic flows forming largely the mare basins are known to occur. The old volcanic land-forms stand largely obliterated and flows studded with impact craters. However, recent findings have indicated global presence of young thrust faults on the Moon, escape of gases from the interior and also pre-dicted the presence of partially molten lower lunar mantle and core. Here, we have used high-resolution datasets from NASA's LRO, Kaguya of JAXA and ISRO's Chandrayan-1 missions to examine the char-acteristics and origin of multiple relatively fresh, coaxial, superposed viscous flows spotted inside the Lowell crater on the far side of the Moon. Various considerations apparently rule out the possibility of these melts being derived from nearby areas. An asso-ciated likely source crater and tectonic structures (a fault and a fracture) of two different ages but emanat-ing from the same crater and affecting different flows have also been located - exhibiting tectono-volcanic relationship. These features provide evidences of like-ly volcanic activity in the region not too far in the past, are consistent with recent results that the Moon may not be internally dead, and thus have implica-tions to the thermal history and present-day geologic nature of the Moon.

Keywords


Craters, Moon, Tectonic Features, Volcanic Flows.



DOI: https://doi.org/10.18520/cs%2Fv107%2Fi3%2F454-460