The PDF file you selected should load here if your Web browser has a PDF reader plug-in installed (for example, a recent version of Adobe Acrobat Reader).

If you would like more information about how to print, save, and work with PDFs, Highwire Press provides a helpful Frequently Asked Questions about PDFs.

Alternatively, you can download the PDF file directly to your computer, from where it can be opened using a PDF reader. To download the PDF, click the Download link above.

Fullscreen Fullscreen Off


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.
User
Notifications
Font Size