Bhabha sinks into the shadows

Last rays striking central peak of Bhabha crater just before sunset. View from the west looking east; image M133982125 [NASA/GSFC/Arizina State University].

The central farside crater Bhabha (64 km diameter) was named in honor of the physicist Homi Jehangir Bhabha (1909-1966), a nuclear physics pioneer in his home country of India. Bhabha Crater lies deep within the interior of the enormous South Pole-Aitken (SPA) Basin.

Full resolution view of summit of Bhabha central peaks [NASA/GSFC/Arizona State University].

 

 

 

Bhabha has a trio of central peaks that rise over a kilometer above the crater floor, and it has an intricate and complex system of rim terraces. Bhabha itself is a deep crater whose floor lies some 3 to 3.5 km below the crater rim. Bhabha is of special interest because the impact that formed it penetrated deep into the SPA Basin floor, excavated materials of the SPA Basin impact-melt complex, and distributed these materials onto the surrounding plains. Even though this event happened long ago in the Moon's history, those materials are still present in the surrounding plains deposits waiting for a lunar explorer - whether robotic or human - to come along and return them to Earth. These materials could then be used to address several important scientific questions, including age-dating the SPA Basin formation event, determining the nature of the materials that melted when SPA formed, and figuring out how deep the impact penetrated - perhaps through the lower crust and into the upper mantle of the Moon! Bhabha is truly a window deep into the interior of the Moon and deep into the ancient history of the Solar System.

Full view across Bhabha crater [NASA/GSFC/Arizona State University].

 

 

Look at those boulders on the summit. They may contain some of the deepest materials readily available from the Moon's crust. Imagine collecting samples of these precious materials yourself and returning them to Earth!

Explore the full-resolution NAC view of Bhabha!

Published by Mark Robinson on 21 July 2010