November 3, 2011
Southern Mare
<img src="" alt="LPOD-Nov3-11.jpg" title="LPOD-Nov3-11.jpg" />
image by Jocelyn Sérot, France
No, there wasn't a pyramid between Jocelyn and the Moon. His efforts to capture the well-librated limb
included taking a series of limb-centered images - the pyramid is simply an area not on the limb. This
view looks halfway across one of the Moon's oddest maria and impact basins. Mare Australe is an 880
km wide collection of mare-filled craters and low spots. This is a basin with no circular mountain rings
to define it, and yet it was recognized 40 years ago as soon as spacecraft images covered this region
right on the southeast limb. Early altimetry measurements suggested that Australe was a depression,
as much as 2 km lower in the center than around the edges. There is also a mascon, an excess mass
concentration, that is modelled as being due to a uprise of material from the mantle, as well as from the
lava on the surface. The interpretation is that the Australe Basin is very ancient, having formed when
the crust of the Moon was so warm that the mountain rims could not be supported, so they subsided.
In this respect, Australe is similar to the South Pole-Aitken Basin, which retains some of its rim, but
overall is much subdued. A final comment - the mare lava patches on the floor of Humboldt probably
are tied to the proximity to deep crustal fractures associated with the Australe Basin.
Chuck Wood
Technical Details
Oct 5, 2011, 19h45 UT. T200 Newton, Barlow 2x, R filter, DMK 31. Registax 6 processing.
Related Links
Rükl plate 76
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