Difference between revisions of "November 3, 2011"
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<em>image by [mailto:jocelyn.serot@free.fr Jocelyn Sérot], France</em><br /> | <em>image by [mailto:jocelyn.serot@free.fr Jocelyn Sérot], France</em><br /> | ||
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| − | No, there wasn't a pyramid between Jocelyn and the Moon. His [http://lpod. | + | No, there wasn't a pyramid between Jocelyn and the Moon. His [http://www2.lpod.org/wiki/October_30,_2011 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 | + | 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 | + | 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 | + | 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 | + | 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, | + | 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 | + | 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 | + | 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 | + | 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. | + | 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 | + | 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 | + | 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.<br /> | + | are tied to the proximity to deep crustal fractures associated with the Australe Basin. |
| + | <br /> | ||
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
| − | Rükl plate [ | + | Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_76 76]<br /> |
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| + | <hr /> | ||
<p><b>Yesterday's LPOD:</b> [[November 2, 2011|Mooned River]] </p> | <p><b>Yesterday's LPOD:</b> [[November 2, 2011|Mooned River]] </p> | ||
<p><b>Tomorrow's LPOD:</b> [[November 4, 2011|Way Around the Limb]] </p> | <p><b>Tomorrow's LPOD:</b> [[November 4, 2011|Way Around the Limb]] </p> | ||
| − | < | + | <!-- End of content --> |
{{wiki/ArticleFooter}} | {{wiki/ArticleFooter}} | ||
Latest revision as of 08:34, 28 October 2018
Southern Mare
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
Yesterday's LPOD: Mooned River
Tomorrow's LPOD: Way Around the Limb
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