Difference between revisions of "April 26, 2009"
| (4 intermediate revisions by the same user not shown) | |||
| Line 1: | Line 1: | ||
__NOTOC__ | __NOTOC__ | ||
=Leaks= | =Leaks= | ||
| + | <!-- Start of content --> | ||
<!-- ws:start:WikiTextHeadingRule:2:<h1> --> | <!-- ws:start:WikiTextHeadingRule:2:<h1> --> | ||
<!-- ws:start:WikiTextLocalImageRule:8:<img src="/file/view/LPOD-Apr26-09.jpg/69671711/LPOD-Apr26-09.jpg" alt="" title="" /> -->[[File:LPOD-Apr26-09.jpg|LPOD-Apr26-09.jpg]]<!-- ws:end:WikiTextLocalImageRule:8 --><br /> | <!-- ws:start:WikiTextLocalImageRule:8:<img src="/file/view/LPOD-Apr26-09.jpg/69671711/LPOD-Apr26-09.jpg" alt="" title="" /> -->[[File:LPOD-Apr26-09.jpg|LPOD-Apr26-09.jpg]]<!-- ws:end:WikiTextLocalImageRule:8 --><br /> | ||
| − | <em>images constructed from USGeological Survey [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_bw&west=266.67&south=6.48&east=277.93&north=12.10&center=272.295&defaultcenter=on&grid=none&stretch=none&projection=SIMP&r=1&g=1&b=1&advoption=NO&info=NO&resolution=64&scale=0.2369&imageTopX=-85402.8803855181&imageTopY=324436.1849874258 | + | <em>images constructed from USGeological Survey [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_bw&west=266.67&south=6.48&east=277.93&north=12.10&center=272.295&defaultcenter=on&grid=none&stretch=none&projection=SIMP&r=1&g=1&b=1&advoption=NO&info=NO&resolution=64&scale=0.2369&imageTopX=-85402.8803855181&imageTopY=324436.1849874258 Map-A-Planet] - Clementine above and Lunar Orbiter IV below.</em><br /> |
<br /> | <br /> | ||
| − | The farside is nearly all old highlands material with the majority of its mare lavas in the center of the South Pole-Aitken Basin. There are two other significant expanses of mare lava within Tsiolkovsky and Mare Moscoviense. Smaller, isolated patches also occur, like little plumbing leaks. And unlike the massive deposits in SPA, Tsiolkovsky and Moscoviense the little leaks typically aren't in large impact structures whose deep fractures provide conduits to the surface. This image shows two odd leaks at about 9° N, just near the western limb as seen from Earth. The larger crater with a dark halo appears to be a normal impact crater that has excavated buried mare lavas - a larger version of Copernicus H. The middle of the images is cut by a secondary crater chain from the Orientale Basin to the south. To the right of the chain is a peculiar feature that has a faint dark nimbus but is not a dark halo imact crater. The enlarged Clementine inset shows that the dark material is on the floor of the crater, and the Lunar Orbit mosaic reveals that the crater is on a rille complex that cuts Orientale ejecta. I don't know of any other pyroclastic deposit that occupies the floor of a small crater. Further east, at Vasco da Gama [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_bw&west=274.14&south=8.61&east=279.76&north=11.43&center=276.945&defaultcenter=on&grid=none&stretch=none&projection=SIMP&r=1&g=1&b=1&advoption=NO&info=NO&resolution=128&scale=0.1185&imageTopX=-42582.9895958304&imageTopY=325087.6632705331 | + | The farside is nearly all old highlands material with the majority of its mare lavas in the center of the South Pole-Aitken Basin. There are two other significant expanses of mare lava within Tsiolkovsky and Mare Moscoviense. Smaller, isolated patches also occur, like little plumbing leaks. And unlike the massive deposits in SPA, Tsiolkovsky and Moscoviense the little leaks typically aren't in large impact structures whose deep fractures provide conduits to the surface. This image shows two odd leaks at about 9° N, just near the western limb as seen from Earth. The larger crater with a dark halo appears to be a normal impact crater that has excavated buried mare lavas - a larger version of Copernicus H. The middle of the images is cut by a secondary crater chain from the Orientale Basin to the south. To the right of the chain is a peculiar feature that has a faint dark nimbus but is not a dark halo imact crater. The enlarged Clementine inset shows that the dark material is on the floor of the crater, and the Lunar Orbit mosaic reveals that the crater is on a rille complex that cuts Orientale ejecta. I don't know of any other pyroclastic deposit that occupies the floor of a small crater. Further east, at Vasco da Gama [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&layers=moon_clementine_bw&west=274.14&south=8.61&east=279.76&north=11.43&center=276.945&defaultcenter=on&grid=none&stretch=none&projection=SIMP&r=1&g=1&b=1&advoption=NO&info=NO&resolution=128&scale=0.1185&imageTopX=-42582.9895958304&imageTopY=325087.6632705331 R] are other pyroclastics, but R is a floor-fractured crater. The dark halo crater implies that mare basalts underly the Orientale ejecta in this region, but other nearby fresh impacts have not excavated it. The pyroclastics in the dark floor crater and R show that magma - not just older solidified lava - was available too.<br /> |
<br /> | <br /> | ||
| − | <em>[mailto:tychocrater@yahoo.com | + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> |
<br /> | <br /> | ||
<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
| − | Danny Caes independently [ | + | Danny Caes independently [https://the-moon.us/wiki/Sundman noted] the dark halo crater.<br /> |
<br /> | <br /> | ||
| + | <p><b>Yesterday's LPOD:</b> [[April 25, 2009|Twin Crescents, Critical Observation]] </p> | ||
| + | <p><b>Tomorrow's LPOD:</b> [[April 27, 2009|Yesterday's News (Cosmic Edition)]] </p> | ||
<hr /> | <hr /> | ||
| + | {{wiki/ArticleFooter}} | ||
Latest revision as of 18:02, 18 August 2018
Leaks
images constructed from USGeological Survey Map-A-Planet - Clementine above and Lunar Orbiter IV below.
The farside is nearly all old highlands material with the majority of its mare lavas in the center of the South Pole-Aitken Basin. There are two other significant expanses of mare lava within Tsiolkovsky and Mare Moscoviense. Smaller, isolated patches also occur, like little plumbing leaks. And unlike the massive deposits in SPA, Tsiolkovsky and Moscoviense the little leaks typically aren't in large impact structures whose deep fractures provide conduits to the surface. This image shows two odd leaks at about 9° N, just near the western limb as seen from Earth. The larger crater with a dark halo appears to be a normal impact crater that has excavated buried mare lavas - a larger version of Copernicus H. The middle of the images is cut by a secondary crater chain from the Orientale Basin to the south. To the right of the chain is a peculiar feature that has a faint dark nimbus but is not a dark halo imact crater. The enlarged Clementine inset shows that the dark material is on the floor of the crater, and the Lunar Orbit mosaic reveals that the crater is on a rille complex that cuts Orientale ejecta. I don't know of any other pyroclastic deposit that occupies the floor of a small crater. Further east, at Vasco da Gama R are other pyroclastics, but R is a floor-fractured crater. The dark halo crater implies that mare basalts underly the Orientale ejecta in this region, but other nearby fresh impacts have not excavated it. The pyroclastics in the dark floor crater and R show that magma - not just older solidified lava - was available too.
Chuck Wood
Related Links
Danny Caes independently noted the dark halo crater.
Yesterday's LPOD: Twin Crescents, Critical Observation
Tomorrow's LPOD: Yesterday's News (Cosmic Edition)
COMMENTS?
Register, Log in, and join in the comments.
