Difference between revisions of "May 1, 2009"
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=The Best Farside Map of the Moon= | =The Best Farside Map of the Moon= | ||
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| − | <em>digital topography image map simplified from [mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | + | <em>digital topography image map simplified from [http://wms.selene.jaxa.jp/selene_viewer/jpn/observation_mission/lalt/lalt_008.html JAXA/Kaguya Image Gallery]</em><br /> |
| + | <br /> | ||
| + | The [http://www2.lpod.org/wiki/April_9,_2009 April 9th] LPOD featured the best ever photomap of the nearside, and here is the companion for the farside. Like the previous map this was made by | ||
| + | transforming the Kaguya colored topographic map into a grayscale image. This map is vastly better than the three existing farside image maps - from | ||
| + | [https://the-moon.us/wiki/Farside Clementine, Chang'e-1] and [[April_10,_2004|Phil Stooke]] - because this map has uniform lighting everywhere. This shows the farside as it has never been seen before | ||
| + | by anyone. Craters are everywhere, with few maria to create patterns. The impact basins are the only landmarks, with the relative emptiness of the South | ||
| + | Pole-Aitken Basin dominating the southern hemisphere. The old, degraded basin in the center is [https://the-moon.us/wiki/Freundlich-Sharanov_Basin Freundlich-Sharanov], 600 km in diameter with a small | ||
| + | patch of mare in its center, and nearly undetectable on other imagery. Hooray, Kaguya! | ||
| + | <br /> | ||
| + | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | ||
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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
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| − | + | <p><b>Yesterday's LPOD:</b> [[April 30, 2009|A Little Bit About a Normal Crater]] </p> | |
| − | ---- | + | <p><b>Tomorrow's LPOD:</b> [[May 2, 2009|Smaller And Smaller Rilles]] </p> |
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Latest revision as of 08:32, 28 October 2018
The Best Farside Map of the Moon
digital topography image map simplified from JAXA/Kaguya Image Gallery
The April 9th LPOD featured the best ever photomap of the nearside, and here is the companion for the farside. Like the previous map this was made by
transforming the Kaguya colored topographic map into a grayscale image. This map is vastly better than the three existing farside image maps - from
Clementine, Chang'e-1 and Phil Stooke - because this map has uniform lighting everywhere. This shows the farside as it has never been seen before
by anyone. Craters are everywhere, with few maria to create patterns. The impact basins are the only landmarks, with the relative emptiness of the South
Pole-Aitken Basin dominating the southern hemisphere. The old, degraded basin in the center is Freundlich-Sharanov, 600 km in diameter with a small
patch of mare in its center, and nearly undetectable on other imagery. Hooray, Kaguya!
Chuck Wood
Related Links
Laser Altimetry instrument
Yesterday's LPOD: A Little Bit About a Normal Crater
Tomorrow's LPOD: Smaller And Smaller Rilles
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