Contains:  Solar system body or event
Southern lunar, Astroavani - Avani Soares

Southern lunar

Southern lunar, Astroavani - Avani Soares

Southern lunar

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Description

Do you have the discipline to ignore the crater Clavius ​​and focus on the images of smaller craters south? The astrophotographer who recorded the image above did it, and we have to respect their work. The crater Blancanus is in the middle of the field of view and the top image is the crater Klaproth with your inner softened. Both had their depths reduced by some kind of material that covered the inside in Balancanus you can still see the central peak and Klaproth a little more. The standard explanation and almost certainly correct, what material is ejected from the fluid formation of Orientale Basin filled the interior of these craters and other low spots. Using tools available in the Quick Map of LRO is possible to determine the elevation of the interior of the crater Clavius ​​which is approximately 3000 meters below the average elevation of the crater, and Blancanus is a little deeper, about 3600 feet below, but is Klaproth much higher than 1800 meters. If a rain uniform ejecta fell through all these craters each of them should have been more shallow by the same amount. And perhaps this has happened. This would mean that each crater has already been modified, or, as is true of course for the Blancanus, some of them were younger than the other. Probably both things happened, and as the rays of craters, the distribution of ejecta was probably not uniform.

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Southern lunar, Astroavani - Avani Soares