Copernicus and Kepler (Marco Lorenzi)

Contains: Solar system body or event

Copernicus and Kepler

Link: https://www.glitteringlights.com/

Acquisition type: Lucky imaging

Copernicus and Kepler

Link: https://www.glitteringlights.com/

Acquisition type: Lucky imaging

One of the most prominent and striking craters on the Moon, Copernicus (at the right in the image) is found in the Oceanus Procellarum, slightly northwest of the center of the Moon's face.
It has a vaguely hexagonal shape with beautiful terraced walls and in the center it does not have a single mountain but several peaks and groups of hills.
Copernicus is easily spotted whenever it is sunlit because it is in the heart of a massive system of rays that extend at least 800 kilometers across the surrounding sea, overlapping with rays from other craters, notably Kepler's crater visible on the left of the image.
These lunar rays are strips of material ejected during the impact that formed the crater and look somewhat like the thin spokes coming from the hub of a wheel. Several smaller craters are visible all around Copernicus, with some of these forming sinuous chains.

North of Copernicus are the Montes Carpatus which to the west (left in the picture) disperse to form sparser hills. Further west is Kepler with its impressive system of Splash Rays extending over 300 kilometers over the Oceano Procellarum. The ejecta mantle appears lighter in contrasts to the dark basaltic materials of the surrounding ocean. Below Kepler is the interesting Encke crater, with its low rim and somewhat polygonal shape.

Mosaic of 2 images

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The “AstroBin Image of the Day and Top Picks”, or IOTD/TP, is a long-running system to promote beautiful, interesting, peculiar, or otherwise amazing astrophotographs, with a focus on technical excellence. Learn more.

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Views by Submitters (available since September 19th, 2023) Every image is assigned to 50% of available Submitters. In the event that at least 80% of them don't view the image before its time in the IOTD/TP process expires, it's assigned to the other 50% of Submitters and the process begins anew.
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Copernicus and Kepler

Copernicus and Kepler

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Copernicus and Kepler

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