Look Inside a Lunar Crater

Article written: 15 Apr , 2011
Updated: 24 Dec , 2015
by

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The crater shown above is located in the lunar highlands and is filled with and surrounded by boulders of all sizes and shapes. It is approximately 550 meters (1800 feet) wide yet is still considered a small crater, and could have been caused by either a direct impact by a meteorite or by an ejected bit of material from another impact. Scientists studying the Moon attempt to figure out how small craters like this were formed by their shapes and the material seen around them…although sometimes the same results can be achieved by different events.

For example, when an object from space strikes the Moon, it is typically traveling around 20 km per second (12 miles/sec). If the impact site happens to have a very hard subsurface, it can make a crater with scattered bouldery chunks composed of the hard material around it. But, if a large piece of ejected material from another impact were to strike the lunar surface at a much slower speed, as ejecta typically do (since they travel slower than incoming space debris and the Moon’s escape velocity is fairly low, meaning any ejecta that does fall back to the surface must be traveling slower than 2.38 km/s,) then the ejected chunk could break apart on impact and scatter boulders of itself around the crater…regardless of subsurface composition.

Really the only way to tell for sure which scenario has taken place around a given crater – such as the one above – is to collect and return samples from the site so they can be tested. (Of course that’s much easier said than done!)

You can read more about this image on Arizona State University’s Lunar Reconnaissance Orbiter Camera site here.

And as an added treat, take a look deep into the shadows of the crater’s interior below…I tweaked the image curves in Photoshop to wrestle some of the details out of there!

 

Brightening the shadowed area reveals details of the crater floor...and even more boulders!

Image credit: NASA/GSFC/Arizona State University. (Edited by J. Major.)

P.S.: Want to see both image versions combined? Click here. (Thanks to Mike C. for the suggestion!)

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5 Responses

  1. Mr Mike says

    @ J Major

    That was some fine filter work, black is not all black… there are discernible features on the walls and floor; now you need to add the walls and floor which were in shadow and lightened with your tweak back into a copy of the original image as a layered image and float that into place where it belongs. Cut it as you must but this will work well when combined.

    You will have the best of both worlds, the contrast is good on both pics and your filter work added value to the image scientifically. Of course that is my opinion, YMMV.

    Mike C

  2. colbite says

    Good work Jason,
    The two origins are of course plausible: a large impact mass with low velocity or a light body impacting at high velocity. The inner, small rim right on the bottom of the crater, made visible by your photo treatment, suggests the second versions as likely realistic. Chemistry, even remote, and structure of the boulders should prove it for sure.

    • It does seem like there’s an interior rim, doesn’t it? Almost with a soft central “peak”, although that’s hard to determine in a structure this small.

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