File:Disintegration Scenario for Asteroid P-2013 R3.jpg

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Summary

Description
English: Though fragile comet nuclei have been seen falling apart as they near the Sun, nothing like the slow breakup of an asteroid has ever before been observed in the asteroid belt. A series of Hubble Space Telescope images shows that the fragments are drifting away from each other at a leisurely one mile per hour. This makes it unlikely that the asteroid is disintegrating because of a collision with another asteroid. A plausible explanation is that the asteroid is crumbling due to a subtle effect of sunlight. This causes the rotation rate to slowly increase until centrifugal force pulls the asteroid apart. The asteroid's remnant debris, weighing in at 200,000 tons, will in the future provide a rich source of meteoroids.
Date
Source https://hubblesite.org/contents/media/images/2014/15/3327-Image.html?news=true
Author NASA, ESA, and A. Feild (STScI)

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current18:15, 2 December 2022Thumbnail for version as of 18:15, 2 December 20223,000 × 1,545 (683 KB)Nrco0eUploaded a work by NASA, ESA, and A. Feild (STScI) from https://hubblesite.org/contents/media/images/2014/15/3327-Image.html?news=true with UploadWizard
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