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File:A disc of rocky debris from a disrupted planetesimal (geminiann17003a).jpg

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Summary

Description
English: A disc of rocky debris from a disrupted planetesimal surrounds white dwarf plus brown dwarf binary star. The white dwarf is the burned-out core of a star that was probably similar to the Sun, the brown dwarf is only ~60 times heavier than Jupiter, and the two stars go around each other in only a bit over two hours.
Date 23 February 2017, 13:58:00 (upload date)
Source A disc of rocky debris from a disrupted planetesimal
Author International Gemini Observatory/NOIRLab/NSF/AURA/UCL/University of Warwick/University of Sheffield//Mark Garlick
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Captions

A disc of rocky debris from a disrupted planetesimal surrounds white dwarf plus brown dwarf binary star.

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media type

image/jpeg

height

6,000 pixel

width

4,500 pixel

data size

3,153,351 byte

checksum

e430baa1cb9385052a6a8e53b37c3b7048ed10a4

determination method: SHA-1

inception

23 February 2017

pHash checksum

47bzqia9ypytga5fq9hmqar3zp7g5u15r1casro8lpv44g7s9p

determination method: JImagehash perceptual hash

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Date/TimeThumbnailDimensionsUserComment
current23:05, 22 October 2023Thumbnail for version as of 23:05, 22 October 20234,500 × 6,000 (3.01 MB)OptimusPrimeBot#Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/geminiann17003a.jpg via Commons:Spacemedia
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