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TX300-year2010.jpg (448 × 190 pixels, file size: 27 KB, MIME type: image/jpeg)

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English: Basic size comparison between dwarf planet candidates Quaoar and 2002 TX300. Given the icy low density of TX300, it is remotely possible that it is in hydrostatic equilibrium. Proper colors and albedos not accounted for.
Date
Source Based off of the work of Martin Kornmesser. This is a simply modified version of File:Iau dozen.jpg intended to illustrate how TX300 has had its size estimate drop significantly.
Author Kevin Heider
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Other versions IAU 2006 (Martin Kornmesser) original File:Iau dozen.jpg

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1 January 2010

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Date/TimeThumbnailDimensionsUserComment
current01:50, 2 January 2010Thumbnail for version as of 01:50, 2 January 2010448 × 190 (27 KB)Kheider== {{int:filedesc}} == {{Information |Description={{en|1=Basic size comparison between dwarf planet candidates Quaoar and 2002 TX<sub>300</sub>. Given the icy low den

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