File:Gliese 105.gif

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DescriptionGliese 105.gif	English: Is the dim star to the upper right of this false-color picture the coolest possible normal star? From this recent picture by the Hubble Space Telescope, astronomers have estimated its mass is just high enough for it to fuse hydrogen into helium in its core. In general, the higher an object's mass, the higher it's core density and temperature. Above a certain point, the intense core conditions cause hydrogen atoms to move so fast that many stick or "fuse" after collision, releasing enormous amounts of energy. Were this object less massive, the object would shine by gravitational contraction and so be termed a "brown dwarf" rather than a normal main-sequence "star." The star on the left is so much brighter than the "coolest star" that it creates the white streak and dramatic pattern visible in the image.
Date	20 September 1995
Source	https://apod.nasa.gov/apod/ap950920.html
Author	NASA, HST, WFPC 2, D. Golimowski (JHU)
Other versions	jpg version (a bit different)

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	13:28, 22 May 2008		502 × 284 (54 KB)	Fran Ara	{{Information \|Description= Gliese 105 \|Source=http://apod.nasa.gov/apod/ap950920.html \|Date= \|Author=NASA \|Permission=see below \|other_versions= }}

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