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Template documentation This template is for use on List of largest known stars to calculate the radius of a star and format the table row if the explicit radius is not given in the source. If the source provides both the radius and method of detection, this template is not required and the information can be entered in as usual with table notation.
This page was last edited on 29 November 2023, at 09:34 (UTC).; Text is available under the Creative Commons Attribution-ShareAlike 4.0 License; additional terms may apply.
The brightest star in the Large Magellanic Cloud. S Doradus: 100 [127] Large Magellanic Cloud L/T eff: A luminous blue variable in the S Doradus instability strip. HD 37974: 99 [128] Large Magellanic Cloud L/T eff: An unusual blue hypergiant with a large dusty disk. [128] R136a1: 42.7 +1.6 −0.9 [129] Large Magellanic Cloud L/T eff
A star chart drawn 5000 years ago by the Indians in Kashmir, which also depict a supernova for the first time in human history. [7] The Nebra sky disk, a 30 cm wide bronze disk dated to 1600 BC, bears gold symbols generally interpreted as a sun or full moon, a lunar crescent, several stars including the Pleiades cluster and possibly the Milky Way.
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[6], § 5.9. If the star's mass, when on the main sequence, was below approximately 0.4 M ☉, it will never reach the central temperatures necessary to fuse helium. [7], p. 169. It will therefore remain a hydrogen-fusing red giant until it runs out of hydrogen, at which point it will become a helium white dwarf. [6], § 4.1, 6.1.
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