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Description: The Mass-Luminosity Relation For main-sequence stars, mass and luminosity are directly correlated—the more massive a star, the more luminous it is. A main-sequence star of 10 solar masses has roughly 3000 times the Sun’s luminosity; one with 0.1 solar masses has a luminosity of only about 0.001 solar luminosities. To fit them on the page, the luminosities and masses are plotted using logarithmic scales. Picture Stats: Views: 759 Filesize: 107.15kB Height: 900 Width: 762 Source: https://biology-forums.com/index.php?action=gallery;sa=view;id=18395 |