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Description: Fully Convective Star This drawing shows how the helium created in the cores of red dwarfs rises into the outer layers of the star by convection, while the hydrogen from the outer layers descends into the core. This process continues until the entire star is helium Picture Stats: Views: 631 Filesize: 88.66kB Height: 900 Width: 900 Source: https://biology-forums.com/index.php?action=gallery;sa=view;id=18424 |