Debris orbiting a white dwarf 插畫檔
The white dwarf shown in the illustration is one of several that an international team of astronomers has been studying. Called ZTF J0923+4236, the star exhibits a series of dips in its brightness. The team, led by Amornrat Aungwerojwit from Naresuan University, Thailand, and Boris T. Gänsicke from Warwick University, UK, has attributed these changes in brightness to clumps of dusty and rocky material that are bound to the star in a highly elongated orbit.This material, that believe, is due to planets that are in the process of disintegrating. Eventually these clumps collide with the star and pollute its atmosphere
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Getty ImagesDebris Orbiting A White Dwarf, 插圖檔
從 Getty Images 下載優越而真實的Debris orbiting a white dwarf插畫檔。在我們廣泛多元的視覺內容目錄中，探索類似的高解像度插畫檔。Product #:2161269640
從 Getty Images 下載優越而真實的Debris orbiting a white dwarf插畫檔。在我們廣泛多元的視覺內容目錄中，探索類似的高解像度插畫檔。Product #:2161269640HK$2,250HK$400
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