Variable Stars in a Distant Spiral Galaxy ,1999

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Largest available format 3504 × 1948 px 1 MB

	Dimension [pixels]	Dimension in 300dpi [mm]	File size [MB]	Online Purchase
Large	3504 × 1948 px	297 × 165 mm	602 KB
Medium	1024 × 570 px	87 × 48 mm	662 KB

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UIS5093523

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Variable Stars in a Distant Spiral Galaxy ,1999

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Variable Stars in a Distant Spiral Galaxy ,1999. NASA Hubble Space Telescope (HST) view of the magnificent spiral galaxy NGC 4603, the most distant galaxy in which a special class of pulsating stars called Cepheid variables have been found. It is associated with the Centaurus cluster, one of the most massive assemblages of galaxies in the nearby universe. The Local Group of galaxies, of which the Milky Way is a member, is moving in the direction of Centaurus at a speed of more than a million miles an hour under the influence of the gravitational pull of the matter in that direction. Clusters of young bright blue stars highlight the galaxy's spiral arms. In contrast, red giant stars in the process of dying are also found. ©SSPL/NASA

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Largest available format 3504 × 1948 px 1 MB View all formats

	Dimension [pixels]	Dimension in 300dpi [mm]	File size [MB]	Online Purchase
Large	3504 × 1948 px	297 × 165 mm	602 KB
Medium	1024 × 570 px	87 × 48 mm	662 KB

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