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Explanation: Spiral galaxy ESO 137-001 hurtles through massive galaxy cluster Abell 3627 some 220 million light years away. The distant galaxy is seen in this colorful Hubble/Chandra composite image through a foreground of the Milky Way's stars toward the southern constellation Triangulum Australe. As the spiral speeds along at nearly 7 million kilometers per hour, its gas and dust are stripped away when ram pressure with the cluster's own hot, tenuous intracluster medium overcomes the galaxy's gravity. Evident in Hubble's near visible light data, bright star clusters have formed in the stripped material along the short, trailing blue streaks. Chandra's X-ray data shows off the enormous extent of the heated, stripped gas as diffuse, darker blue trails stretching over 400,000 light-years toward the bottom right. The significant loss of dust and gas will make new star formation difficult for this galaxy. A yellowish elliptical galaxy, lacking in star forming dust and gas, is just to the right of ESO 137-001 in the frame.
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: galaxy cluster - spiral galaxy
Publications with words: galaxy cluster - spiral galaxy
See also:
- APOD: 2026 January 14 Á M51: The Whirlpool Galaxy
- IC 342: Hidden Galaxy in Camelopardalis
- NGC 253: Dusty Island Universe
- APOD: 2025 November 5 Á Spiral Galaxy NGC 3370 from Hubble
- APOD: 2025 October 3 Á Pandora's Cluster of Galaxies
- Portrait of NGC 1055
- APOD: 2025 September 4 Á NGC 4565: Galaxy on Edge