Dosya:NGC 5714 - HST - Potw1813a.tif
Ebadê verqaytê JPG na dosyay TIF: 800 × 467 piksel. Agoznayışê bini: 320 × 187 piksel | 640 × 373 piksel | 1,024 × 597 piksel | 1,280 × 747 piksel | 2,560 × 1,493 piksel | 4,037 × 2,355 piksel.
Ebato oricinale (4,037 × 2,355 pikselan, ebatê dosya: 17.67 MB, MIME tipê cı: image/tiff)
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Tarix/Zeman | Resımo qıckek | Ebadi | Karber | Mışewre | |
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nıkayên | 05:26, 26 Adare 2018 | 4,037 - 2,355 (17.67 MB) | Fabian RRRR | == {{int:filedesc}} == {{Information |description={{en|1='''The curious case of calcium-rich supernovae This image, captured by the Advanced Camera for Surveys (ACS) on the NASA/ESA Hubble Space Telescope, shows the spiral galaxy NGC 5714, about 130 million light-years away in the constellation of Boötes (the Herdsman). NGC 5714 is classified as a Sc spiral galaxy, but its spiral arms — the dominating feature of spiral galaxies — are almost impossible to see, as NGC 1787 presents itself at an almost perfectly edge-on angle. Discovered by William Herschel in 1787, NGC 5714 was host to a fascinating and rare event in 2003. A faint supernova appeared about 8000 light-years below the central bulge of NGC 5714. Supernovae are the huge, violent explosions of dying stars, and the one that exploded in NGC 5714 — not visible in this much later image — was classified as a Type Ib/c supernova and named SN 2003dr. It was particularly interesting because its spectrum showed strong signatures o... |
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