Astrophoto Lab
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The
Curious Case of Calcium-rich Supernovae
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NGC 5714 Spiral galaxy RA 14h 38m 9.96s Dec 46° 38' 22.57" Boötes 120 million light-years 13.4 3.2 by 0.4 arcmin 3.37 x 1.96 arcminutes North is 6.3° left of vertical ESA/Hubble & NASA March 26, 2018 |
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ABOUT THIS IMAGE: 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 on May 12, 1787, NGC 5714 was host to a fascinating and rare event in 2003. A faint supernova called SN 2003dr.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 of calcium. Calcium-rich
supernovae are rare and hence of great interest to astronomers. Astronomers
still struggle to explain these particular explosions as their existence
presents a challenge to both observation and theory. In particular, their
appearance outside of galaxies, their lower luminosity compared to other
supernovae, and their rapid evolution, are still open questions for researchers. |
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