Binary Star Eta Carinae—A Source of Very High-energy Cosmic Gamma Radiation

Binary Star Eta Carinae—A Source of Very High-energy Cosmic Gamma Radiation

The binary star Eta Carinae may be about to explode. However, no one knows when. It may be next year. It may be a million years from now. Eta Carinae's mass—about 100 times greater than our Sun—makes it an excellent candidate for a full blown supernova. Historical records do show that about 170 years ago Eta Carinae underwent an unusual outburst that made it one of the brightest stars in the southern sky. This binary star in the Homunculus Nebula is located 7,500 light-years away in the constellation Carina. Eta Carinae is the only star system currently thought to emit natural LASER light. 

With the gamma-ray telescopes of the High Energy Stereoscopic System (H.E.S.S.), astrophysicists have detected very high energy gamma rays from Eta Carinae. It constitutes a new type of source for such high-energy radiation. The DESY animation by Science Communication Lab takes you on an interstellar roadtrip to this extraordinary system.

Video Credit: Deutsches Elektronen-Synchrotron (DESY)

Duration: 3 minutes, 35 seconds

Release Date: July 1, 2020

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