Astronomy:Zombie star

From HandWiki

A zombie star is a hypothetical result of a Type Iax supernova which leaves behind a remnant star, rather than completely dispersing the stellar mass.[1][2][3][4][5] Type Iax supernovae are similar to Type Ia, but have a lower ejection velocity and lower luminosity.[6] Type Iax supernovae may occur at a rate between 5 and 30 percent of the Ia supernova rate. Thirty supernovae have been identified in this category.[7]

In a binary system consisting of a white dwarf and a companion star, the white dwarf strips away material from its companion. Normally the white dwarf would eventually reach a critical mass, and fusion reactions would make it explode and completely dissipate it, but in a Type Iax supernova, only half of the dwarf's mass is lost.[8]

The two inset images show before-and-after images captured by NASA's Hubble Space Telescope of Supernova 2012Z in the spiral galaxy NGC 1309. The white X at the top of the main image marks the location of the supernova in the galaxy.

Observed instances

Supernova SN 2012Z in the NGC 1309 galaxy is thought to be of Type Iax, and was discovered in 2012 by S. B. Cenko, W. Li, and A. V. Filippenko using the Katzman Automatic Imaging Telescope on January 29.15 UT as part of the Lick Observatory Supernova Search. It is believed that the more massive of the binary stars at the heart of the supernova lost substantial amounts of its hydrogen and helium to its smaller companion, becoming a white dwarf. The companion star then became larger and engulfed the white dwarf, ejecting the outer hydrogen layers of the combined star and leaving behind a helium core. In turn, the white dwarf drained matter from the companion star until the dwarf became so unstable that it exploded as a supernova, with a zombie star left behind as a remnant.[3]

There were images of the area from before the supernova, allowing before and after images, and the process of the supernova to be studied. To test the zombie star hypothesis, the area was observed again a few years after the event. The authors found that the decline of the light curve was consistent with the existence of a radioactively-heated bound remnant, but that it was difficult to come up with a model that could explain the whole light curve.[9]

This discovery is a milestone in a decades long search by astronomers for such an occurrence; the observation of SN 2012Z was the first time astrophysicists were able to identify a star system that later went supernova.[8]

SN 2008ha may be a Type Iax supernova, but significantly weaker than SN 2012Z.[3]


  1. Hubbard, Amy (6 August 2014). "Hubble sees 'zombie star' lurking in space: What it is, why it matters". Los Angeles Times ( 
  2. "Hubble discovers 'zombie star' haunting the universe". CNET. 
  3. 3.0 3.1 3.2 Weaver, Donna; Villard, Ray (6 August 2014). "NASA's Hubble Finds Supernova Star System Linked to Potential "Zombie Star"". HubbleSite - NewsCenter. 
  4. "Zombie star: Hubble spots star SN 2012Z living after supernova.". Slate Magazine. 12 August 2014. 
  5. Hauk, Alexis (6 August 2014). "Hubble Finds Supernova Star System Linked to Potential "Zombie Star"". Time Magazine. 
  6. McCully, Curtis; Jha, Saurabh W.; Foley, Ryan J.; Bildsten, Lars; Fong, Wen-fai; Kirshner, Robert P.; Marion, G. H.; Riess, Adam G. et al. (7 August 2014). "A luminous, blue progenitor system for the Type Iax supernova 2012Z". Nature 512 (512): 54–56. doi:10.1038/nature13615. PMID 25100479. Bibcode2014Natur.512...54M. 
  7. Feltman, Rachel. "Astronomers may have found a new zombie star". Washington Post. 
  8. 8.0 8.1 Choi, Charles Quixote (6 August 2014). "Supernovas Might Create Weird 'Zombie Stars'". 
  9. Curtis McCully; Saurabh W. Jha; Richard A. Scalzo; D. Andrew Howell; Ryan J. Foley; Yaotian Zeng; Zheng-Wei Liu; Griffin Hosseinzadeh et al. (2022). "Still Brighter than Pre-explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart". The Astrophysical Journal 925. doi:10.3847/1538-4357/ac3bbd.