Watching a red supergiant go supernova

Publicly released:
International
Image by Pexels from Pixabay
Image by Pexels from Pixabay

International researchers have observed the early stages of a supernova from a red supergiant star around 11.5 billion years ago. The team analyzed 3 images from the Hubble Space Telescope taken in 2010 which show the beginnings of a star going supernova, something that they say has been rarely observed before. The team found that the radius of the star appeared to be about 530 times larger than our Sun, and say that there was a rapid cooling of the star which took place over eight days.

Media release

From: Springer Nature

Astronomy: Early phases of a supernova captured

Observations of the early phases of a supernova (within hours of the star’s explosion) that occurred approximately 11.5 billion years ago are presented in a paper published in this week’s Nature.

As part of a systematic search of archival imaging from the Hubble Space Telescope, Wenlei Chen and colleagues identified images of a rapidly evolving supernova in the Abell 370 galaxy cluster obtained in December 2010. The three gravitationally lensed images show the early phases of the supernova at different times, beginning around six hours after the explosion of the star. The authors report that the supernova has a redshift (a measure of how much the Universe has expanded) of approximately 3, corresponding to the event taking place around 11.5 billion years ago. An analysis of the brightness and colour of the images suggests that rapid cooling took place over the course of around eight days. From this, the authors were able to calculate the radius of the star prior to the explosion to be about 530 times that of the Sun. This size is consistent with that of a red supergiant.

Chen and co-authors suggest that the discovery of further gravitationally lensed supernovae offer the opportunity to study massive stellar populations at high redshift.

Journal/
conference:
Nature
Research:Paper
Organisation/s: University of Minnesota, USA
Funder: We are most fortunate to have the opportunity to conduct observations from this mountain. P.L.K. is supported by US National Science Foundation (NSF) grant AST-1908823. J.M.D. acknowledges support from projects PGC2018-101814-B-100 and MDM-2017-0765. M.O. acknowledges support from World Premier International Research Center Initiative, MEXT, Japan, and JSPS KAKENHI grants JP20H00181, JP20H05856, JP22H01260 and JP18K03693. A.Z. acknowledges support by grant 2020750 from the USA–Israel Binational Science Foundation (BSF) and grant 2109066 from the US NSF, and by the Ministry of Science & Technology, Israel. A.V.F. is grateful for assistance from the Christopher R. Redlich Fund, the UC Berkeley Miller Institute for Basic Research in Science (where he was a Miller Senior Fellow), and many individual donors. We acknowledge the help of W. Zheng with the Keck MOSFIRE observations.
Media Contact/s
Contact details are only visible to registered journalists.