Jan 27, 2020
November 09, 2022 11:00AM (EST)


Light from a star that exploded over 11 billion years ago was captured by Hubble Space Telescope not just as one postcard from the remote past but three messages that chronicle the fading fireball over a period of one week.

For starters, the feeble light from the supernova was amplified by the gravitational field of an enormous foreground galaxy cluster, Abell 370. The gravitational warp in space acts as a cosmic lens, bending and magnifying the light from the more distant supernova, which was located far behind the cluster.

A bonus for astronomers is that not one but three images of the supernova appear in the photo, strung along the cluster. They show the explosion over different times that all arrived at Hubble simultaneously. A clue is that the cooling supernova fireball appears in slightly different colors among the supernova images. The images arrived at different times because length of the pathways the supernova light followed is different. The later images were delayed due to taking a longer route across "valleys" of warped space.

supernova abell 370.png
Lensed Supernova in Abell 370

Three different moments in a far-off supernova explosion were captured in a single snapshot by NASA's Hubble Space Telescope. The star exploded more than 11 billion years ago, when the universe was less than a fifth of its current age of 13.8 billion years.

This is the first detailed look at a supernova so early in the universe's history. The research could help scientists learn more about the formation of stars and galaxies in the early universe. The supernova images are also special because they show the early stages of a stellar explosion.

"It is quite rare that a supernova can be detected at a very early stage, because that stage is really short," explained Wenlei Chen, first author of the paper and a postdoctoral researcher in the University of Minnesota School of Physics and Astronomy. "It only lasts for hours to a few days, and it can be easily missed even for a nearby detection. In the same exposure, we are able to see a sequence of the images—like multiple faces of a supernova."

This was possible through a phenomenon called gravitational lensing, which was first predicted in Einstein's theory of general relativity. In this case, the immense gravity of the galaxy cluster Abell 370 acted as a cosmic lens, bending and magnifying the light from the more distant supernova located behind the cluster.

The warping also produced multiple images of the explosion over different time periods that all arrived at Earth at the same time and were caught in one Hubble image. That was possible only because the magnified images took different routes through the cluster due both to differences in the length of the pathways the supernova light followed, and to the slowing of time and curvature of space due to gravity.

The Hubble exposure also captured the fading supernova's rapid change of color, which indicates temperature change. The bluer the color means the hotter the supernova is. The earliest phase captured appears blue. As the supernova cooled its light turned redder.

"You see different colors in the three different images," said Patrick Kelly, study leader and an assistant professor in the University of Minnesota's School of Physics and Astronomy. "You've got the massive star, the core collapses, it produces a shock, it heats up, and then you're seeing it cool over a week. I think that's probably one of the most amazing things I've ever seen!"

This is also the first time astronomers were able to measure the size of a dying star in the early universe. This was based on the supernova's brightness and rate of cooling, both of which depend on the size of the progenitor star. Hubble observations show that the red supergiant whose supernova explosion the researchers discovered was about 500 times larger than the Sun.

Chen, Kelly, and an international team of astronomers found this supernova by sifting through the Hubble data archives, looking for transient events. Chen wrote machine-learning algorithms to find these events, but this was the only multiply imaged supernova identified.

Chen and Kelly both have time planned for NASA's James Webb Space Telescope to observe even more distant supernovae. They hope to contribute to a catalog of very far-off supernovae to help astronomers understand if the stars that existed many billions of years ago are different from those in the nearby universe.

The team's paper, entitled "Shock cooling of a red-supergiant supernova at redshift 3 in lensed images," will be published in Nature on November 10.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, in Washington, D.C.



Ann Jenkins
Space Telescope Science Institute, Baltimore, Maryland

Ray Villard
Space Telescope Science Institute, Baltimore, Maryland


Wenlei Chen
University of Minnesota, Minneapolis, Minnesota

Patrick Kelly
University of Minnesota, Minneapolis, Minnesota


Shock cooling of a red-supergiant supernova at redshift 3 in lensed images
The core-collapse supernova of a massive star rapidly brightens when a shock, produced following the collapse of its core, reaches the stellar surface. As the shock-heated star subsequently expands and cools, its early-time light curve should have a simple dependence on the size of the progenitor1 and therefore final evolutionary state. Measurements of the radius of the progenitor from early light curves exist for only a small sample of nearby supernovae 2,3,4,5,6,7,8,9,10,11,12,13,14, and almost all lack constraining ultraviolet observations within a day of explosion. The several-day time delays and magnifying ability of galaxy-scale gravitational lenses, however, should provide a powerful tool for measuring the early light curves of distant supernovae, and thereby studying massive stellar populations at high redshift. Here we analyse individual rest-frame exposures in the ultraviolet to the optical taken with the Hubble Space Telescope, which simultaneously capture, in three separate gravitationally lensed images, the early phases of a supernova at redshift z ≈ 3 beginning within 5.8 ± 3.1 hours of explosion. The supernova, seen at a lookback time of approximately 11.5 billion years, is strongly lensed by an early-type galaxy in the Abell 370 cluster. We constrain the pre-explosion radius to be 533+154−119533−119+154 solar radii, consistent with a red supergiant. Highly confined and massive circumstellar material at the same radius can also reproduce the light curve, but because no similar low-redshift examples are known, this is unlikely.

The HST data used for this study can be retrieved from the NASA Mikulski Archive for Space Telescopes ( The supernova is found in the HST imaging of the Abell 370 field acquired from programme GO-11591 (PI J.-P. Kneib). The LBT spectroscopy data are available from the LBT archive ( The Keck MOSFIRE data can be retrieved from the Keck Observatory Archive ( The HFF data and models can be downloaded from Additional data including the MMT spectroscopic data, the HST coaddition and image differencing data, the GALFIT scripts and resulting models, the HST photometry data of the SN host galaxy, the SN light curve fitting script and resulting MCMC data, and our best-fit GLAFIC lens model are available from


It is amazing to find a such an early Supernova, from 11 billion years ago, thanks to the marvels of the gravitational lensing found in the dense mass of Abell 370. And this is also the first time astronomers were able to measure the size of a dying star so deep in the early universe.