ESA Science & Technology - Hubble breaks record for furthest supernova [heic1306]

The supernova, designated SN UDS10Wil [1], belongs to a special class of exploding stars known as Type Ia supernovae. These bright beacons are prized by astronomers because they can be used as a yardstick for measuring cosmic distances, thereby yielding clues to the nature of dark energy, the mysterious force accelerating the rate of expansion of the Universe.

"This new distance record holder opens a window into the early Universe, offering important new insights into how these supernovae form," said astronomer David O. Jones of The Johns Hopkins University in Baltimore, Md., lead author on the science paper detailing the discovery. "At that epoch, we can test theories about how reliable these detonations are for understanding the evolution of the Universe and its expansion."

One of the debates surrounding Type Ia supernovae is the nature of the fuse that ignites them. This latest discovery adds credence to one of two competing theories of how they explode. Although preliminary, the evidence favours the explosive merger of two burned out stars – small, dim, and dense stars known as white dwarfs, the final state for stars like our Sun.

The discovery was part of a three-year Hubble program called the CANDELS+CLASH Supernova Project, begun in 2010 [2]. This program aimed to survey faraway Type Ia supernovae to determine their distances and see if their behaviour has changed over the 13.8 billion years since the Big Bang, using the sharpness and versatility of Hubble's Wide Field Camera 3.

So far, CANDELS+CLASH has uncovered more than 100 supernovae of all types that exploded from 2.4 to over 10 billion years ago. The team has identified eight of these discoveries as Type Ia supernovae that exploded more than 9 billion years ago – including this new record-breaker, which, although only four percent older than the previous record holder, pushes the record roughly 350 million years further back in time [3].

The supernova team's search technique involved taking multiple near-infrared images spaced roughly 50 days apart over the span of three years, looking for a supernova's faint glow. After spotting SN UDS10Wil in December 2010, the CANDELS team then used the spectrometer on Hubble's Wide Field Camera 3, along with the European Southern Observatory's Very Large Telescope, to verify the supernova's distance and to decode its light, hoping to find the unique signature of a Type Ia supernova.

Finding remote supernovae opens up the possibility to measure the Universe's accelerating expansion due to dark energy [4]. However, this is an area that is not fully understood – and nor are the origins of Type Ia supernovae. "This new result is a really exciting step forward in our study of supernovae and the distant Universe," said team member Jens Hjorth of the Dark Cosmology Centre at the Niels Bohr Institute, University of Copenhagen. "We can begin to explore and understand the stars that cause these violent explosions."

The team's preliminary evidence shows a sharp decline in the rate of Type Ia supernova blasts between roughly 7.5 billion years ago and more than 10 billion years ago. This, combined with the discovery of such Type Ia supernovae so early in the Universe, suggests that the explosion mechanism is a merger between two white dwarfs.

In the single white dwarf scenario – a pathway in which a white dwarf gradually feeds off a partnering normal star and explodes when it accretes too much mass – the rate of supernovae can be relatively high in the early Universe, because some of these systems can reach the point of explosion very quickly. The steep drop-off favours the double white dwarf mechanism, because it predicts that most stars in the early Universe are too young to become Type Ia supernovae.

Knowing what triggers Type Ia supernovae will also show how quickly the Universe enriched itself with heavier elements, such as iron. These exploding stars produce about half of the iron in the Universe, the raw material for building planets, and life.

The team's results will appear in the 10 May 2013 issue of The Astrophysical Journal.

Notes

[1] The supernova has been catalogued as SN UDS10Wil in the CANDEL-CLASH list. It has also been nicknamed SN Wilson, after the 28th U.S. president Woodrow Wilson.

[2] This project searches for supernovae in near-infrared light and verifies their distances with spectroscopy. The supernova search draws on two large Hubble programs studying distant galaxies and galaxy clusters: the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS) and the Cluster Lensing and Supernova Survey with Hubble (CLASH).

[3] The previous record holder was recently announced by a team that identified a supernova that exploded around 9 billion years ago (redshift 1.7). The paper was published in The Astrophysical Journal (Rubin et al. 2013 ApJ 763 35), available from the right-hand menu.

[4] It has been known since the late 1920s that distant galaxies appear to be moving away from us with a speed that is proportional to their distance. Edwin Hubble and Georges Lemaître were the first to infer that this implied the whole Universe is expanding. In 2011, the Nobel Prize in Physics was awarded to the teams of astronomers that discovered, using Type Ia supernovae, that this expansion is actually accelerating – Adam Riess of Johns Hopkins University, Saul Perlmutter of the University of California at Berkeley, and Brian Schmidt of the Australian National University in Canberra. This acceleration is attributed to dark energy, whose nature is unknown.

Notes for editors

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

The research is presented in a paper entitled "The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914", accepted for publication in 10 May 2013 issue of The Astrophysical Journal.

The international team of astronomers in this study consists of:

D. O. Jones (Johns Hopkins University, USA), S. A. Rodney (Johns Hopkins University, USA; Hubble Fellow), A. G. Riess (Johns Hopkins University, USA; Space Telescope Science Institute, USA), B. Mobasher (University of California, USA), T. Dahlen (Space Telescope Science Institute, USA), C. McCully (The State University of New Jersey, USA), T. F. Frederiksen (University of Copenhagen, Denmark), S. Casertano (Space Telescope Science Institute, USA), J. Hjorth (University of Copenhagen, Denmark), C. R. Keeton (The State University of New Jersey, USA), A. Koekemoer (Space Telescope Science Institute, USA), L. Strolger (Western Kentucky University, USA), T. G. Wiklind (Joint ALMA Observatory, ESO, Chile), P. Challis (Harvard/Smithsonian Center for Astrophysics, USA), O. Graur (Tel-Aviv University, Israel;  American Museum of Natural History, USA), B. Hayden (University of Notre Dame, USA), B. Patel (The State University of New Jersey, USA), B. J. Weiner (University of Arizona, USA), A. V. Filippenko (University of California, USA), P. Garnavich (University of Notre Dame, USA), S. W. Jha (The State University of New Jersey, USA), R. P. Kirshner (Harvard/Smithsonian Center for Astrophysics, USA), S. M. Faber (University of California, USA), H. C. Ferguson (Space Telescope Science Institute, USA), N. A. Grogin (Space Telescope Science Institute, USA), and D. Kocevski (Harvard/Smithsonian Center for Astrophysics, USA).

Contacts

David Jones
The Johns Hopkins University
Baltimore, USA
Tel: +1-410-516-8312
Cell: +1-541-740-0816
Email: djonespha.jhu.edu

Jens Hjorth
Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen
Copenhagen, Denmark
Tel: +45-353-25928
Email: jensdark-cosmology.dk

Nicky Guttridge
Hubble/ESA
Garching, Germany
Tel: +49-89-3200-6855
Email: nguttridpartner.eso.org