The Nature of Supernovae
Supernovae – brilliant explosions of stars at the ends of their lives – have been observed and studied by humanity for hundreds of years. Yet we are still working out which types of stars end up exploding as the different types of supernovae we observe in the night sky.
The answer to this question will impact our understanding of how stars evolve, how they create and spread the elements that comprise the periodic table (and our bodies), and how we use them as tools for other experiments in astrophysics.
Type Ia supernovae, specifically, have famously been used as “standard candles” to measure distances to other galaxies. This use led to the discovery that the Universe’s expansion is accelerating under the influence of something new and mysterious we call “dark energy.” But the use of Type Ia supernovae as standard candles is based on the assumption that the supernovae we see in the nearby Universe are identical in nature to the ones we observe in faraway galaxies.
Until we figure out exactly which stars explode as Type Ia supernovae, and how those explosions take place, we will never be wholly certain that we are using them correctly.
At the University's Institute of Cosmology and Gravitation (ICG), Dr Or Graur and his research group conduct observations of supernovae using the world's leading observatories and surveys in order to reveal their workings.
Our research methods
We use several avenues of research to try and figure out what kinds of stars explode as different types of supernovae, with an emphasis on Type Ia supernovae. Each of these research projects provides a different angle on the physics of the progenitor stars and the way in which the explosions unfurl.
We use both ground- and space-based surveys to discover supernovae and measure the rates at which different types of supernovae explode throughout cosmic history and in different types of galaxies.
- Watch: The Secret Lives (and Deaths) of Stars
- In the news: Super-Old Supernovas Spotted Across the Universe
We use large supernova surveys to conduct population studies of supernovae, such as examining correlations between properties of the supernovae and those of the galaxies in which they explode.
Observations of old supernovae
We use the Hubble Space Telescope to observe Type Ia supernovae hundreds of days after they explode. These observations provide clues to the physics of the explosion mechanism and the state of the star before it exploded.
- Watch: Science Bulletins: Shedding Light on Type Ia Supernovae
- In the news: Scientists observe year-long plateaus in decline of Type Ia supernova light curves
We use images taken by the Hubble Space Telescope before and after the explosions to search for predicted impacts of the supernovae on their environments.
We develop new ways to discover supernovae, such as picking out the signatures they leave on the spectra of their host galaxies.
Or Graur, David Zurek, Michael M. Shara, Adam G. Riess, Ivo R. Seitenzahl, Armin Rest
Graur, O., Maguire, K., Ryan, R., Nicholl, M., Avelino, A., Riess, A. G., Shingles, L., Seitenzahl, I. R. & Fisher, R., 1 Feb 2020, In: Nature Astronomy. 4, p. 188-195 8 p.
Graur, O., Rodney, S. A., Maoz, D., Riess, A. G., Jha, S. W., Postman, M., Dahlen, T., Holoien, T. W. -S., McCully, C., Patel, B., Strolger, L. -G., Benitez, N., Coe, D., Jouvel, S., Medezinski, E., Molino, A., Nonino, M., Bradley, L., Koekemoer, A., Balestra, I. & 21 others, , 10 Feb 2014, In: The Astrophysical Journal. 783, 1, 19 p., 28.
Kelly, P. L., Rodney, S. A., Treu, T., Foley, R. J., Brammer, G., Schmidt, K. B., Zitrin, A., Sonnenfeld, A., Strolger, L-G., Graur, O., Filippenko, A. V., Jha, S. W., Riess, A. G., Bradac, M., Weiner, B. J., Scolnic, D., Malkan, M. A., Linden, A. V. D., Trenti, M., Hjorth, J. & 11 others, , 6 Mar 2015, In: Science. 347, 6226, p. 1123-1126 4 p.
Supernova by Or Graur
Supernova: A concise illustrated introduction to the history and physics of supernovae by Dr Or Graur will be published by MIT Press in February 2022.
Discover our areas of expertise
We're researching the evolution of galaxies, from the most local to the most distant, and using their light to model stellar radiation and probe the formation and development of the Universe.
We're studying supernovae and the appearance of distance between Earth and galaxies, and measuring the positions of large-scale structures in the Universe.
Interested in a PhD in Cosmology & Astrophysics?
Browse our postgraduate research degrees – including PhDs and MPhils – at our Cosmology & Astrophysics postgraduate research degrees page.