The Astronomy group is part of Physics and Astronomy
at the University of Southampton
, which is currently ranked 4th in the UK for Physics and is a world top-30 Physics department. We are part of the larger Faculty of Physical Sciences and Engineering
, which brings together fundamental research with one of the UK's largest and strongest Computer Science
departments. We are also part of the new STAG (Southampton Theory, Astronomy and Gravity) Research Centre
, which combines researchers across Physics, Astronomy and Mathematics
, and SEPnet
, a consortium of nine partner universities in the South East Region of England for advancing and protecting Physics.
Research at Southampton Astronomy covers a broad range of astrophysical phenomena:
We are a leading group in the UK researching the growth and evolution of compact objects. This includes white dwarfs, neutron stars and black holes across their full mass scale. We use multiwavelength observations to examine the relationship between the phenomena of accretion and outflows. This is bringing us closer to understanding how some of the most extreme objects in the cosmos form, grow and change with time, and how they impact their surrounding galaxies.
As part of the Astronomy group, the Space Environment Physics group
study the interaction between the Sun and the magnetospheres and upper atmospheres of several planets in the Solar System - from large-scale dynamics of magnetospheres down to the behaviour of the aurora on the finest scales.
Time Domain Astronomy
We are leading large projects across the optical, infrared, X-ray and radio wavelengths studying the time-domain universe. This includes research that spans a wide range of astrophysical events: from supernovae
and other cosmic explosions that last weeks and months, to variability from accretion onto black holes on the timescale of milliseconds. We aim to discover new transient events in the sky and to use their characteristic variations to gain a deeper understanding of extreme physics and the life cycles of stars, and to measure the expansion rate of the universe.