The Institute of Astronomy plans to host one large summer conference each year. Below is a list of upcoming and previous meetings at the IoA.
Upcoming & Recent Meetings
31 March 2014 - 1 April 2014
The 14th BritGrav (British Gravity) Meeting will be held on 31 March – 1 April 2014
at the University of Cambridge in St Catharine's College.
28 July 2014 - 1 August 2014
The University of Cambridge Institute of Astronomy will host a 5 day scientific meeting to further our understanding of the formation and evolution of planetary systems. The meeting will focus on the full lifetime of planetary systems, from pre- to post-main sequence host star stages, and the connections that can be made by viewing these evolutionary stages as parts of a whole. In this way, the program aims to provide an integrative approach rather than focusing on each stellar stage separately.
7 September 2009 - 8 September 2009
The aim of this conference is to bring together an outstanding group of young researchers to discuss theoretical and observational progress toward understanding accretion disc physics in Young Stellar Objects, compact binaries, and galactic nuclei.
21 July 2008 - 25 July 2008
Putting Gravity to Work: from black holes to galaxy clusters was a high energy astrophysics conference held at the Institute of Astronomy, Cambridge, in celebration of Andy Fabian's 60th birthday.
17 July 2006 - 21 July 2006
Observations of the later evolutionary stages of discs around young stars offer the best opportunity to study planet formation from an observational perspective. Localised clearing of dust and gas in discs can be inferred from a variety of imaging/spectroscopic diagnostics and is often interpreted as evidence for planet formation; alternatively, such clearing results from some other process which needs to be taken into account when assessing the environment in which planets form.
6 September 2004 - 10 September 2004
Large-scale starbursts are very common features of early galaxy evolution. At high redshifts, the majority of the present-day "normal" galaxy progenitors either appear to be undergoing violent gravitational interactions, or experience very active star formation throughout.