Meetings
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
1 August 2021 - 7 August 2021
A century ago the theory of stellar evolution was in its infancy. Ideas abounded on the equation of state, the internal structure and the energy source. The next few decades saw consolidation with Saha' theory of ionization in 1920 leading to Payne's affirmation that the stars are predominantly hydrogen in 1925, Gamov's calculations of quantum mechanical tunnelling in 1925 leading ultimately to the nuclear fusion reactions we understand today.
Previous Meetings
2 August 2010 - 6 August 2010
The Institute of Astronomy, Cambridge, summer conference will focus on Dark Matter, bring together recent progress in astrophysical studies, direct and indirect detection experiemnts, and the LHC.
We invite applications for contributed talks and posters to fill an expanded format for the Darkness Visible meeting to be held at the Institute of Astronomy, Cambridge (UK). This meeting will bring together particle- and astro - physicists (theoretical, experimental and observational) to present recent advances in our understanding of dark matter at scales ranging from particle pysics to cosmology.
Meeting Website
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.
Meeting Website
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.
Meeting Website
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.
Meeting Website
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.
Meeting Website
