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.

Topics to be covered:
Invited speakers will include: Frank Bertoldi, Jamie Bolton, Rychard Bouwens, Joanna Dunkley, Richard Ellis, Steven Furlanetto, Piero Madau, Matthew McQuinn, Masami Ouchi, Dominik Reichers, Michael Shull, Brian Siana, Chris Willott and Saleem Zaroubi.

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.

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.

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.

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.

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.