Transiting planets with the CoRoT space mission

Lead Research Organisation: University of Exeter
Department Name: Physics


In this Rolling Grant application, we describe an interdisciplinary programme of observational and theoretical research in extrasolar planets, to be conducted at the University of Exeter, through a new collaboration between the Astrophysics Group in the School of Physics and the Centre for Geophysical and Astrophysical Fluid Dynamics (CGAFD) in the School of Engineering, Computing and Mathematics (SECaM). The research programme combines state-of-the-art observations and theoretical calculations to detect, determine the properties of, and model the formation and evolution of extrasolar planets. We will perform three-dimensional self-gravitating radiation hydrodynamical simulations of gas accretion by a protoplanet core to form giant planets to produce more accurate models of young gas giant planets. We will directly image gas giant planets around young nearby stars using adaptive optics on the VLT and the Gemini Planet Imager and use these observations to test the models. We will undertake space-based observations of transiting planets using HST and Spitzer to understand the chemistry and dynamics of the atmospheres of giant planets that are very close to their stars and model these atmospheres using convective three-dimensional simulations. Finally, we will analyse the data from CoRoT, the first space-based transiting planet search mission, to detect and characterise planets of Neptune-mass and below and the systems they are part of, as well as search for light reflected by giant planets.

Related Projects

Project Reference Relationship Related To Start End Award Value
ST/G002266/1 01/10/2009 31/01/2010 £272,257
ST/G002266/2 Transfer ST/G002266/1 18/01/2010 31/03/2012 £242,685
Description This grant funded me and a PDRA for three years to work on the detection and characterisation of transiting planets, mainly using data from the CoRoT space mission, the Hubble Space Telescope and the Gemini telescopes. One of the main outcomes was the development of novel methods to model instrumental systematic effects and / or stellar variability using a technique known as Gaussian Process regression, which we introduced to the exoplanet community, and where it is now becoming widely used.
Exploitation Route The novel light curve analysis methods we developed are becoming widely used in the community. This work also contributed to establishing the prevalence of clouds in the atmospheres of numerous hot Jupiter planets, which is prompting renewed interest in modelling and understanding clouds in hot Jupiters and brown dwarfs.
Sectors Digital/Communication/Information Technologies (including Software),Education

Description The main impact of this research beyond its immediate subject matter is educational: we were the first to apply Gaussian Process regression to exoplanet time-series data, and this has had a significant impact in the way in which researchers and students now approach the analysis of such datasets, including in other areas of astronomy that involve time-series or correlated datasets (e.g pulsar science and CMB cosmology)
First Year Of Impact 2012
Sector Digital/Communication/Information Technologies (including Software),Education