We are an inter-university research group focussed on utilising radar data from past, present and future planetary missions.
The group covers a range of research areas from planetary surface mapping to the creation of algorithms for change detection.
We study various planetary bodies, with our main focusses being on Venus and the Moon.
The main area studied on the Moon is the characterisation of subsurface ice around the South Pole. The search will be achieved by in-house developed software at Royal Holloway as part of a collaboration between the UK Space Agency and the ISRO in India.
In regards to Venus, the range of topics studied is much more varied. Mapping is a primary output of the group,
with the southern region of Lada Terra and also areas around the Beta-Atla-Themis (BAT) triangle being studied in greater
detail. Change detection algorithms are being developed for use when data is returned from future missions.