Collisional and structural properties of water ice in planet-forming regions

With the number of detected exoplanets standing at close to 2000, it seems that planets are ubiquitous throughout the universe. However, the processes leading to their formation are not well understood. It is widely accepted that planets form by dust aggregation from the material of protoplanetary d...

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Bibliographic Details
Main Author: Hill, Catherine
Published: Open University 2015
Subjects:
Online Access:http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.680394