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Authors: Schinella, Elyse
Date: 2014
Language: eng
Resource Type: Thesis PhD
Identifier: http://hdl.handle.net/1959.14/1142279
Description: "A thesis submitted for the fulfillment of the degree: Doctor of Philosophy February, 2014"
Date: 2011
Language: eng
Resource Type: conference paper
Identifier: http://hdl.handle.net/1959.14/172528
Description: Venus and Earth share a similar size, mass and density, however Venus' high surface temperatures, pressures, dehydrated crust and absence of subduction zones, makes the surface unique. One area which ... More
Reviewed: Reviewed
Date: 2007
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/20471
Description: Standard models for a warm, wet early Mars require a significant CO₂-H₂O atmosphere in the past. The source for these phases is assumed to be volcanic degassing. However, no consistent, dynamical mode ... More
Reviewed: Reviewed
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