Home > Research > Publications & Outputs > Laboratory simulation of the release of subsurf...

Associated organisational unit

View graph of relations

Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites.

Research output: Contribution to conference - Without ISBN/ISSN Conference paper

Published

Standard

Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites. / Bargery, Alistair; Lane, Stephen; Wilson, Lionel et al.
2008. Paper presented at 39th Lunar and Planetary Science Conference 2008, League City, Texas, United States.

Research output: Contribution to conference - Without ISBN/ISSN Conference paper

Harvard

Bargery, A, Lane, S, Wilson, L & Gilbert, J 2008, 'Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites.', Paper presented at 39th Lunar and Planetary Science Conference 2008, League City, Texas, United States, 10/03/08 - 14/03/08. <http://www.lpi.usra.edu/meetings/lpsc2008/pdf/1702.pdf>

APA

Vancouver

Bargery A, Lane S, Wilson L, Gilbert J. Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites.. 2008. Paper presented at 39th Lunar and Planetary Science Conference 2008, League City, Texas, United States.

Author

Bargery, Alistair ; Lane, Stephen ; Wilson, Lionel et al. / Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites. Paper presented at 39th Lunar and Planetary Science Conference 2008, League City, Texas, United States.2 p.

Bibtex

@conference{6916592629f54bf9b9517a47e315664f,
title = "Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites.",
abstract = "For most extraterrestrial studies of volcanic and aqueous activity, the processes involved can be studied only by theoretical modelling, simula-tion in analogue experiments, or examination of the geomorphological and geological record. The last of these approaches is limited by the spatial resolution and coverage of satellite data, or to the very limited localities where rovers or landers have been deployed (e.g., Viking, Mars Exploration Rovers). There have been no observed releases of water on to the surface of Mars. Therefore, a series of experiments should add insight to our understanding of this phenomenon. The experiments are intended to be primarily a study of the temperature-pressure relationships and how they affect phase changes in both pure wate",
author = "Alistair Bargery and Stephen Lane and Lionel Wilson and Jennifer Gilbert",
year = "2008",
language = "English",
note = "39th Lunar and Planetary Science Conference 2008 ; Conference date: 10-03-2008 Through 14-03-2008",

}

RIS

TY - CONF

T1 - Laboratory simulation of the release of subsurface water and brine on to the surface of Mars and icy satellites.

AU - Bargery, Alistair

AU - Lane, Stephen

AU - Wilson, Lionel

AU - Gilbert, Jennifer

PY - 2008

Y1 - 2008

N2 - For most extraterrestrial studies of volcanic and aqueous activity, the processes involved can be studied only by theoretical modelling, simula-tion in analogue experiments, or examination of the geomorphological and geological record. The last of these approaches is limited by the spatial resolution and coverage of satellite data, or to the very limited localities where rovers or landers have been deployed (e.g., Viking, Mars Exploration Rovers). There have been no observed releases of water on to the surface of Mars. Therefore, a series of experiments should add insight to our understanding of this phenomenon. The experiments are intended to be primarily a study of the temperature-pressure relationships and how they affect phase changes in both pure wate

AB - For most extraterrestrial studies of volcanic and aqueous activity, the processes involved can be studied only by theoretical modelling, simula-tion in analogue experiments, or examination of the geomorphological and geological record. The last of these approaches is limited by the spatial resolution and coverage of satellite data, or to the very limited localities where rovers or landers have been deployed (e.g., Viking, Mars Exploration Rovers). There have been no observed releases of water on to the surface of Mars. Therefore, a series of experiments should add insight to our understanding of this phenomenon. The experiments are intended to be primarily a study of the temperature-pressure relationships and how they affect phase changes in both pure wate

M3 - Conference paper

T2 - 39th Lunar and Planetary Science Conference 2008

Y2 - 10 March 2008 through 14 March 2008

ER -