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020 a| 9781786203625 (ebook) :c| No price;

035 a| (Sirsi) a5335913;

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050 4 a| QB643.G46;

082 04 a| 559.9232| 23;

111 2 a| International Workshop on Martian Gulliesn| (2nd :d| 2015 :c| London, England),j| creator.=| ^A1404812;

245 10 a| Martian gullies and their Earth analogues /c| S.J. Conway, J.L. Carrivick, P.A. Carling, T. de Haas, T.N. Harrison.;

264 1 a| London :b| Geological Society of London,c| 2019.;

300 a| 1 online resource (vi, 434 pages) :b| illustrations (black and white, and colour), maps (black and white, and colour).;

336 a| textb| txt2| rdacontent;

336 a| still imageb| sti2| rdacontent;

336 a| cartographic imageb| cri2| rdacontent;

337 a| computerb| c2| rdamedia;

338 a| online resourceb| cr2| rdacarrier;

490 1 a| Geological Society special publication ;v| no. 467;

500 a| Previously issued in print in 2019. Digital resource published 2019.;

500 a| Proceedings from the Second International Workshop on Martian Gullies held at the Geological Society, London, 2015.;

504 a| Includes bibliographical references and index.;

520 8 a| Gullies on Mars resemble terrestrial gullies involved in the transport of abundant material down steep slopes by liquid water. However, liquid water should not be stable at the Martian surface. The articles in this volume present the two main opposing theories for Martian gully formation: climate-driven melting of surficial water-ice deposits and seasonal dry-ice sublimation. The evidence presented ranges from remote-sensing observations, to experimental simulations, to comparison with Earth analogues. The opposing hypotheses imply either that Mars has been unusually wet in the last few million years or that it has remained a cold dry desert - both with profound implications for understanding the water budget of Mars and its habitability.;

521 a| Specialized.;

588 a| Description based on online resource; title from home page (viewed on May 29, 2019).;

650 0 a| River channelsv| Congresses.=| ^A20652;

651 0 a| Mars (Planet)x| Geologyv| Congresses.=| ^A79502;

700 1 a| Conway, S. J.q| (Susan J.),e| editor.=| ^A1404813;

700 1 a| Carrivick, Jonathan,e| editor.=| ^A1322709;

700 1 a| Carling, Paul,e| editor.=| ^A243608;

700 1 a| De Haas, T.,e| editor.=| ^A711405;

700 1 a| Harrison, T. N.q| (Tanya N.),e| editor.=| ^A1404814;

710 2 a| Geological Society of Londone| host institution.=| ^A53543;

776 08 i| Print version :z| 9781786203601;

830 0 a| Geological Society special publication ;v| no. 467.=| ^A465527;

856 40 3| GeoScienceWorldu| https://go.openathens.net/redirector/ecu.edu?url=https://geoscienceworld.org/books/book/2151;

949 a| Click on web addressw| asish| joyner151o| jjlm;

596 a| 1;

998 a| 5335913;

999 a| CLICK ON WEB ADDRESSw| ASISc| 1i| 5335913-1001l| JNETm| JOYNERr| Ys| Yt| JNEGSWBKu| 7/9/2020x| EBOOKz| JERESOURCEo| .STAFF. jjlm;

Martian gullies and their Earth analogues / S.J. Conway, J.L. Carrivick, P.A. Carling, T. de Haas, T.N. Harrison.

Author/creator	International Workshop on Martian Gullies
Format	Electronic
Publication	London : Geological Society of London, 2019.
Description	1 online resource (vi, 434 pages) : illustrations (black and white, and colour), maps (black and white, and colour).
Supplemental Content	GeoScienceWorld
Subjects	River channels--Congresses. Mars (Planet)--Geology. --Congresses. Mars (Planet)--Geology. --Earth analogs. --Congresses.

Other author/creator	Conway, S. J. (Susan J.), editor.
Other author/creator	Carrivick, Jonathan, editor.
Other author/creator	Carling, Paul, editor.
Other author/creator	De Haas, T., editor.
Other author/creator	Harrison, T. N. (Tanya N.), editor.
Other author/creator	Geological Society of London host institution.
Series	Geological Society special publication ; no. 467 Geological Society special publication ; no. 467. ^A465527
Summary	Gullies on Mars resemble terrestrial gullies involved in the transport of abundant material down steep slopes by liquid water. However, liquid water should not be stable at the Martian surface. The articles in this volume present the two main opposing theories for Martian gully formation: climate-driven melting of surficial water-ice deposits and seasonal dry-ice sublimation. The evidence presented ranges from remote-sensing observations, to experimental simulations, to comparison with Earth analogues. The opposing hypotheses imply either that Mars has been unusually wet in the last few million years or that it has remained a cold dry desert - both with profound implications for understanding the water budget of Mars and its habitability.
General note	Previously issued in print in 2019. Digital resource published 2019.
General note	Proceedings from the Second International Workshop on Martian Gullies held at the Geological Society, London, 2015.
Bibliography note	Includes bibliographical references and index.
Spec. audience char.	Specialized.
Source of description	Description based on online resource; title from home page (viewed on May 29, 2019).
Issued in other form	Print version : 9781786203601
ISBN	9781786203625 (ebook) :

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Martian gullies and their Earth analogues / S.J. Conway, J.L. Carrivick, P.A. Carling, T. de Haas, T.N. Harrison.

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