Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Cedric Gillmann"'
Publikováno v:
Space: Science & Technology, Vol 4 (2024)
No matter how fascinating and exotic other terrestrial planets are revealed to be, nothing generates more excitement than announcements regarding their habitability. From the observation of Mars to present-day efforts toward Venus and the characteriz
Externí odkaz:
https://doaj.org/article/fcc55d151c4a49868ebb8b09802a4f29
Baltis Vallis (BV) is a 6,800-km long lava channel on Venus with a present-day uphill flow direction. The apparently uphill flow must be a consequence of deformation changing the topography after flow emplacement. The topography of BV thus retains a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1053d4b85bc594dd482629743a14d025
https://doi.org/10.5194/egusphere-egu23-9783
https://doi.org/10.5194/egusphere-egu23-9783
Autor:
M. J. Way, Colby Ostberg, Bradford J. Foley, Cedric Gillmann, Dennis Höning, Helmut Lammer, Joseph O’Rourke, Moa Persson, Ana-Catalina Plesa, Arnaud Salvador, Manuel Scherf, Matthew Weller
Publikováno v:
Way, M J, Ostberg, C, Foley, B J, Gillmann, C, Höning, D, Lammer, H, O’Rourke, J, Persson, M, Plesa, A C, Salvador, A, Scherf, M & Weller, M 2023, ' Synergies Between Venus & Exoplanetary Observations : Venus and Its Extrasolar Siblings ', Space Science Reviews, vol. 219, no. 1, 13 . https://doi.org/10.1007/s11214-023-00953-3
Here we examine how our knowledge of present day Venus can inform terrestrial exoplanetary science and how exoplanetary science can inform our study of Venus. In a superficial way the contrasts in knowledge appear stark. We have been looking at Venus
Autor:
Michael Way, Colby Ostberg, Bradford J Foley, Cedric Gillmann, Dennis Höning, Helmut Lammer, Joseph O'Rourke, Moa Persson, Ana-Catalina Plesa, Arnaud Salvador, Manuel Scherf, Matthew Weller
In this chapter we examine how our knowledge of present day Venus can inform terrestrial exoplanetary science and how exoplanetary science can inform our study of Venus. In a superficial way the contrasts in knowledge appear stark. We have been looki
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::40d18b1006ed14d2128918837f7bbed6
Autor:
Frances Westall, Dennis Höning, Guillaume Avice, Diana Gentry, Taras Gerya, Cedric Gillmann, Noam Izenberg, Michael Way, Colin Wilson
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a2f736b0722ab12b521704ccca4f8715
https://doi.org/10.1002/essoar.10512790.1
https://doi.org/10.1002/essoar.10512790.1
Autor:
Cedric Gillmann, M. J. Way, Guillaume Avice, Doris Breuer, Gregor J. Golabek, Dennis Höning, Joshua Krissansen-Totton, Helmut Lammer, Joseph G. O’Rourke, Moa Persson, Ana-Catalina Plesa, Arnaud Salvador, Manuel Scherf, Mikhail Y. Zolotov
Publikováno v:
Gillmann, C, Way, M J, Avice, G, Breuer, D, Golabek, G J, Höning, D, Krissansen-Totton, J, Lammer, H, O’Rourke, J G, Persson, M, Plesa, A C, Salvador, A, Scherf, M & Zolotov, M Y 2022, ' The Long-Term Evolution of the Atmosphere of Venus: Processes and Feedback Mechanisms : Interior-Exterior Exchanges ', Space Science Reviews, vol. 218, no. 7, 56, pp. 1-71 . https://doi.org/10.1007/s11214-022-00924-0
This work reviews the long-term evolution of the atmosphere of Venus, and modulation of its composition by interior/exterior cycling. The formation and evolution of Venus’s atmosphere, leading to contemporary surface conditions, remain hotly debate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5bbb9466f19ad04c180770c891063fc
https://hdl.handle.net/1871.1/2774d540-4103-4523-a749-350c2dde73c8
https://hdl.handle.net/1871.1/2774d540-4103-4523-a749-350c2dde73c8
Publikováno v:
Earth and Planetary Science Letters. 502:46-56
Venus lacks an internally generated magnetic field today. Whether one existed in the past is unknown, but critical to atmospheric evolution and potential habitability. Canonical models assume the core of Venus is cooling too slowly for convection and
Autor:
Vinciane Debaille, Cedric Gillmann, Maria Schönbächler, Sean N. Raymond, Paul J. Tackley, Gregor J. Golabek, Véronique Dehant
Terrestrial planets in the Solar system generally lack surface liquid water. Earth is at odd with this observation and with the idea of the giant Moon-forming impact that should have vaporized any pre-existing water, leaving behind a dry Earth. Given
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7f72c6e6c061e857a0deb3bc4dd9bd88
https://doi.org/10.5194/egusphere-egu21-5920
https://doi.org/10.5194/egusphere-egu21-5920
Venus shares some striking similarities with Earth; at the same time, it exhibits characteristics that are widely different from that of our own planet. Indeed, it is an example of an active planet that may have followed a radically different evoluti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::48d513ccbdfc8ffe0df41d26b81c0cc4
https://doi.org/10.5194/egusphere-egu2020-5164
https://doi.org/10.5194/egusphere-egu2020-5164
Autor:
Cedric Gillmann, Vinciane Debaille, Gregor J. Golabek, Véronique Dehant, M. Schönbächler, Sean N. Raymond, Paul J. Tackley
Publikováno v:
Nature Geoscience
Nature Geoscience, Nature Publishing Group, 2020, 13 (4), pp.265-269. ⟨10.1038/s41561-020-0561-x⟩
Nature Geoscience, 13 (4
Nature Geoscience, Nature Publishing Group, 2020, 13 (4), pp.265-269. ⟨10.1038/s41561-020-0561-x⟩
Nature Geoscience, 13 (4
It remains contentious whether the meteoritic material delivered to the terrestrial planets after the end of core formation was rich or poor in water and other volatiles. As Venus’s atmosphere has probably experienced less volatile recycling over i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc348431dfc61a67383ac8e333621c4d