Zobrazeno 1 - 10 of 171 pro vyhledávání: '"M. Godolt"'
1
Distinguishing between Wet and Dry Atmospheres of TRAPPIST-1 e and f
Autor: Fabian Wunderlich, A. Sánchez-López, Manuel López-Puertas, M Godolt, Peter Schneider, Franz Schreier, Heike Rauer, David J. Wilson, John Lee Grenfell, Markus Scheucher
Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
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The Astrophysical Journal, 901(2), 126
The nearby TRAPPIST-1 planetary system is an exciting target for characterizing the atmospheres of terrestrial planets. The planets e, f, and g lie in the circumstellar habitable zone and could sustain liquid water on their surfaces. During the exten
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14136e4b61755917e4b197361defc414
http://hdl.handle.net/10261/221609
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2
Searching for Atmospheric Bioindicators in Planets around the Two Nearby Stars, Proxima Centauri and Epsilon Eridani-Test Cases for Retrieval of Atmospheric Gases with Infrared Spectroscopy
Autor: Denis Defrere, Feng Tian, A. García Muñoz, Heike Rauer, A. Léger, M Godolt, John Lee Grenfell
Publikováno v: Astrobiology. 19(6)
We tested the ability of thermal infrared spectroscopy to retrieve assumed atmospheric compositions for different types of planets orbiting Proxima Centauri and Epsilon Eridani. Six cases are considered, covering a range of atmospheric compositions a
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b70c84534980467f2a1c72f7d6c64a8a
https://pubmed.ncbi.nlm.nih.gov/30985192
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3
New Insights into Cosmic Ray induced Biosignature Chemistry in Earth-like Atmospheres
Autor: Franz Schreier, Markus Scheucher, John Lee Grenfell, M. Godolt, Heike Rauer, Fabian Wunderlich
With the recent discoveries of terrestrial planets around active M-dwarfs, destruction processes masking the possible presence of life are receiving increased attention in the exoplanet community. We investigate potential biosignatures of planets hav
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e32891e13de4949bb26071560a814d21
http://arxiv.org/abs/1808.02347
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4
The habitability of a stagnant-lid Earth
Autor: Nicola Tosi, Athanasia Nikolaou, John Lee Grenfell, B. Stracke, Tilman Spohn, Doris Breuer, M. Godolt, Thomas Ruedas, Dennis Höning, Ana-Catalina Plesa
Plate tectonics is a fundamental component for the habitability of the Earth. Yet whether it is a recurrent feature of terrestrial bodies orbiting other stars or unique to the Earth is unknown. The stagnant lid may rather be the most common tectonic
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59e0cf3b7f7026bcc7b28ee345123700
https://elib.dlr.de/116458/
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6
Fahndung nach der zweiten Erde
Autor: Ruth Titz-Weider, John Lee Grenfell, M. Godolt, Stefanie Gebauer
Publikováno v: Physik in unserer Zeit. 44:64-71
Erdahnliche Planeten oder Supererden, bei denen man Transit- und Bedeckungsereignisse beobachten kann, sind fur spektroskopische Untersuchungen der Atmosphare geeignete Objekte. Es ist aber keineswegs eindeutig zu sagem, welche Bestandteile der Atmos
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::591040e16aa04aff4f304623909b2b82
https://doi.org/10.1002/piuz.201301320
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7
Assessing the habitability of planets with Earth-like atmospheres with 1D and 3D climate modeling
Autor: John Lee Grenfell, Markus Kunze, M. Godolt, D. Kitzmann, Ulrike Langematz, Heike Rauer, B. Stracke, A. B. C. Patzer
The habitable zone (HZ) describes the range of orbital distances around a star where the existence of liquid water on the surface of an Earth-like planet is in principle possible. While 3D climate studies can calculate the water vapor, ice albedo, an
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dbfe9563bff63269748c2c4d2ae8206e
http://arxiv.org/abs/1605.08231
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8
The unstable CO2 feedback cycle on ocean planets
Autor: John Lee Grenfell, Heike Rauer, Barbara Stracke, M. Godolt, Kevin Heng, P. von Paris, Daniel Kitzmann, A. B. C. Patzer, Yann Alibert
Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 452 (4), pp.3752-3758. ⟨10.1093/mnras/stv1487⟩
Monthly Notices of the Royal Astronomical Society, 2015, 452 (4), pp.3752-3758. ⟨10.1093/mnras/stv1487⟩
American Astronomical Society, ESS meeting #3, #500.04. BAAS volume 47 #6, November 2015. Held in HawaÏ 29-11 au 04-12-2015
American Astronomical Society, ESS meeting #3, #500.04. BAAS volume 47 #6, November 2015. Held in HawaÏ 29-11 au 04-12-2015, Nov 2015, HawaÏ United States
MNRAS
Kitzmann, D.; Alibert, Yann; Godolt, M.; Grenfell, J. L.; Heng, K.; Patzer, A. B. C.; Rauer, H.; Stracke, B.; von Paris, P. (2015). The unstable CO2 feedback cycle on ocean planets. Monthly notices of the Royal Astronomical Society, 452(4), pp. 3752-3758. Oxford University Press 10.1093/mnras/stv1487
Ocean planets are volatile rich planets, not present in our Solar System, which are thought to be dominated by deep, global oceans. This results in the formation of high-pressure water ice, separating the planetary crust from the liquid ocean and, th
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26527f23a364c07dbb6a1bb9554f537d
https://hal.archives-ouvertes.fr/hal-01174412
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9
Effect of O3 on the atmospheric temperature structure of early Mars
Autor: Heike Rauer, John Lee Grenfell, Barbara Stracke, P. von Paris, M. Godolt, Franck Selsis
Publikováno v: Icarus
Icarus, Elsevier, 2015, 257, pp.406-416. ⟨10.1016/j.icarus.2015.05.028⟩
Ozone is an important radiative trace gas in the Earth's atmosphere. The presence of ozone can significantly influence the thermal structure of an atmosphere, and by this e.g. cloud formation. Photochemical studies suggest that ozone can form in carb
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::acfa2444ef28b26ca0dc351ed294311d
http://arxiv.org/abs/1505.07713
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10
3D climate modeling of Earth-like extrasolar planets orbiting different types of host stars
Autor: Markus Kunze, A. B. C. Patzer, P. von Paris, D Kitzmann, Heike Rauer, John Lee Grenfell, A Hamann-Reinus, Ulrike Langematz, M. Godolt, Barbara Stracke
Publikováno v: Planetary and Space Science
Planetary and Space Science, Elsevier, 2015, 111, pp.62-76. ⟨10.1016/j.pss.2015.03.010⟩
The potential habitability of a terrestrial planet is usually defined by the possible existence of liquid water on its surface. The potential presence of liquid water depends on many factors such as, most importantly, surface temperatures. The proper
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2d20711e90bffaec9cf70a37021a402
https://doi.org/10.1016/j.pss.2015.03.010
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