Zobrazeno 1 - 10
of 173
pro vyhledávání: '"von Paris, P."'
Autor:
Gebauer, S., Grenfell, J. L., Stock, J. W., Lehmann, R., Godolt, M., von Paris, P., Rauer, H.
Publikováno v:
published in Astrobiology, Volume 17, Issue 1, 2017, pp.27-54
Understanding the evolution of Earth and potentially habitable Earth-like worlds is essential to fathom our origin in the Universe. The search for Earth-like planets in the habitable zone and investigation of their atmospheres with climate and photoc
Externí odkaz:
http://arxiv.org/abs/1807.06844
Autor:
Chiavassa, A., Caldas, A., Selsis, F., Leconte, J., Von Paris, P., Bordé, P., Magic, Z., Collet, R., Asplund, M.
Publikováno v:
A&A 597, A94 (2017)
Stellar activity and convection-related surface structures might cause bias in planet detection and characterization that use these transits. Surface convection simulations help to quantify the granulation signal. We used realistic three-dimensional
Externí odkaz:
http://arxiv.org/abs/1609.08966
Clouds have been shown to be present in many exoplanetary atmospheres. Cloud formation modeling predicts considerable inhomogeneities of cloud cover, consistent with optical phase curve observations. However, optical phase curves cannot resolve some
Externí odkaz:
http://arxiv.org/abs/1602.04362
Publikováno v:
A&A 587, A149 (2016)
Basic atmospheric properties such as albedo and heat redistribution between day and nightside have been inferred for a number of planets using observations of secondary eclipses and thermal phase curves. Optical phase curves have not yet been used to
Externí odkaz:
http://arxiv.org/abs/1512.04908
Publikováno v:
PSS, 98, 66-76 2014
We find that variations in the UV emissions of cool M-dwarf stars have a potentially large impact upon atmospheric biosignatures in simulations of Earth-like exoplanets i.e. planets with Earths development, and biomass and a molecular nitrogen-oxygen
Externí odkaz:
http://arxiv.org/abs/1507.02823
Autor:
Kitzmann, D., Alibert, Y., Godolt, M., Grenfell, J. L., Heng, K., Patzer, A. B. C., Rauer, H., Stracke, B., von Paris, P.
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:
http://arxiv.org/abs/1507.01727
Autor:
Grenfell, John Lee, Grriessmeier, Jean-Mathias, von Paris, Philip, Patzer, Beate, Lammer, Helmut, Stracke, Barbara, Gebauer, Stefanie, Schreier, Franz, Rauer, Heike
Understanding whether M-dwarf stars may host habitable planets with Earth-like atmospheres and biospheres is a major goal in exoplanet research. If such planets exist, the question remains as to whether they could be identified via spectral signature
Externí odkaz:
http://arxiv.org/abs/1506.06508
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:
http://arxiv.org/abs/1505.07713
Autor:
Godolt, M., Grenfell, J. L., Hamann-Reinus, A., Kitzmann, D., Kunze, M., Langematz, U., von Paris, P., Patzer, A. B. C., Rauer, H., Stracke, B.
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:
http://arxiv.org/abs/1504.01558
Autor:
von Paris, P., Petau, A., Grenfell, J. L., Hauber, E., Breuer, D., Jaumann, R., Rauer, H., Tirsch, D.
We compare estimates of atmospheric precipitation during the Martian Noachian-Hesperian boundary 3.8 Gyr ago as calculated in a radiative-convective column model of the atmosphere with runoff values estimated from a geomorphological analysis of dendr
Externí odkaz:
http://arxiv.org/abs/1411.5144