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Approximately two-thirds of the Earth, the only known inhabited planet, is covered in ocean. Why not 0.01% or 99.99%? It has been previously suggested that this may represent a certain degree of fine-tuning, and thus perhaps observers are…

Earth and Planetary Astrophysics · Physics 2026-02-03 David Kipping

One of the unique features associated with the Earth is that the fraction of its surface covered by land is comparable to that spanned by its oceans and other water bodies. Here, we investigate how extraterrestrial biospheres depend on the…

Earth and Planetary Astrophysics · Physics 2019-01-04 Manasvi Lingam , Abraham Loeb

Large terrestrial planets are expected to have muted topography and deep oceans, implying that most super-Earths should be entirely covered in water, so-called waterworlds. This is important because waterworlds lack a silicate weathering…

Earth and Planetary Astrophysics · Physics 2014-01-06 Nicolas B. Cowan , Dorian S. Abbot

Earth has a unique surface character among Solar System worlds. Not only does it harbor liquid water, but also large continents. An exoplanet with a similar appearance would remind us of home, but it is not obvious whether such a planet is…

Earth and Planetary Astrophysics · Physics 2015-11-20 Nicolas B. Cowan

In the past 15 years, astronomers have revealed that a significant fraction of the stars should harbor planets and that it is likely that terrestrial planets are abundant in our galaxy. Among these planets, how many are habitable, i.e.…

Earth and Planetary Astrophysics · Physics 2013-05-09 Francois Forget

It is likely that unambiguous habitable zone terrestrial planets of unknown water content will soon be discovered. Water content helps determine surface land fraction, which influences planetary weathering behavior. This is important…

Earth and Planetary Astrophysics · Physics 2015-06-11 Dorian S. Abbot , Nicolas B. Cowan , Fred J. Ciesla

A balanced ratio of ocean to land is believed to be essential for an Earth-like biosphere and one may conjecture that plate-tectonics planets should be similar in geological properties. After all, the volume of continental crust evolves…

Earth and Planetary Astrophysics · Physics 2023-04-12 Dennis Höning , Tilman Spohn

Water and land surfaces on a planet interact with gases in the atmosphere and with radiation from the star. These interactions define the environments that prevail on the planet, some of which may be more amenable to prebiotic chemistry,…

Earth-like planets are expected to provide the greatest opportunity for the detection of life beyond the Solar System. However our planet cannot be considered a fair sample, especially if intelligent life exists elsewhere. Just as a…

Popular Physics · Physics 2016-03-29 Fergus Simpson

The habitable fraction of a planet's surface is important for the detectability of surface biosignatures. The extent and distribution of habitable areas is influenced by external parameters that control the planet's climate, atmospheric…

Earth and Planetary Astrophysics · Physics 2020-01-08 Anthony D. Del Genio , M. J. Way , Nancy Y. Kiang , Igor Aleinov , Michael J. Puma , Benjamin Cook

Habitability is a measure of an environment's potential to support life, and a habitable exoplanet supports liquid water on its surface. However, a planet's success in maintaining liquid water on its surface is the end result of a complex…

Earth and Planetary Astrophysics · Physics 2021-12-15 Ravi kumar Kopparapu , Eric T. Wolf , Victoria S. Meadows

Recent detections of potentially habitable exoplanets around sunlike stars demand increased exploration of the physical conditions that can sustain life, by whatever methods available. Insight into these conditions can be gained by…

Earth and Planetary Astrophysics · Physics 2023-02-27 McCullen Sandora , Vladimir Airapetian , Luke Barnes , Geraint F. Lewis

Liquid water is one of the most important materials affecting the climate and habitability of a terrestrial planet. Liquid water vaporizes entirely when planets receive insolation above a certain value, which is called the runaway…

Earth and Planetary Astrophysics · Physics 2018-03-28 T. Kodama , A. Nitta , H. Genda , Y. Takao , R. O'ishi , A. Abe-Ouchi , Y. Abe

Super-Earths are highly irradiated, small planets with bulk densities approximately consistent with Earth. We construct combined interior-atmosphere models of super-Earths that trace the partitioning of water throughout a planet, including…

Earth and Planetary Astrophysics · Physics 2024-12-17 James G. Rogers , Caroline Dorn , Vivasvaan Aditya Raj , Hilke E. Schlichting , Edward D. Young

Conventionally, a habitable planet is one that can support liquid water on its surface. Habitability depends on temperature, which is set by insolation and the greenhouse effect, due mainly to CO2 and water vapor. The CO2 level is increased…

Earth and Planetary Astrophysics · Physics 2020-06-24 John Chambers

According to the standard liquid-water definition, the Earth is only partially habitable. We reconsider planetary habitability in the framework of energy-balance models, the simplest seasonal models in physical climatology, to assess the…

Astrophysics · Physics 2009-11-13 David S. Spiegel , Kristen Menou , Caleb A. Scharf

The climates of terrestrial planets with a small amount of water on their surface, called land planets, are significantly different from the climates of planets having a large amount of surface water. Land planets have a higher runaway…

Earth and Planetary Astrophysics · Physics 2021-11-29 T. Kodama , H. Genda , J. Leconte , A. Abe-Ouchi

How good is our universe at making habitable planets? The answer to this depends on which factors are important for life: Does a planet need to be Earth mass? Does it need to be inside the temperate zone? are systems with hot Jupiters…

Earth and Planetary Astrophysics · Physics 2019-08-15 McCullen Sandora

The water content of magma oceans is widely accepted as a key factor that determines whether a terrestrial planet is habitable. Water ocean mass is determined as a result not only of water delivery and loss, but also of water partitioning…

Earth and Planetary Astrophysics · Physics 2018-05-16 Masahiro Ikoma , Linda Elkins-Tanton , Keiko Hamano , Jenny Suckale

Super-Earths orbiting M-dwarf stars may be the most common habitable planets in the Universe. However, their habitability is threatened by intense irradiation from their host stars, which drives the escape of water to space and can lead to…

Earth and Planetary Astrophysics · Physics 2024-08-28 Keavin Moore , Benjamin David , Albert Yian Zhang , Nicolas B. Cowan
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