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Related papers: On the probability of habitable planets

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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

Habitability is usually defined as the requirement for a terrestrial planet's atmosphere to sustain liquid water. This definition can be complemented by the dynamical requirement that other planets in the system do not gravitationally…

Astrophysics · Physics 2009-11-07 Kristen Menou , Serge Tabachnik

With the discovery of hundreds of exoplanets and a potentially huge number of Earth-like planets waiting to be discovered, the conditions for their habitability have become a focal point in exoplanetary research. The classical picture of…

Earth and Planetary Astrophysics · Physics 2015-06-22 M. Guedel , R. Dvorak , N. Erkaev , J. Kasting , M. Khodachenko , H. Lammer , E. Pilat-Lohinger , H. Rauer , I. Ribas , B. E. Wood

As of late 2025 there are about 70 exoplanets that meet the formal criterion of having equilibrium temperatures allowing the presence of liquid water and about 50 of them orbit M-stars, known for their strong chromospheric activity. Most of…

Instrumentation and Methods for Astrophysics · Physics 2025-12-29 Rebecca Szabó , Valentin D. Ivanov , M. Švanda

A habitable exoplanet is a world that can maintain stable liquid water on its surface. Techniques and approaches to characterizing such worlds are essential, as performing a census of Earth-like planets that may or may not have life will…

Earth and Planetary Astrophysics · Physics 2024-01-22 Tyler D. Robinson

Dozens of habitable zone, approximately earth-sized exoplanets are known today. An emerging frontier of exoplanet studies is identifying which of these habitable zone, small planets are actually habitable (have all necessary conditions for…

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

A habitable zone of a star is defined as a range of orbits within which a rocky planet can support liquid water on its surface. The most intriguing question driving the search for habitable planets is whether they host life. But is the age…

Earth and Planetary Astrophysics · Physics 2016-03-24 M. Safonova , J. Murthy , Yu. A. Shchekinov

It is currently unknown how common life is on exoplanets, or how long planets can remain viable for life. To date, we have a superficial notion of habitability, a necessary first step, but so far lacking an understanding of the detailed…

Our understanding of the processes that are relevant to the formation and maintenance of habitable planetary systems is advancing at a rapid pace, both from observation and theory. The present review focuses on recent research that bears on…

Earth and Planetary Astrophysics · Physics 2014-03-27 Guillermo Gonzalez

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

Understanding the concept of habitability is related to an evolutionary knowledge of the particular planet-in-question. Additional indications so-called "systemic aspects" of the planetary system as a whole governs a particular planet's…

How do habitable environments arise and evolve within the context of their planetary systems? This is one fundamental question, and it can be addressed partly by identifying how planets in habitable zones obtain water. Historically,…

Instrumentation and Methods for Astrophysics · Physics 2025-10-10 Yasuhiro Hasegawa , Courtney Dressing , Ludmila Carone

The ability of a planet to maintain surface water, key to life as we know it, depends on solar and planetary energy. As a star ages, it delivers more energy to a planet. As a planet ages it produces less internal heat, which leads to…

Earth and Planetary Astrophysics · Physics 2021-06-29 Johnny Seales , Adrian Lenardic

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

The aim of my dissertation is to investigate habitability in extra-Solar Systems. Most of the time, only planets are considered as possible places where extraterrestrial life can emerge and evolve, however, their moons could be inhabited,…

Earth and Planetary Astrophysics · Physics 2017-04-26 Vera Dobos

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

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

Two habitable planetary states are proposed: an aqua planet like the Earth and a land planet that has a small amount of water. Land planets keep liquid water under larger solar radiation compared to aqua planets. Water loss may change an…

Earth and Planetary Astrophysics · Physics 2015-10-28 T. Kodama , H. Genda , Y. Abe , K. J. Zahnle

Conventional definitions of habitability require abundant liquid surface water to exist continuously over geologic timescales. Water in each of its thermodynamic phases interacts with solar and thermal radiation and is the cause for strong…

Earth and Planetary Astrophysics · Physics 2017-03-15 Eric T. Wolf , Aomawa L. Shields , Ravi K. Kopparapu , Jacob Haqq-Misra , Owen B. Toon
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