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Earth-like planets in the habitable zone of low-mass stars undergo strong tidal effects that modify their spin states. These planets are expected to host dense atmospheres that can also play an important role in the spin evolution. On one…

地球与行星天体物理 · 物理学 2024-10-02 E. F. S. Valente , A. C. M. Correia , P. Auclair-Desrotour , M. Farhat , J. Laskar

With improvements in exoplanet detection techniques, the number of multiple planet systems discovered is increasing, while the detection of potentially habitable Earth-mass planets remains complicated and thus requires new search…

地球与行星天体物理 · 物理学 2014-02-13 E. Thilliez , L. Jouvin , S. T. Maddison , J. Horner

Exoplanet habitability is traditionally assessed by comparing a planet's semi-major axis to the location of its host star's "habitable zone," the shell around a star for which Earth-like planets can possess liquid surface water. The Kepler…

地球与行星天体物理 · 物理学 2015-10-01 Rory Barnes , Victoria S. Meadows , Nicole Evans

The ongoing discoveries of extrasolar planets are unveiling a wide range of terrestrial mass (size) planets around their host stars. In this letter, we present estimates of habitable zones (HZs) around stars with stellar effective…

As a contribution to the study of the habitability of extrasolar planets, we implemented a 1-D Energy Balance Model (EBM), the simplest seasonal model of planetary climate, with new prescriptions for most physical quantities. Here we apply…

地球与行星天体物理 · 物理学 2015-06-15 Giovanni Vladilo , Giuseppe Murante , Laura Silva , Antonello Provenzale , Gaia Ferri , Gregorio Ragazzini

Several concepts have been brought forward to determine where terrestrial planets are likely to remain habitable in multi-stellar environments. Isophote-based habitable zones, for instance, rely on insolation geometry to predict…

地球与行星天体物理 · 物理学 2020-09-07 Siegfried Eggl , Nikolaos Georgakarakos , Elke Pilat-Lohinger

We report the detection of GJ 832c, a super-Earth orbiting near the inner edge of the habitable zone of GJ 832, an M dwarf previously known to host a Jupiter analog in a nearly-circular 9.4-year orbit. The combination of precise…

Astronomers have always wanted to know whether there are other planets around other stars that support life like our Earth. The search for life elsewhere has led us to new findings of extreme planetary conditions that humans were unaware…

地球与行星天体物理 · 物理学 2024-01-15 Sattik Bhaumik , Geetanjali Sethi

Given the considerable percentage of stars that are members of binaries or stellar multiples in the Solar neighborhood, it is expected that many of these binaries host planets, possibly even habitable ones. The discovery of a terrestrial…

地球与行星天体物理 · 物理学 2015-06-12 Siegfried Eggl , Nader Haghighipour , Elke Pilat-Lohinger

We derive fitting formulae for the quick determination of the existence of S-type and P-type habitable zones in binary systems. Based on previous work, we consider the limits of the climatological habitable zone in binary systems (which…

地球与行星天体物理 · 物理学 2017-10-11 Zhaopeng Wang , Manfred Cuntz

The notion of a Galactic Habitable Zone (GHZ), or regions of the Milky Way galaxy that preferentially maintain the conditions to sustain complex life, has recently gained attention due to the detection of numerous exoplanets and advances…

地球与行星天体物理 · 物理学 2018-02-22 Michael G. Gowanlock , Ian S. Morrison

We investigate the possibility of habitable Trojan planets in the HD 23079 star-planet system. This system consists of a solar-type star and a Jupiter-type planet, which orbits the star near the outer edge of the stellar habitable zone in…

太阳与恒星天体物理 · 物理学 2015-05-27 J. Eberle , M. Cuntz , B. Quarles , Z. E. Musielak

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,…

地球与行星天体物理 · 物理学 2017-04-26 Vera Dobos

We propose the concept of a "Galactic Habitable Zone" (GHZ). Analogous to the Circumstellar Habitable Zone (CHZ), the GHZ is that region in the Milky Way where an Earth-like planet can retain liquid water on its surface and provide a…

天体物理学 · 物理学 2008-11-26 Guillermo Gonzalez , Donald Brownlee , Peter Ward

The Habitable Zone (HZ) is defined by the possibility of sustaining liquid water on a planetary surface. In the Solar System, the HZ for a conservative climate model extends approximately between the orbits of Earth and Mars. We elaborate…

地球与行星天体物理 · 物理学 2025-10-02 Amri Wandel

Kepler-452b is currently the best example of an Earth-size planet in the habitable zone of a sun-like star, a type of planet whose number of detections is expected to increase in the future. Searching for biosignatures in the supposedly…

地球与行星天体物理 · 物理学 2017-07-26 Laura Silva , Giovanni Vladilo , Giuseppe Murante , Antonello Provenzale

The aim of this paper is to underline conditions necessary for the emergence and development of life. They are placed at local planetary scale, at Galactic scale and within the cosmological evolution, as pointed out by the Anthropic…

地球与行星天体物理 · 物理学 2019-12-04 Luigi Secco , Marco Fecchio , Francesco Marzari

Definition of habitability depends on the organisms under consideration. One way to determine habitability of some environment is to compare its certain parameters to environments where extremophilic micro-organisms thrive on Earth. We can…

科普物理 · 物理学 2013-11-28 Pauli Erik Laine

Studying the habitability, internal structure and composition of exoplanets is crucial for understanding their potential to sustain life beyond our solar system. Characterizing planetary structures and atmospheric evolution provides…

地球与行星天体物理 · 物理学 2025-07-08 Sushmita Deb , Kaushal Sharma , Samrat Biswas , Biman Jyoti Medhi

The concept of the Circumstellar Habitable Zone has served the scientific community well for some decades. It slips easily off the tongue, and it would be hard to replace. Recently, however, several workers have postulated types of…

地球与行星天体物理 · 物理学 2009-12-15 Martin J. Heath , Laurance R. Doyle