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Detecting massive satellites of extrasolar planets has now become feasible, which led naturally to questions about their habitability. In a previous study we presented constraints on the habitability of moons from stellar and planetary…

地球与行星天体物理 · 物理学 2015-06-11 René Heller

Detections of massive extrasolar moons are shown feasible with the Kepler space telescope. Kepler's findings of about 50 exoplanets in the stellar habitable zone naturally make us wonder about the habitability of their hypothetical moons.…

地球与行星天体物理 · 物理学 2015-06-11 René Heller , Rory Barnes

Moons orbiting extrasolar planets are the next class of object to be observed and characterized for possible habitability. Like the host-planets to their host-star, exomoons have a limiting radius at which they may be gravitationally bound,…

地球与行星天体物理 · 物理学 2015-06-16 Natalie R. Hinkel , Stephen R. Kane

We discuss the possibility of screening the atmosphere of exomoons for habitability. We concentrate on Earth-like satellites of extrasolar giant planets (EGP) which orbit in the Habitable Zone of their host stars. The detectability of…

地球与行星天体物理 · 物理学 2015-05-14 L. Kaltenegger

Exomoons may play an important role in determining the habitability of worlds outside of our solar system. They can stabilize conditions, alter the climate by breaking tidal locking with the parent star, drive tidal heating, and perhaps…

地球与行星天体物理 · 物理学 2020-10-14 Armen Tokadjian , Anthony L. Piro

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

The habitable zone for exomoons with Earth-like properties is a non-trivial manifold, compared to that of Earth-like exoplanets. The presence of tidal heating, eclipses and planetary illumination in the exomoon energy budget combine to…

地球与行星天体物理 · 物理学 2016-02-17 Duncan Forgan , Vera Dobos

With most planets and planetary candidates detected in the stellar habitable zone (HZ) being super-Earths and gas giants, rather than Earth-like planets, we naturally wonder if their moons could be habitable. The first detection of such an…

地球与行星天体物理 · 物理学 2016-03-27 René Heller , Jorge I. Zuluaga

The exquisite photometric precision of the Kepler space telescope now puts the detection of extrasolar moons at the horizon. Here, we firstly review observational and analytical techniques that have recently been proposed to find exomoons.…

地球与行星天体物理 · 物理学 2015-06-12 René Heller , Rory Barnes

We investigate the habitability of hypothethical moons orbiting known exoplanets. This study focuses on big, rocky exomoons that are capable of maintaining a significant atmosphere. To determine their habitability, we calculate the incident…

地球与行星天体物理 · 物理学 2022-06-08 Vera Dobos , András Haris , Inga E. E. Kamp , Floris F. S. van der Tak

Discoveries of extrasolar planets in the habitable zone (HZ) of their parent star lead to questions about the habitability of massive moons orbiting planets in the HZ. Around low-mass stars, the HZ is much closer to the star than for…

地球与行星天体物理 · 物理学 2017-07-25 Rhett R. Zollinger , John C. Armstrong , René Heller

The habitability of exoplanets can be strongly influenced by the presence of an exomoon, and in some cases the exomoon itself could be a possible place for life to develop. For moons outside of the habitable zone, significant tidal heating…

地球与行星天体物理 · 物理学 2023-03-28 Armen Tokadjian , Anthony L. Piro

The diversity and quantity of moons in the Solar System suggest a manifold population of natural satellites exist around extrasolar planets. Of peculiar interest from an astrobiological perspective, the number of sizable moons in the…

Recent studies have shown that large exomoons can form in the accretion disks around super-Jovian extrasolar planets. These planets are abundant at about 1 AU from Sun-like stars, which makes their putative moons interesting for studies of…

地球与行星天体物理 · 物理学 2018-07-04 Jacob Haqq-Misra , René Heller

With the detection of extrasolar moons (exomoons) on the horizon, it is important to consider their potential for habitability. If we consider the circumstellar Habitable Zone (HZ, often described in terms of planet semi-major axis and…

地球与行星天体物理 · 物理学 2015-06-15 Duncan Forgan , David Kipping

With dozens of Jovian and super-Jovian exoplanets known to orbit their host stars in or near the stellar habitable zones, it has recently been suggested that moons the size of Mars could offer abundant surface habitats beyond the solar…

地球与行星天体物理 · 物理学 2017-05-10 Vera Dobos , René Heller , Edwin L. Turner

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 satellites of extrasolar planets (exomoons) have been recently proposed as astrobiological targets. Since giant planets in the habitable zone are thought to have migrated there, it is possible that they may have captured a former…

地球与行星天体物理 · 物理学 2012-06-27 Simon B. Porter , William M. Grundy

The search for life outside of the Solar System should not be restricted to exclusively planetary bodies; large moons of extrasolar planets may also be common habitable environments throughout the Galaxy. Extrasolar moons, or exomoons, may…

地球与行星天体物理 · 物理学 2009-11-30 David M. Kipping , Stephen J. Fossey , Giammarco Campanella , Jean Schneider , Giovanna Tinetti

Exoplanet discoveries have motivated numerous efforts to find unseen populations of exomoons, yet they have been unsuccessful. A plausible explanation is that most discovered planets are located on close-in orbits, which would make their…

地球与行星天体物理 · 物理学 2020-01-08 Mario Sucerquia , Vanesa Ramírez , Jaime A. Alvarado-Montes , Jorge I. Zuluaga
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