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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.…

Earth and Planetary Astrophysics · Physics 2015-06-11 René Heller , Rory Barnes

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…

Earth and Planetary Astrophysics · Physics 2015-05-14 L. Kaltenegger

The detection of moons orbiting extrasolar planets ("exomoons") has now become feasible. Once they are discovered in the circumstellar habitable zone, questions about their habitability will emerge. Exomoons are likely to be tidally locked…

Earth and Planetary Astrophysics · Physics 2013-10-31 René Heller , Rory Barnes

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…

In this paper we investigate the detectability of a habitable-zone exomoon around various configurations of exoplanetary systems with the Kepler Mission or photometry of approximately equal quality. We calculate both the predicted transit…

Earth and Planetary Astrophysics · Physics 2015-05-13 David M. Kipping , Stephen J. Fossey , Giammarco Campanella

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…

Earth and Planetary Astrophysics · Physics 2009-11-30 David M. Kipping , Stephen J. Fossey , Giammarco Campanella , Jean Schneider , Giovanna Tinetti

Two decades ago, astronomers began detecting planets orbiting stars other than our Sun, so-called exoplanets. Since that time, the rate of detections and the sensitivity to ever-smaller planets has improved dramatically with several…

Earth and Planetary Astrophysics · Physics 2014-05-08 David M. Kipping

Since the discovery of a planet transiting its host star in the year 2000, thousands of additional exoplanets and exoplanet candidates have been detected, mostly by NASA's Kepler space telescope. Some of them are almost as small as the…

Earth and Planetary Astrophysics · Physics 2019-02-06 René Heller

Two decades ago, empirical evidence concerning the existence and frequency of planets around stars, other than our own, was absent. Since this time, the detection of extrasolar planets from Jupiter-sized to most recently Earth-sized worlds…

Earth and Planetary Astrophysics · Physics 2015-06-03 David M. Kipping , Gáspár Á. Bakos , Lars A. Buchhave , David Nesvorny , Allan Schmitt

Satellite formation is a natural by-product of planet formation. With the discovery of nu- merous extrasolar planets, it is likely that moons of extrasolar planets (exomoons) will soon be discovered. Some of the most promising techniques…

Earth and Planetary Astrophysics · Physics 2017-01-10 Amy C. Barr

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…

Earth and Planetary Astrophysics · Physics 2012-06-27 Simon B. Porter , William M. Grundy

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…

Earth and Planetary Astrophysics · Physics 2022-06-08 Vera Dobos , András Haris , Inga E. E. Kamp , Floris F. S. van der Tak

Since planets were first discovered outside our own Solar System in 1992 (around a pulsar) and in 1995 (around a main sequence star), extrasolar planet studies have become one of the most dynamic research fields in astronomy. Now that more…

Earth and Planetary Astrophysics · Physics 2009-10-06 Giammarco Campanella

Exomoons are the natural satellites of planets orbiting stars outside our solar system, of which there are currently no confirmed examples. We present new observations of a candidate exomoon associated with Kepler-1625b using the Hubble…

Earth and Planetary Astrophysics · Physics 2018-10-08 Alex Teachey , David M. Kipping

Beyond Earth-like planets, moons can be habitable, too. No exomoons have been securely detected, but they could be extremely abundant. Young Jovian planets can be as hot as late M stars, with effective temperatures of up to 2000 K. Transits…

Earth and Planetary Astrophysics · Physics 2016-03-16 René Heller

The field of exoplanetary science has experienced a recent surge of new systems that is largely due to the precision photometry provided by the Kepler mission. The latest discoveries have included compact planetary systems in which the…

Earth and Planetary Astrophysics · Physics 2015-06-17 Stephen R. Kane , Natalie R. Hinkel , Sean N. Raymond

Despite years of high accuracy observations, none of the available theoretical techniques has yet allowed the confirmation of a moon beyond the solar system. Methods are currently limited to masses about an order of magnitude higher than…

Earth and Planetary Astrophysics · Physics 2014-05-02 René Heller

For much of human history we have wondered how our solar system formed, and whether there are any other planets like ours around other stars. Only in the last 20 years have we had direct evidence for the existence of exoplanets, with the…

Solar and Stellar Astrophysics · Physics 2013-08-26 Jeffrey L. Coughlin

We demonstrate the ability of existing and planned telescopes, on the ground and in space, to directly image tidally heated exomoons orbiting gas-giant exoplanets. Tidally heated exomoons can plausibly be far more luminous than their host…

Earth and Planetary Astrophysics · Physics 2015-06-11 Mary Anne Peters , Edwin L. Turner

Moons of giant planets may represent an alternative to the classical picture of habitable worlds. They may exist within the circumstellar habitable zone of a parent star, and through tidal energy dissipation they may also offer alternative…

Astrophysics · Physics 2008-11-26 Caleb A. Scharf
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