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(Aims) We investigate whether volcanic exomoons can be detected in thermal wavelength light curves due to their phase variability along their orbit. The method we use is based on the photometric signal variability that volcanic features or…

地球与行星天体物理 · 物理学 2024-07-03 E. Kleisioti , D. Dirkx , X. Tan , M. A. Kenworthy

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

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…

地球与行星天体物理 · 物理学 2015-06-11 Mary Anne Peters , Edwin L. Turner

Exomoons are expected to orbit gas giant exoplanets just as moons orbit solar system planets. Tidal heating is present in solar system satellites and it can heat up their interior depending on their orbital and interior properties. We aim…

地球与行星天体物理 · 物理学 2023-07-12 E. Kleisioti , D. Dirkx , M. Rovira-Navarro , M. A. Kenworthy

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 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

Using viscoelastic mass spring model simulations to track heat distribution inside a tidally perturbed body, we measure the asymmetry of heating in the crust of a spin synchronous Moon in eccentric orbit about the Earth. With the Moon…

地球与行星天体物理 · 物理学 2019-05-01 Alice C. Quillen , Larkin Martini , Miki Nakajima

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…

地球与行星天体物理 · 物理学 2013-10-31 René Heller , Rory Barnes

Though efforts to detect them have been made with a variety of methods, no technique can claim a successful, confirmed detection of a moon outside the Solar System yet. Moon detection methods are restricted in capability to detecting moons…

地球与行星天体物理 · 物理学 2024-02-13 Quirijn B. van Woerkom , Evangelia Kleisioti

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…

地球与行星天体物理 · 物理学 2016-03-16 René Heller

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

Tidal heating of exomoons may play a key role in their habitability, since the elevated temperature can melt the ice on the body even without significant solar radiation. The possibility of life is intensely studied on Solar System moons…

地球与行星天体物理 · 物理学 2015-04-30 Vera Dobos , Edwin L. Turner

The number of known transiting exoplanets is rapidly increasing, which has recently inspired significant interest as to whether they can host a detectable moon. Although there has been no such example where the presence of a satellite was…

太阳与恒星天体物理 · 物理学 2015-05-20 Gy. M. Szabo , A. E. Simon , L. L. Kiss , Zs. Regaly

M type stars are good targets in the search for habitable extrasolar planets. Because of their low effective temperatures, the habitable zone of M stars is very close to the star itself. For planets close to their stars, tidal heating plays…

地球与行星天体物理 · 物理学 2014-06-11 Daigo Shoji , Kei Kurita

In the Jupiter-Io system, the moon's motion produces currents along the field lines that connect it to Jupiter's polar regions. The currents generate, and modulate radio emissions along their paths via the electron-cyclotron maser…

地球与行星天体物理 · 物理学 2015-06-16 Joaquin P. Noyola , Suman Satyal , Zdzislaw E. Musielak

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

More than 200 moons exist in our Solar System, yet no exomoon has been confirmed to date. While the innermost two planets of the Solar System lack natural satellites and most studies favour the existence of exomoons around long-period…

地球与行星天体物理 · 物理学 2026-03-20 Xinyi Song , Jun Yang , Yueyun Ouyang

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

From analytical studies of tidal heating, eclipses and planetary illumination, it is clear that the exomoon habitable zone (EHZ) - the set of moon and host planet orbits that permit liquid water on an Earthlike moon's surface - is a…

地球与行星天体物理 · 物理学 2015-06-19 Duncan Forgan , Vergil Yotov

Large surface temperatures on the illuminated hemisphere of the Moon can lead it to contribute a significant amount of flux to spatially unresolved infrared (IR) observations of the Earth-Moon system, especially at wavelengths where Earth's…

地球与行星天体物理 · 物理学 2015-05-30 Tyler D. Robinson
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