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Related papers: Evidence for a Large Exomoon Orbiting Kepler-1625b

200 papers

Exoplanets classified as super-Earths are commonly observed on short period orbits, close to their host stars, but their abundance on wider orbits is poorly constrained. Gravitational microlensing is sensitive to exoplanets on wide orbits.…

Whereas the Solar System has Mars and Europa as the best candidates for finding fossil/extant life as we know it - based on complex carbon compounds and liquid water - the 263 (non-pulsar) planetary systems around other stars as known at 15…

Earth and Planetary Astrophysics · Physics 2018-12-05 Barrie W Jones

Context: Detecting moons around exoplanets is a major goal of current and future observatories. Moons are suspected to influence rocky exoplanet habitability, and gaseous exoplanets in stellar habitable zones could harbour abundant and…

Earth and Planetary Astrophysics · Physics 2018-10-24 Javier Berzosa Molina , Loic Rossi , Daphne M. Stam

The current exoplanet database includes 5454 confirmed planets and candidate planets observed with the KEPLER mission. We find 932 planet pairs from which we extract distance and orbital period ratios. While earlier studies used the…

Earth and Planetary Astrophysics · Physics 2017-09-26 Markus J. Aschwanden , Felix Scholkmann

The Kepler spacecraft, whose single instrument was a 0.95 m diameter wide-field telescope, operated in a heliocentric orbit for nearly a decade, returning a wealth of data that have revolutionized exoplanet science. Kepler data have been…

Earth and Planetary Astrophysics · Physics 2023-11-10 Jack J. Lissauer , Natalie M. Batalha , William J. Borucki

We conduct a comprehensive search for transiting exomoons and exosatellites within 44 archival Spitzer light curves of 32 substellar worlds with estimated masses ranging between 3-30M$_{\rm Jup}$. This sample's median host mass is 16M$_{\rm…

Earth and Planetary Astrophysics · Physics 2024-05-15 Mary Anne Limbach , Johanna M. Vos , Andrew Vanderburg , Fei Dai

Direct imaging of exoplanetary systems is a powerful technique that can reveal Jupiter-like planets in wide orbits, can enable detailed characterization of planetary atmospheres, and is a key step towards imaging Earth-like planets. Imaging…

Astrophysics · Physics 2009-09-17 C. Marois , B. Macintosh , T. Barman , B. Zuckerman , I. Song , J. Patience , D. Lafreniere , R. Doyon

We identify a subsample of the recently detected extrasolar planets that is minimally affected by the selection effects of the Doppler detection method. With a simple analysis we quantify trends in the surface density of this subsample in…

Astrophysics · Physics 2009-11-07 Charles H. Lineweaver , Daniel Grether

In this work, we hunt for the best places to find exo-Earths in the currently known exoplanet population. While it is still unclear whether Jupiter had a beneficial or detrimental effect on the creation of the right environment for a…

Earth and Planetary Astrophysics · Physics 2018-09-26 Matthew T. Agnew , Sarah T. Maddison , Jonathan Horner

The highest priority recommendation of the Astro2020 Decadal Survey for space-based astronomy was the construction of an observatory capable of characterizing habitable worlds. In this paper series we explore the detectability of and…

Earth and Planetary Astrophysics · Physics 2024-05-07 Mary Anne Limbach , Jacob Lustig-Yaeger , Andrew Vanderburg , Johanna M. Vos , Rene Heller , Tyler D. Robinson

With their smaller radii and high cosmic abundance, transiting planets around cool stars hold a unique appeal. As part of our on-going project to measure the occurrence rate of extrasolar moons, we here present results from a survey…

Earth and Planetary Astrophysics · Physics 2015-06-18 David M. Kipping , David Nesvorny , Lars A. Buchhave , Joel Hartman , Gáspár Á. Bakos , Allan R. Schmitt

As of 2025, over 6000 planets are known to orbit stars other than our Sun. We can measure their sizes and orbital periods, infer their masses and temperatures, and constrain their compositions. Based on these data, about 1% of extrasolar…

Astrophysics of Galaxies · Physics 2025-10-13 Floris van der Tak

Three transiting exoplanet candidate stars were discovered in a ground-based photometric survey prior to the launch of NASA's {\it Kepler} mission. {\it Kepler} observations of them were obtained during Quarter 1 of the {\it Kepler}…

In this short review, we summarize our present understanding (and non-understanding) of exoplanet formation, structure and evolution, in the light of the most recent discoveries. Recent observations of transiting massive brown dwarfs seem…

Solar and Stellar Astrophysics · Physics 2015-05-20 G. Chabrier , J. Leconte , I. Baraffe

The search for extrasolar planets is strongly motivated by the goal of characterizing how frequent habitable worlds and life may be within the Galaxy. Whilst much effort has been spent on searching for Earth-like planets, large moons may…

Earth and Planetary Astrophysics · Physics 2015-03-19 David M. Kipping

The holy grail of exoplanet searches is an exo-Earth, an Earth mass planet in the habitable zone around a nearby star. Mass is the most important parameter of a planet and can only be measured by observing the motion of the star around the…

Earth and Planetary Astrophysics · Physics 2010-06-23 Michael Shao , Joseph Catanzarite , Xiaopei Pan

It has been recently claimed that KOIs-268.01, 303.01, 1888.01, 1925.01, 2728.01 & 3320.01 are exomoon candidates, based on an analysis of their transit timing. Here, we perform an independent investigation, which is framed in terms of…

Earth and Planetary Astrophysics · Physics 2020-08-11 David Kipping

Submoons, moons orbiting other moons, may be exotic environments capable of hosting extraterrestrial life. We extend previous studies to revise the maximum lifetime of these objects due to planetary, lunar and sublunar tidal migration.…

Earth and Planetary Astrophysics · Physics 2025-10-17 Iason Saganas , Grant Mayberry , Barbara Ercolano

In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of $7.6 \pm 0.6$ Jupiter…