English
Related papers

Related papers: Cryptoplanet update

200 papers

Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby stars. We now hope to conduct a census of all planets around nearby stars and to characterize their atmospheres and surfaces with spectroscopy. Rocky planets within…

Earth and Planetary Astrophysics · Physics 2009-11-17 J. Kasting , W. Traub , A. Roberge , A. Leger , A. Schwartz , A. Wooten , A. Vosteen , A. Lo , A. Brack , A. Tanner , A. Coustenis , B. Lane , B. Oppenheimer , B. Mennesson , B. Lopez , C. Grillmair , C. Beichman , C. Cockell , C. Hanot , C. McCarthy , C. Stark , C. Marois , C. Aime , D. Angerhausen , D. Montes , D. Wilner , D. Defrere , D. Mourard , D. Lin , E. Kite , E. Chassefiere , F. Malbet , F. Tian , F. Westall , G. Illingworth , G. Vasisht , G. Serabyn , G. Marcy , G. Bryden , G. White , G. Laughlin , G. Torres , H. Hammel , H. Ferguson , H. Shibai , H. Rottgering , J. Surdej , J. Wiseman , J. Ge , J. Bally , J. Krist , J. Monnier , J. Trauger , J. Horner , J. Catanzarite , J. Harrington , J. Nishikawa , K. Stapelfeldt , K. von Braun , K. Biazzo , K. Carpenter , K. Balasubramanian , L. Kaltenegger , M. Postman , M. Spaans , M. Turnbull , M. Levine , M. Burchell , M. Ealey , M. Kuchner , M. Marley , M. Dominik , M. Mountain , M. Kenworthy , M. Muterspaugh , M. Shao , M. Zhao , M. Tamura , N. Kasdin , N. Haghighipour , N. Kiang , N. Elias , N. Woolf , N. Mason , O. Absil , O. Guyon , O. Lay , P. Borde , P. Fouque , P. Kalas , P. Lowrance , P. Plavchan , P. Hinz , P. Kervella , P. Chen , R. Akeson , R. Soummer , R. Waters , R. Barry , R. Kendrick , R. Brown , R. Vanderbei , R. Woodruff , R. Danner , R. Allen , R. Polidan , S. Seager , S. MacPhee , S. Hosseini , S. Metchev , S. Kafka , S. Ridgway , S. Rinehart , S. Unwin , S. Shaklan , T. ten Brummelaar , T. Mazeh , V. Meadows , W. Weiss , W. Danchi , W. Ip , Y. Rabbia

Just fourteen years ago the Solar System represented the only known planetary system in the Galaxy, and conceptions of planet formation were shaped by this sample of one. Since then, 320 planets have been discovered orbiting 276 individual…

Earth and Planetary Astrophysics · Physics 2015-05-13 John A. Johnson

The recent detection of planets around very low mass stars raises the question of the formation, composition and potential habitability of these objects. We use planetary system formation models to infer the properties, in particular their…

Earth and Planetary Astrophysics · Physics 2017-02-01 Yann Alibert , Willy Benz

Approximately half of the extrasolar planets (exoplanets) with radii less than four Earth radii are in orbits with short periods. Despite their sheer abundance, the compositions of such planets are largely unknown. The available evidence…

The number of exoplanets detected using gravitational microlensing technique is currently larger than 200, which enables population studies. Microlensing is uniquely sensitive to low-mass planets orbiting at separations of several…

Earth and Planetary Astrophysics · Physics 2024-06-05 P. Mroz , R. Poleski

Planet formation encompasses processes that span a remarkable 40 magnitudes in mass, ranging from collisions between micron-sized grains inherited from the ISM to the accretion of gas by giant planets. The planet formation process takes…

Earth and Planetary Astrophysics · Physics 2024-12-18 Chris Ormel

This review is based on lectures given at the 45th Saas-Fee Advanced Course 'From Protoplanetary Disks to Planet Formation' held in March 2015 in Les Diablerets, Switzerland. Starting with an overview of the main characterictics of the…

Earth and Planetary Astrophysics · Physics 2017-07-25 Wilhelm Kley

Models of planet formation are built on underlying physical processes. In order to make sense of the origin of the planets we must first understand the origin of their building blocks. This review comes in two parts. The first part presents…

Earth and Planetary Astrophysics · Physics 2022-03-14 Sean N. Raymond , Alessandro Morbidelli

We hypothesise that planets are made by tidal downsizing of migrating giant planet embryos. The proposed scheme for planet formation consists of these steps: (i) a massive young protoplanetary disc fragments at R ~ several tens to hundreds…

Earth and Planetary Astrophysics · Physics 2015-05-19 Sergei Nayakshin

The prevailing assumption is that all exoplanets are made of ordinary matter. However, we propose an unconventional possibility that some exoplanets could be made of dark matter, which we name "dark exoplanets." In this paper, we explore…

Earth and Planetary Astrophysics · Physics 2023-11-20 Yang Bai , Sida Lu , Nicholas Orlofsky

The discovery of now about 20 extrasolar planets orbiting solar-type stars with properties quite different from those in our Solar System has raised many questions about the formation and evolution of planets. The tidal interaction between…

Astrophysics · Physics 2007-05-23 Willy Kley

Over 50 circumbinary exoplanets have been discovered in recent years, with several of them being gas giants on wide orbits ($>10$AU). The aim of this work is to investigate whether these planets can form through circumbinary disc…

Solar and Stellar Astrophysics · Physics 2026-04-28 Matthew Teasdale , Dimitris Stamatellos

I discuss the role that disc fragmentation plays in the formation of gas giant and terrestrial planets, and how this relates to the formation of brown dwarfs and low-mass stars, and ultimately to the process of star formation. Protostellar…

Earth and Planetary Astrophysics · Physics 2015-06-15 Dimitris Stamatellos

The evolution of gravitationally unstable protoplanetary gaseous disks has been studied with the use of three-dimensional smoothed particle hydrodynamics simulations with unprecedented resolution. We have considered disks with initial…

Astrophysics · Physics 2008-11-26 Lucio Mayer , Thomas Quinn , James Wadsley , Joachim Stadel

The discovery of the first extra-solar planet surrounding a main-sequence star was announced in 1995, based on very precise radial velocity (Doppler) measurements. A total of 34 such planets were known by the end of March 2000, and their…

Astrophysics · Physics 2008-11-26 M. A. C. Perryman

The first mass-estimate of an exoplanet around a Sun-like star, 51 Peg b and the first radius measurement of an exoplanet, HD209458b pointed to the challenges of understanding the atmosphere, interior, and evolution of exoplanets including…

Earth and Planetary Astrophysics · Physics 2021-12-15 Nadine Nettelmann , Diana Valencia

Among the hundred or so extrasolar planets discovered to date, 19 are orbiting a component of a double or multiple star system. In this paper, we discuss the properties of these planets and compare them to the characteristics of planets…

Astrophysics · Physics 2009-11-10 A. Eggenberger , S. Udry , M. Mayor

6500+ exoplanets have been detected using various techniques. This prompted the emergence of many recent works on the taxonomy, or classification, of exoplanets. However, there is still no basic, fundamental definition of 'What is a…

Earth and Planetary Astrophysics · Physics 2026-02-03 Madhu Kashyap Jagadeesh , Arkil Parikh , Margarita Safonova , Bernard Foing , Oleg Kotsyurbenko

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

Recent spacecraft observations exploring solar system properties impact standard paradigms of the formation of stars, planets and comets. We stress the unexpected cloud of microscopic dust resulting from the DEEP IMPACT mission, and the…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-30 Rudolph E. Schild , Carl H. Gibson