Results 11 to 20 of about 4,693,249 (249)
Atmospheric signatures of giant exoplanet formation by pebble accretion [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 Atmospheric chemical abundances of giant planets lead to important constraints on planetary formation and migration. Studies have shown that giant planets that migrate through the protoplanetary disk can accrete substantial amounts of oxygen-rich ...
N. Madhusudhan +3 more
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Characterization of exoplanets from their formation [PDF]
Astronomy and Astrophysics, 2012 A first characterization of many exoplanets has recently been achieved by the observational determination of their radius. For some planets, a measurement of the luminosity has also been possible, with many more directly imaged planets expected in the future.
C. Mordasini +3 more
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Understanding exoplanet formation, structure and evolution in 2010 [PDF]
Proceedings of the International Astronomical Union, 2010 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.
G. Chabrier, J. Leconte, I. Baraffe
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Characterization of exoplanets from their formation III: The statistics of planetary luminosities [PDF]
Astronomy & Astrophysics, 2017 44 pages, 26 figures (journal format). A&A in print.
C. Mordasini +2 more
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C/O Ratios and the Formation of Wide-separation Exoplanets [PDF]
The Astrophysical Journal LettersThe gas and solid-state C/O ratios provide context to potentially link the atmospheric composition of planets to that of the natal disk. We provide a synthesis of extant estimates of the gaseous C/O and C/H ratios in planet-forming disks obtained ...
E. Bergin +3 more
semanticscholar +4 more sources
On the Local Formation of the TRAPPIST-1 Exoplanets [PDF]
The Astronomical JournalAbstract The discovery of seven approximately Earth-mass planets orbiting the 0.09 M ⊙ M dwarf TRAPPIST-1 captivated the public and sparked a proliferation of investigations into the system’s origins. Among other properties, the resonant architecture of the planets has been interpreted to imply that orbital migration ...
Matthew S. Clement +2 more
+6 more sources
Planet Formation Theory in the Era of ALMA and Kepler: from Pebbles to\n Exoplanets [PDF]
Drazkowska , J , Bitsch , B , Lambrechts , M T A , Mulders , G D , Harsono , D , Vazan , A , Liu , B , Ormel , C W , Kretke , K & Morbidelli , A 2022 ' Planet Formation Theory in the Era of ALMA and Kepler : from Pebbles to Exoplanets ' arXiv.org . https://doi.org/10.48550/arXiv.2203.09759, 2022 38 pages, 13 figures, review chapter accepted to Protostars and Planets VII, editors: Shu-ichiro Inutsuka, Yuri Aikawa, Takayuki Muto, Kengo Tomida, and Motohide Tamura, corrected label in Fig ...
Joanna Dra̧żkowska +9 more
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Planet formation – implication of statistical properties of exoplanets [PDF]
Journal of Physics: Conference Series, 2010 Models of planetary formation are developed based on the observation of our Solar System, star-forming regions and circumstellar disks and on an the ever increasing number of exoplanetary systems. The solar nebula theory and the planetesimal hypothesis are discussed.
Á. Süli
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Set to Music, Exoplanets Reveal Insights on Their Formation
Eos, 2019 Sonification hints at how some Kepler planets may have been configured in the late stages of their development.
Nola Redd
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Formation, Evolution and Multiplicity of Brown Dwarfs and Giant Exoplanets [PDF]
, 2010 "Highlights of Spanish Astrophysics V", Proceedings of the VIII Scientific Meeting of the Spanish Astronomical Society (SEA) held in Santander, 7-11 July, 2008. Edited by J. Gorgas, L. J. Goicoechea, J. I. Gonzalez-Serrano, J. M. Diego.
J. A. Caballero, J. A. Caballero
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