Extrasolar Planets Encyclopaedia
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The Extrasolar Planets Encyclopaedia
In their respective pages, the
, including all error range values.The individual planet data pages also contain the data on the parent star, including name, distance in
As of June 2011, the catalog includes objects up to 25 Jupiter masses,[9] an increase on the previous inclusion criteria of 20 Jupiter masses.[10] As of 2016 this limit was increased to 60 Jupiter masses[11] based on a study of mass–density relationships.[12]
See also
References
- ^ Martin, Pierre-Yves (1995). "Mentions Légales". Extrasolar Planets Encyclopaedia.
- ^
Pätzold, M.; Rauer, H. (2002). "Where Are the Massive Close-in Extrasolar Planets?". doi:10.1086/339794.
- ^
Ida, S.; Lin, D. N. C. (2004). "Toward a Deterministic Model of Planetary Formation. I. A Desert in the Mass and Semimajor Axis Distributions of Extrasolar Planets". S2CID 119454346.
- ^
Raymond, S. N.; Mandell, A. M.; Sigurdsson, S. (2006). "Exotic Earths: Forming Habitable Worlds with Giant Planet Migration". S2CID 20112677.
- ^
Armstron, J. C.; Larson, S. L. (2007). "Specific Angular Momenta of Extrasolar Planetary Systems". Bibcode:2007AAS...210.0904A.
- ^
Stevenson, D. J. (2008). "A planetary perspective on the deep Earth". PMID 18202637.
- ^
Kirkland, K. (2010). Space and Astronomy: Notable Research and Discoveries. ISBN 978-0-8160-7445-7.
- ^
Dvořák, R. (2008). Extrasolar Planets: Formation, Detection and Dynamics. ISBN 978-3-527-40671-5.
- ^
Schneider, J.; Dedieu, C.; Le Sidaner, P.; Savalle, R.; Zolotukhin, I. (2011). "Defining and Cataloging Exoplanets: The Exoplanet.eu Database". S2CID 55994657.
- ^ Matson, J. (29 November 2010). "How One Astronomer Became the Unofficial Exoplanet Record-Keeper". Scientific American. Retrieved 2012-07-29.
- ^ Exoplanets versus brown dwarfs: the CoRoT view and the future, Jean Schneider, 4 Apr 2016
- S2CID 119111221.