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Extrasolar Planets Encyclopaedia

From Wikipedia, the free encyclopedia
Astronomical database
The Extrasolar Planets Encyclopaedia
Home page, as seen on December 14, 2023
Type of site
Astronomy
OwnerParis Observatory
Created byJean Schneider
URLexoplanet.euEdit this at Wikidata
Registrationnone
LaunchedFebruary 1995
Current statusActive
Content license
CC-BY 4.0[1]

TheExtrasolar Planets Encyclopaedia[2][3][4][5][6] (also known asEncyclopaedia of exoplanetary systems andCatalogue of Exoplanets) is anastronomywebsite, founded inParis,France at theMeudon Observatory byJean Schneider in February 1995,[7][8] which maintains a database of all the currently known and candidateextrasolar planets, with individual pages for each planet and a full list interactive catalog spreadsheet. The main catalogue comprises databases of all of the currently confirmed extrasolar planets as well as a database of unconfirmed planet detections. The databases are frequently updated with new data from peer-reviewed publications and conferences.

In their respective pages, theplanets are listed along with their basic properties, including the year of planet's discovery,mass,radius,orbital period,semi-major axis,eccentricity,inclination,longitude of periastron, time ofperiastron,maximum time variation, andtime of transit, including all error range values.

The individual planet data pages also contain the data on the parent star, including name, distance inparsecs,spectral type,effective temperature,apparent magnitude,mass,radius,age, and celestial coordinates (Right Ascension andDeclination). Even when they are known, not all of these figures are listed in the interactive spreadsheet catalog, and many missing planet figures that would simply require the application ofKepler's third law of motion are left blank. Most notably absent on all pages is a star'sluminosity.

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

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References

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  1. ^Martin, Pierre-Yves (1995)."Mentions Légales".Extrasolar Planets Encyclopaedia.
  2. ^Pätzold, M.; Rauer, H. (2002). "Where Are the Massive Close-in Extrasolar Planets?".Astrophysical Journal Letters.568 (2): L117.Bibcode:2002ApJ...568L.117P.doi:10.1086/339794.
  3. ^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".Astrophysical Journal.604 (1):388–413.arXiv:astro-ph/0312144.Bibcode:2004ApJ...604..388I.doi:10.1086/381724.S2CID 119454346.
  4. ^Raymond, S. N.; Mandell, A. M.; Sigurdsson, S. (2006). "Exotic Earths: Forming Habitable Worlds with Giant Planet Migration".Science.313 (5792):1413–6.arXiv:astro-ph/0609253.Bibcode:2006Sci...313.1413R.doi:10.1126/science.1130461.PMID 16960000.S2CID 20112677.
  5. ^Armstron, J. C.; Larson, S. L. (2007). "Specific Angular Momenta of Extrasolar Planetary Systems".Bulletin of the American Astronomical Society.38: 105.Bibcode:2007AAS...210.0904A.
  6. ^Stevenson, D. J. (2008)."A planetary perspective on the deep Earth".Nature.451 (7176):261–5.Bibcode:2008Natur.451..261S.doi:10.1038/nature06582.PMID 18202637.
  7. ^Kirkland, K. (2010).Space and Astronomy: Notable Research and Discoveries.Frontiers of Science.Infobase Publishing. p. 29.ISBN 978-0-8160-7445-7.
  8. ^Dvořák, R. (2008).Extrasolar Planets: Formation, Detection and Dynamics.Wiley-VCH. p. 57.ISBN 978-3-527-40671-5.
  9. ^Schneider, J.; Dedieu, C.; Le Sidaner, P.; Savalle, R.; Zolotukhin, I. (2011). "Defining and Cataloging Exoplanets: The Exoplanet.eu Database".Astronomy & Astrophysics.532: A79.arXiv:1106.0586.Bibcode:2011A&A...532A..79S.doi:10.1051/0004-6361/201116713.S2CID 55994657.
  10. ^Matson, J. (29 November 2010)."How One Astronomer Became the Unofficial Exoplanet Record-Keeper".Scientific American. Retrieved2012-07-29.
  11. ^Schneider, J. (2016). "III.8 Exoplanets versus brown dwarfs: The CoRoT view and the future".The CoRoT Legacy Book. p. 157.arXiv:1604.00917.doi:10.1051/978-2-7598-1876-1.c038.ISBN 978-2-7598-1876-1.
  12. ^Hatzes Heike Rauer, Artie P. (2015). "A Definition for Giant Planets Based on the Mass-Density Relationship".The Astrophysical Journal.810 (2): L25.arXiv:1506.05097.Bibcode:2015ApJ...810L..25H.doi:10.1088/2041-8205/810/2/L25.S2CID 119111221.

External links

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