HD 24040b was discovered in 2006 based on observations made at the W. M. Keck Observatory in Hawaii. However, because the observations covered less than one complete orbit there were only weak constraints on the period and mass.[2] The first reliable orbit for HD 24040b was obtained by astronomers at Haute-Provence Observatory in 2012 who combined the keck measurements with ones from the SOPHIE and ELODIE spectrographs.[3] The most recent orbit published in 2015 added additional keck measurements and refined the orbital parameters.[1]
Referencesedit
^ abcdefgFeng, Y. Katherina; et al. (2015). "The California Planet Survey IV: A Planet Orbiting the Giant Star HD 145934 and Updates to Seven Systems with Long-period Planets". The Astrophysical Journal. 800 (1). 22. arXiv:1501.00633. Bibcode:2015ApJ...800...22F. doi:10.1088/0004-637X/800/1/22. S2CID 56390823.
^Wright, J. T.; et al. (2007). "Four New Exoplanets and Hints of Additional Substellar Companions to Exoplanet Host Stars". The Astrophysical Journal. 657 (1): 533–545. arXiv:astro-ph/0611658. Bibcode:2007ApJ...657..533W. doi:10.1086/510553. S2CID 35682784.
24040, long, period, exoplanet, taking, approximately, 3500, days, orbit, astronomical, units, almost, circular, orbit, minimum, mass, times, that, jupiter, discoverydiscovered, bybutler, discovery, sitecalifornia, usadiscovery, datemarch, 2006detection, metho. HD 24040 b is a long period exoplanet taking approximately 3500 days to orbit at 4 6 astronomical units in an almost circular orbit It has a minimum mass 4 times that of Jupiter 1 HD 24040 bDiscoveryDiscovered byButler et al Discovery siteCalifornia USADiscovery dateMarch 12 2006Detection methodDoppler spectroscopyOrbital characteristicsSemi major axis4 637 0 067 AUEccentricity0 047 0 020 1 Orbital period sidereal 3490 25 1 dTime of periastron2456 670 240 1 Argument of periastron67 24 1 Semi amplitude51 8 1 6 1 StarHD 24040Discovery editHD 24040b was discovered in 2006 based on observations made at the W M Keck Observatory in Hawaii However because the observations covered less than one complete orbit there were only weak constraints on the period and mass 2 The first reliable orbit for HD 24040b was obtained by astronomers at Haute Provence Observatory in 2012 who combined the keck measurements with ones from the SOPHIE and ELODIE spectrographs 3 The most recent orbit published in 2015 added additional keck measurements and refined the orbital parameters 1 References edit a b c d e f g Feng Y Katherina et al 2015 The California Planet Survey IV A Planet Orbiting the Giant Star HD 145934 and Updates to Seven Systems with Long period Planets The Astrophysical Journal 800 1 22 arXiv 1501 00633 Bibcode 2015ApJ 800 22F doi 10 1088 0004 637X 800 1 22 S2CID 56390823 Wright J T et al 2007 Four New Exoplanets and Hints of Additional Substellar Companions to Exoplanet Host Stars The Astrophysical Journal 657 1 533 545 arXiv astro ph 0611658 Bibcode 2007ApJ 657 533W doi 10 1086 510553 S2CID 35682784 Boisse Isabelle Pepe Francesco Perrier Christian Queloz Didier Bonfils Xavier Bouchy Francois Santos Nuno C Arnold Luc Beuzit Jean Luc Diaz Rodrigo F Delfosse Xavier Eggenberger Anne Ehrenreich David Forveille Thierry Hebrard Guillaume Lagrange Anne Marie Lovis Christophe Mayor Michel Moutou Claire Naef Dominique Santerne Alexandre Segransan Damien Sivan Jean Pierre Udry Stephane 2012 The SOPHIE search for northern extrasolar planets V Follow up of ELODIE candidates Jupiter analogs around Sun like stars Astronomy and Astrophysics 545 A55 arXiv 1205 5835 Bibcode 2012A amp A 545A 55B doi 10 1051 0004 6361 201118419 S2CID 119109836External links edit HD 24040 Exoplanets Archived from the original on 2012 02 19 Retrieved 2008 09 10 nbsp This extrasolar planet related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title HD 24040 b amp oldid 1122701226, wikipedia, wiki, book, books, library,
