Abstract:A half of the Nobel Prize in Physics 2019 was awarded jointly to Michel Mayor and Didier Queloz for the discovery of an exoplanet orbiting a solar-type star. In this paper we review the academic achievements of these two scientists, the scientific significance of this important discovery, and the future development of this research area in China.
马波. 太阳系外行星的探测——2019年诺贝尔物理学奖成果简析[J]. 科技导报, 2019, 37(24): 30-35.
MA Bo. Exploration of an Exoplanet: Commentary on the Nobel Prize in Physics 2019. Science & Technology Review, 2019, 37(24): 30-35.
[1] Mayor M, Queloz D. A Jupiter-mass companion to a solar-type star[J]. Nature, 1995, 378(6555):355-359.
[2] NASA exoplanet archive[EB/OL].[2019-10-20]. https://exoplanetarchive.ipac.caltech.edu.
[3] Wright J T, Fakhouri O, Marcy G W, et al. The exoplanet orbit database[J]. Publications of the Astronomical Society of the Pacific 2011, 123:412-422.
[4] Howard A W, Marcy G W, Bryson S T, et al. Planet occurrence within 0.25 AU of solar-type stars from Kepler[J]. The Astrophysical Journal, 2012, 201(Suppl):15.
[5] Borucki W J, Koch D, Basri G, et al. Kepler planet-detection mission:Introduction and first results[J]. Science, 2010, 327(5968):977-980.
[6] Borucki W J, Koch D G, Basri G, et al. Characteristics of planetary candidates observed by Kepler, II:Analysis of the first four months of data[J]. The Astrophysical Journal, 2011, 736(1):19.
[7] Struve O. Proposal for a project of high-precision stellar radial velocity work[J]. The Observatory1952, 72:199-200.
[8] Griffin. On the possibility of determining stellar radial velocities to 0.01 km s-1[J]. Monthly Notices of the Royal Astronomical Society, 1973, 162(3):243-253.
[9] Ilovaisky S A. A user's guide to Elodie archive data products[EB/OL].[2019-10-20]. http://www.obs-hp.fr/www/archive/elodie-for-dummies.html.
[10] Baranne A, Mayor M, Poncet J L. Coravel-A new tool for radial velocity measurements[J]. Vistas in Astronomy. 1979, 23:279-316.
[11] Marcy G W, Butler R P. Precision radial velocities with an iodine absorption cell[J]. Publications of The Astronomical Society of The Pacific, 1992, 104:270-277.
[12] Butler R P, Marcy G W, Williams E, et al. Attaining doppler precision of 3 m s-1[J]. Publications of The Astronomical Society of The Pacific, 1996, 108:500-509.
[13] Vogt S S, Allen S L, Bigelow B C, et al. HIRES:The high-resolution echelle spectrometer on the Keck 10-m telescope[J]. Proceedings of SPIE, 1994, 2198:362-375.
[14] Mayor M, Pepe F, Queloz D, et al. Setting new standards with HARPS[J]. ESO Messenger, 2003, 114:20.
[15] Pepe F A, Cristiani S, Lopez R R, et al. ESPRESSO:The Echelle spectrograph for rocky exoplanets and stable spectroscopic observations[J]. Proceedings of SPIE-The International Society for Optical Engineering, Doi:10.1117/12.857122.
[16] Ma B, Ge J, Muterspaugh M, et al. The first superEarth detection from Dharma Planet Survey[J]. Monthly Notices of the Royal Astronomical Society, 2018, 480(2):2411-2422.
[17] Schwab C, Rakich A, Gong Q, et al. Design of NEID, an extreme precision Doppler spectrograph for WIYN[EB/OL].[2019-10-20]. https://doi.org/10.1117/12.2234411.
[18] Vogt S S, Radovan M, Kibrick R, et al. APF:The Lick Observatory Automated Planet Finder[J]. Publications of the Astronomical Society of the Pacific, 2014, 126:359.