The Realm of Extrasolar Planets

被引:0
作者
Ferlet, Roger [1 ]
机构
[1] UPMC, CNRS, Inst Astrophys Paris, F-75014 Paris, France
来源
THIRD ALGERIAN WORKSHOP ON ASTRONOMY AND ASTROPHYSICS | 2010年 / 1295卷
关键词
Extrasolar planets; detection; characterization; TRANSITING PLANET; MASS COMPANION; BROWN DWARF; ATMOSPHERE; DISCOVERY; EMISSION;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
hi November 1995, an article published in Nature [1] put planetary sciences not only as a new hot field in both observational and theoretical astrophysics but also as a topic with a large impact toward the layman. This article was reporting the first discovery of a planet orbiting a star beyond our Sun, namely the solar-type star 51 Pegasi. Nearly four centuries after Giordano Bruno was burnt in public in Roma partly for having intuitively claimed the plurality of worlds, we were entering the extraordinary epoch in which one of the oldest inquiries of mankind - are we alone in the Universe ? - can be tackled with the scientific method, leaving aside centuries of endless speculations. To date (July 2010), almost 500 extrasolar planets are known. We shall briefly review the main detection methods, together with the big surprises which arose during these last exciting fifteen years, without being exhaustive.
引用
收藏
页码:16 / 24
页数:9
相关论文
共 50 条
  • [31] Spectroscopic Characterisation of Close Orbiting Extrasolar Giant Planets
    Barnes, J. R.
    Barman, Travis S.
    Jones, H. R. A.
    Leigh, C. J.
    Cameron, A. Collier
    Prato, Lisa
    Barber, R.
    COOL STARS, STELLAR SYSTEMS AND THE SUN, 2009, 1094 : 417 - +
  • [32] Models of the in situ formation of detected extrasolar giant planets
    Bodenheimer, P
    Hubickyj, O
    Lissauer, JJ
    ICARUS, 2000, 143 (01) : 2 - 14
  • [33] Characterizing habitable extrasolar planets using spectral fingerprints
    Kaltenegger, Lisa
    Selsis, Franck
    COMPTES RENDUS PALEVOL, 2009, 8 (07) : 679 - 691
  • [34] Requirements of a nulling space interferometer for the search for extrasolar planets
    Kaltenegger, L
    Karlsson, A
    Neger, T
    ASTRONOMY AT IR/SUBMM AND THE MICROWAVE BACKGOUND, 2004, 34 (03): : 618 - 624
  • [35] Intercomparison of general circulation models for hot extrasolar planets
    Polichtchouk, I.
    Cho, J. Y-K.
    Watkins, C.
    Thrastarson, H. Th.
    Umurhan, O. M.
    de la Torre Juarez, M.
    ICARUS, 2014, 229 : 355 - 377
  • [36] Mass-radius curve for extrasolar Earth-like planets and ocean planets
    Sotin, C.
    Grasset, O.
    Mocquet, A.
    ICARUS, 2007, 191 (01) : 337 - 351
  • [37] PEPPER: a photometer designed for the direct detection of extrasolar planets
    Graham, MC
    Potter, DE
    Close, L
    GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3, 2004, 5492 : 545 - 552
  • [38] Searching for extra-terrestrial intelligence and the discovering of extrasolar planets
    Wu, GJ
    Chen, DH
    CHINESE ASTRONOMY AND ASTROPHYSICS, 2002, 26 (02) : 125 - 140
  • [39] An intuitive clustering algorithm for spherical data with application to extrasolar planets
    Hung, Wen-Liang
    Chang-Chien, Shou-Jen
    Yang, Miin-Shen
    JOURNAL OF APPLIED STATISTICS, 2015, 42 (10) : 2220 - 2232
  • [40] Direct Imaging of Extrasolar Planets: Overview of Ground and Space Programs
    Boccaletti, A.
    MOLECULES IN THE ATMOSPHERES OF EXTRASOLAR PLANETS, 2011, 450 : 163 - 172