Exoplanet status report: Observation, characterization and evolution of exoplanets and their host stars

被引：6

作者：

Lammer, H. ^{[1
]}

Hanslmeier, A. ^{[2
]}

Schneider, J. ^{[3
]}

Stateva, I. K. ^{[4
]}

Barthelemy, M. ^{[5
]}

Belu, A. ^{[6
]}

Bisikalo, D. ^{[7
]}

Bonavita, M. ^{[8
]}

Eybl, V. ^{[9
]}

du Foresto, V. Coude ^{[10
]}

Fridlund, M. ^{[11
]}

Dvorak, R. ^{[9
]}

Eggl, S. ^{[9
]}

Griessmeier, J. -M. ^{[12
]}

Guedel, M. ^{[9
,13
]}

Guenther, E. ^{[14
]}

Hausleitner, W. ^{[1
]}

Holmstrom, M. ^{[27
]}

Kallio, E. ^{[15
]}

Khodachenko, M. L. ^{[1
]}

Konovalenko, A. A. ^{[16
]}

Krauss, S. ^{[1
]}

Ksanfomality, L. V. ^{[17
]}

Kulikov, Yu N. ^{[18
]}

Kyslyakova, K. ^{[19
]}

Leitzinger, M. ^{[2
]}

Liseau, R. ^{[20
]}

Lohinger, E. ^{[9
]}

Odert, P. ^{[2
]}

Palle, E. ^{[14
]}

Reiners, A. ^{[21
]}

Ribas, I. ^{[22
]}

Rucker, H. O. ^{[1
]}

Sarda, N. ^{[23
]}

Seckbach, J. ^{[24
]}

Shematovich, V. I. ^{[7
]}

Sozzetti, A. ^{[25
]}

Tavrov, A. ^{[17
]}

Xiang-Gruess, M. ^{[26
]}

机构：

[1] Austrian Acad Sci, Space Res Inst IWF, Graz, Austria

[2] Graz Univ, Inst Geophys & Meteorol IGAM, A-8010 Graz, Austria

[3] Observ Paris, F-75014 Paris, France

[4] European Sci Fdn, Standing Comm Phys & Engn Sci, Strasbourg, France

[5] CNRS UJF, Lab Planetol Grenoble, Grenoble, France

[6] Univ Bordeaux, Bordeaux, France

[7] Russian Acad Sci, Inst Astron INASAN, Moscow, Russia

[8] Osservatorio Astron Padova INAF, Padua, Italy

[9] Univ Vienna, Inst Astron, A-1180 Vienna, Austria

[10] Observ Paris LESIA, Paris, France

[11] European Space Agcy, Estec, Noordwijk, Netherlands

[12] ASTRON, Dwingeloo, Netherlands

[13] ETH, Zurich Astrophys Inst Astron, Zurich, Switzerland

[14] Inst Astrofis Canarias, Tenerife, Spain

[15] Finish Meteorol Inst, Helsinki, Finland

[16] Ukrainian Acad Sci, Inst Radio Astron Kharkov, UA-252601 Kiev, Ukraine

[17] Russian Acad Sci, Space Res Inst IKI, Moscow, Russia

[18] Russian Acad Sci, PGI, Murmansk, Russia

[19] NI Lobachevsky State Univ, Nizhnii Novgorod, Russia

[20] Chalmers, Onsala Space Observ, S-43900 Onsala, Sweden

[21] Univ Gottingen, Inst Astrophys, Gottingen, Germany

[22] Inst Estudis Espacials Catalunya, Barcelona, Spain

[23] Astrium Ltd, Stevenage, Herts, England

[24] Hebrew Univ Jerusalem, Jerusalem, Israel

[25] INAF Osservatorio Astron Torino, Turin, Italy

[26] Univ Kiel, Inst Theoret Phys & Astrophys, Kiel, Germany

[27] Swedish Inst Space Phys, S-98128 Kiruna, Sweden

来源：

SOLAR SYSTEM RESEARCH | 2010年 / 44卷 / 04期

关键词：

ENERGETIC NEUTRAL ATOMS; EXTRASOLAR PLANETS; HD; 209458B; EARTH; ATMOSPHERE; GAIA;

D O I：

10.1134/S0038094610040039

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

After the discovery of more than 400 planets beyond our Solar System, the characterization of exoplanets as well as their host stars can be considered as one of the fastest growing fields in space science during the past decade. The characterization of exoplanets can only be carried out in a well coordinated interdisciplinary way which connects planetary science, solar/stellar physics and astrophysics. We present a status report on the characterization of exoplanets and their host stars by reviewing the relevant space- and ground-based projects. One finds that the previous strategy changed from space mission concepts which were designed to search, find and characterize Earth-like rocky exoplanets to: A statistical study of planetary objects in order to get information about their abundance, an identification of potential target and finally its analysis. Spectral analysis of exoplanets is mandatory, particularly to identify bio-signatures on Earth-like planets. Direct characterization of exoplanets should be done by spectroscopy, both in the visible and in the infrared spectral range. The way leading to the direct detection and characterization of exoplanets is then paved by several questions, either concerning the pre-required science or the associated observational strategy.

引用

页码：290 / 310

页数：21

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H. Lammer
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V. Eybl
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