Impact of space weather on climate and habitability of terrestrial-type exoplanets

被引：171

作者：

Airapetian, V. S. ^{[1
,2
]}

Barnes, R. ^{[3
]}

Cohen, O. ^{[4
]}

Collinson, G. A. ^{[1
]}

Danchi, W. C. ^{[1
]}

Dong, C. F. ^{[5
]}

Del Genio, A. D. ^{[6
]}

France, K. ^{[7
]}

Garcia-Sage, K. ^{[1
]}

Glocer, A. ^{[1
]}

Gopalswamy, N. ^{[1
]}

Grenfell, J. L. ^{[8
]}

Gronoff, G. ^{[9
]}

Guedel, M. ^{[10
]}

Herbst, K. ^{[11
]}

Henning, W. G. ^{[1
]}

Jackman, C. H. ^{[1
]}

Jin, M. ^{[12
]}

Johnstone, C. P. ^{[10
]}

Kaltenegger, L. ^{[13
]}

Kay, C. D. ^{[11
]}

Kobayashi, K. ^{[14
]}

Kuang, W. ^{[1
]}

Li, G. ^{[15
]}

Lynch, B. J. ^{[16
]}

Lueftinger, T. ^{[10
]}

Luhmann, J. G. ^{[16
]}

Maehara, H. ^{[17
]}

Mlynczak, M. G. ^{[9
]}

Notsu, Y. ^{[18
]}

Osten, R. A. ^{[30
,31
]}

Ramirez, R. M. ^{[19
]}

Rugheimer, S. ^{[20
]}

Scheucher, M. ^{[21
]}

Schlieder, J. E. ^{[1
]}

Shibata, K. ^{[22
]}

Sousa-Silva, C. ^{[23
]}

Stamenkovic, V ^{[24
]}

Strangeway, R. J. ^{[25
]}

Usmanov, A., V ^{[1
,26
]}

Vergados, P. ^{[24
]}

Verkhoglyadova, O. P. ^{[24
]}

Vidotto, A. A. ^{[27
]}

Voytek, M. ^{[28
]}

Way, M. J. ^{[6
]}

Zank, G. P. ^{[15
]}

Yamashiki, Y. ^{[29
]}

机构：

[1] NASA, Sellers Exopianet Environm Collaborat, GSFC, Greenbelt, MD 20771 USA

[2] Amer Univ, Dept Phys, Washington, DC 20016 USA

[3] Univ Washington, Seattle, WA 98195 USA

[4] Univ Massachusetts, Lowell Ctr Space Sci & Technol, Lowell, MA USA

[5] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[6] NASA, Goddard Inst Space Studies, New York, NY 10025 USA

[7] Univ Colorado, Lab Atmospher & Space Phys, 600 UCB, Boulder, CO 80309 USA

[8] German Aerosp Ctr DLR, Inst Planetary Res, Dept Extrasoiar Planets & Atmospheres EPA, Rutherfordstr 2, D-12489 Berlin, Adiershof, Germany

[9] NASA, LaRC, Hampton, VA USA

[10] Univ Vienna, Dept Astrophys, Turkenschanzstr 17, A-1180 Vienna, Austria

[11] Christian Albrechts Univ Kiel, Inst Expt & Appl Phys, Leibnizstr 11, D-24118 Kiel, Germany

[12] SETI Inst, Mountain View, CA 94043 USA

[13] Cornell Univ, Carl Sagan Inst, Ithaca, NY USA

[14] Yokohama Natl Univ, Dept Chem, Yokohama, Kanagawa, Japan

[15] Univ Alabama, Ctr Space Plasma & Aeron Res CSPAR, Huntsville, AL 35899 USA

[16] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[17] NAOJ, Subaru Telescope Okayama Branch Off, Asakuchi, Okayama 71902, Japan

[18] Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto, Japan

[19] Tokyo Inst Technol, Earth Life Sci Inst, Tokyo 1528550, Japan

[20] Univ St Andrews, Sch Earth & Environm Sci, Ctr Exoplanet Sci, Irvine Bldg,North St, St Andrews KY16 9AL, Fife, Scotland

[21] Tech Univ Berlin, Zentrum Astron & Astrophys, D-10623 Berlin, Germany

[22] Kyoto Univ, Astron Observ, Sakyo Ku, Kyoto 6068502, Japan

[23] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA

[24] CALTECH, Jet Prop Lab, NASA, Pasadena, CA 91125 USA

[25] Univ Calif Los Angeles, Los Angeles, CA USA

[26] Univ Delaware, Newark, DE 19716 USA

[27] Trinity Coll Dublin, Dublin, Ireland

[28] NASA Headquarters, Washington, DC USA

[29] Kyoto Univ, Grad Sch Adv Integrated Studies Human Survivabil, Kyoto, Japan

[30] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[31] Johns Hopkins Univ, Baltimore, MD 21218 USA

来源：

INTERNATIONAL JOURNAL OF ASTROBIOLOGY | 2020年 / 19卷 / 02期

关键词：

astrobiology; atmospheres; biosignatures; chemistry; CME; exoplanets; flares; habitability; internal dynamics; magnetic field; SEP; space weather; stars; Sun; EARTH-LIKE PLANETS; CORONAL MASS EJECTIONS; SOLAR-WIND INTERACTION; X-RAY-EMISSION; PARTICLE-PRECIPITATION EVENTS; PLATE-TECTONICS; MIDDLE ATMOSPHERE; MAGNETIC-FIELDS; SUPER-EARTHS; THERMAL EVOLUTION;

D O I：

10.1017/S1473550419000132

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The search for life in the Universe is a fundamental problem of astrobiology and modern science. The current progress in the detection of terrestrial-type exoplanets has opened a new avenue in the characterization of exoplanetary atmospheres and in the search for biosignatures of life with the upcoming ground-based and space missions. To specify the conditions favourable for the origin, development and sustainment of life as we know it in other worlds, we need to understand the nature of global (astrospheric), and local (atmospheric and surface) environments of exoplanets in the habitable zones (HZs) around G-K-M dwarf stars including our young Sun. Global environment is formed by propagated disturbances from the planet-hosting stars in the form of stellar flares, coronal mass ejections, energetic particles and winds collectively known as astrospheric space weather. Its characterization will help in understanding how an exoplanetary ecosystem interacts with its host star, as well as in the specification of the physical, chemical and biochemical conditions that can create favourable and/or detrimental conditions for planetary climate and habitability along with evolution of planetary internal dynamics over geological timescales. A key linkage of (astro)physical, chemical and geological processes can only be understood in the framework of interdisciplinary studies with the incorporation of progress in heliophysics, astrophysics, planetary and Earth sciences. The assessment of the impacts of host stars on the climate and habitability of terrestrial (exo)planets will significantly expand the current definition of the HZ to the biogenic zone and provide new observational strategies for searching for signatures of life. The major goal of this paper is to describe and discuss the current status and recent progress in this interdisciplinary field in light of presentations and discussions during the NASA Nexus for Exoplanetary System Science funded workshop 'Exoplanetary Space Weather, Climate and Habitability' and to provide a new roadmap for the future development of the emerging field of exoplanetary science and astrobiology.

引用

页码：136 / 194

页数：59

共 606 条

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