國立虎尾科技大學 |

Host Stars and their Effects on Exoplanet Atmospheres = An Introductory Overview /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Host Stars and their Effects on Exoplanet Atmospheres / by Jeffrey Linsky.
其他題名:	An Introductory Overview /
作者:	Linsky, Jeffrey.
面頁冊數:	X, 273 p. 143 illus., 104 illus. in color.online resource. :
Contained By:	Springer Nature eBook
標題:	Planetary science. -
電子資源:	https://doi.org/10.1007/978-3-030-11452-7
ISBN:	9783030114527

Host Stars and their Effects on Exoplanet Atmospheres = An Introductory Overview /
Linsky, Jeffrey.

Host Stars and their Effects on Exoplanet Atmospheres An Introductory Overview /[electronic resource] :by Jeffrey Linsky. - 1st ed. 2019. - X, 273 p. 143 illus., 104 illus. in color.online resource. - Lecture Notes in Physics,9550075-8450 ;. - Lecture Notes in Physics,891.

Why are Host Stars Important for Understanding Exoplanet Atmospheres? -- Stellar activity–phenomenology and general principles -- Magnetic Fields–the Source of Stellar Activity -- Stellar Chromospheres–the Source of UV Emission -- Stellar Coronae–the Source of X-ray Emission -- Reconstructing the Missing Stellar Emission -- Stellar Winds -- Correlations of Observables with Stellar Age and Rotation -- Stellar Space Weather–Connecting Host Stars to Their Exoplanets - Host Star Driven Exoplanet Mass Loss -- Host Star Driven Photochemistry in Exoplanet Atmospheres -- Star-Planet Interactions (SPI)–Real or Imaginary? -- Final Comments and Speculation.

Like planets in our solar system, exoplanets form, evolve, and interact with their host stars in many ways. As exoplanets acquire material and grow to the final size, their atmospheres are subjected to intense UV and X-radiation and high-energy particle bombardment from the young host star. Whether a planet can retain its atmosphere and the conditions for significant mass loss both depend upon the strength of the host star's high-energy radiation and wind, the distance of the exoplanet from its host star, the gravitational potential of the exoplanet, and the initial chemical composition of the exoplanet atmosphere. This introductory overview describes the physical processes responsible for the emission of radiation and acceleration of winds of host stars that together control the environment of an exoplanet, focusing on topics that are critically important for understanding exoplanetary atmospheres but are usually not posed from the perspective of host stars. Accordingly, both host stars and exoplanets are not studied in isolation but are treated as integrated systems. Stellar magnetic fields, which are the energy source for activity phenomena including high-energy radiation and winds, play a critical role in determining whether exoplanets are habitable. This text is primarily for researchers and graduate students who are studying exoplanet atmospheres and habitability, but who may not have a background in the physics and phenomenology of host stars that provide the environment in which exoplanets evolve. It provides a comprehensive overview of this broad topic rather than going deeply into many technical aspects but includes a large list of references to guide those interested in pursuing these questions. Nonspecialists with a scientific background should also find this text a valuable resource for understanding the critical issues of contemporary exoplanet research.

ISBN: 9783030114527

Standard No.: 10.1007/978-3-030-11452-7doiSubjects--Topical Terms:

1069474
Planetary science.

LC Class. No.: QB600-701

Dewey Class. No.: 523.2

Host Stars and their Effects on Exoplanet Atmospheres = An Introductory Overview /
LDR:03983nam a22004095i 4500 001 1014895
003 DE-He213
005 20200704060520.0
007 cr nn 008mamaa
008 210106s2019 gw | s |||| 0|eng d
020 $a 9783030114527 $9 978-3-030-11452-7
024 7 $a 10.1007/978-3-030-11452-7 $2 doi
035 $a 978-3-030-11452-7
050 4 $a QB600-701
072 7 $a PGS $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGS $2 thema
082 0 4 $a 523.2 $2 23
100 1 $a Linsky, Jeffrey. $4 aut $4 http://id.loc.gov/vocabulary/relators/aut $3 1227579
245 1 0 $a Host Stars and their Effects on Exoplanet Atmospheres $h [electronic resource] : $b An Introductory Overview / $c by Jeffrey Linsky.
250 $a 1st ed. 2019.
264 1 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2019.
300 $a X, 273 p. 143 illus., 104 illus. in color. $b online resource.
336 $a text $b txt $2 rdacontent
337 $a computer $b c $2 rdamedia
338 $a online resource $b cr $2 rdacarrier
347 $a text file $b PDF $2 rda
490 1 $a Lecture Notes in Physics, $x 0075-8450 ; $v 955
505 0 $a Why are Host Stars Important for Understanding Exoplanet Atmospheres? -- Stellar activity–phenomenology and general principles -- Magnetic Fields–the Source of Stellar Activity -- Stellar Chromospheres–the Source of UV Emission -- Stellar Coronae–the Source of X-ray Emission -- Reconstructing the Missing Stellar Emission -- Stellar Winds -- Correlations of Observables with Stellar Age and Rotation -- Stellar Space Weather–Connecting Host Stars to Their Exoplanets - Host Star Driven Exoplanet Mass Loss -- Host Star Driven Photochemistry in Exoplanet Atmospheres -- Star-Planet Interactions (SPI)–Real or Imaginary? -- Final Comments and Speculation.
520 $a Like planets in our solar system, exoplanets form, evolve, and interact with their host stars in many ways. As exoplanets acquire material and grow to the final size, their atmospheres are subjected to intense UV and X-radiation and high-energy particle bombardment from the young host star. Whether a planet can retain its atmosphere and the conditions for significant mass loss both depend upon the strength of the host star's high-energy radiation and wind, the distance of the exoplanet from its host star, the gravitational potential of the exoplanet, and the initial chemical composition of the exoplanet atmosphere. This introductory overview describes the physical processes responsible for the emission of radiation and acceleration of winds of host stars that together control the environment of an exoplanet, focusing on topics that are critically important for understanding exoplanetary atmospheres but are usually not posed from the perspective of host stars. Accordingly, both host stars and exoplanets are not studied in isolation but are treated as integrated systems. Stellar magnetic fields, which are the energy source for activity phenomena including high-energy radiation and winds, play a critical role in determining whether exoplanets are habitable. This text is primarily for researchers and graduate students who are studying exoplanet atmospheres and habitability, but who may not have a background in the physics and phenomenology of host stars that provide the environment in which exoplanets evolve. It provides a comprehensive overview of this broad topic rather than going deeply into many technical aspects but includes a large list of references to guide those interested in pursuing these questions. Nonspecialists with a scientific background should also find this text a valuable resource for understanding the critical issues of contemporary exoplanet research.
650 0 $a Planetary science. $3 1069474
650 0 $a Astrobiology. $3 672804
650 0 $a Atmospheric sciences. $3 1179392
650 0 $a Planetology. $3 593937
650 0 $a Solar system. $3 897437
650 0 $a Space sciences. $3 715034
650 1 4 $a Planetary Sciences. $3 1141894
650 2 4 $a Atmospheric Sciences. $3 881331
650 2 4 $a Solar and Heliospheric Physics . $3 1227580
650 2 4 $a Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). $3 1114976
710 2 $a SpringerLink (Online service) $3 593884
773 0 $t Springer Nature eBook
776 0 8 $i Printed edition: $z 9783030114510
776 0 8 $i Printed edition: $z 9783030114534
830 0 $a Lecture Notes in Physics, $x 0075-8450 ; $v 891 $3 1253935
856 4 0 $u https://doi.org/10.1007/978-3-030-11452-7
912 $a ZDB-2-PHA
912 $a ZDB-2-SXP
912 $a ZDB-2-LNP
950 $a Physics and Astronomy (SpringerNature-11651)
950 $a Physics and Astronomy (R0) (SpringerNature-43715)