國立高雄大學圖資館 |

語系: 繁體中文

說明(常見問題)

圖資館首頁

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Planetary giant impactssimulating co...

Kegerreis, Jacob.

Planetary giant impactssimulating collisions and their consequences /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Planetary giant impactsby Jacob Kegerreis.
其他題名:	simulating collisions and their consequences /
作者:	Kegerreis, Jacob.
出版者:	Cham :Springer International Publishing :2020.
面頁冊數:	xxiii, 125 p. :ill., digital ;24 cm.
Contained By:	Springer Nature eBook
標題:	Collisions (Astrophysics)Computer simulation.
電子資源:	https://doi.org/10.1007/978-3-030-49958-7
ISBN:	9783030499587$q(electronic bk.)

Planetary giant impactssimulating collisions and their consequences /
Kegerreis, Jacob.

Planetary giant impactssimulating collisions and their consequences /[electronic resource] :by Jacob Kegerreis. - Cham :Springer International Publishing :2020. - xxiii, 125 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Methods -- Uranus Giant Impacts and Convergence -- Atmospheric Erosion -- The Lunar Argon Exosphere -- Conclusions.

Based on 3D smoothed particle hydrodynamics simulations performed with unprecedented high resolution, this book examines the giant impacts that dominate many planets' late accretion and evolution. The numerical methods developed are now publicly available, greatly facilitating future studies of planetary impacts in our solar system and exoplanetary systems. The book focuses on four main topics: (1) The development of new methods to construct initial conditions as well as a hydrodynamical simulation code to evolve them, using 1000 times more simulation particles than the previous standard. (2) The numerical convergence of giant impact simulations -- standard-resolution simulations fail to converge on even bulk properties like the post-impact rotation period. (3) The collision thought to have knocked over the planet Uranus causing it to spin on its side. (4) The erosion of atmospheres by giant impacts onto terrestrial planets, and the first full 3D simulations of collisions in this regime.

ISBN: 9783030499587$q(electronic bk.)

Standard No.: 10.1007/978-3-030-49958-7doiSubjects--Topical Terms:

874650
Collisions (Astrophysics)
--Computer simulation.

LC Class. No.: QB466.C64 / K444 2020

Dewey Class. No.: 523.2

Planetary giant impactssimulating collisions and their consequences /
LDR:02175nmm a2200337 a 4500 001 583869
003 DE-He213
005 20201125160109.0
006 m d
007 cr nn 008maaau
008 210202s2020 sz s 0 eng d
020 $a 9783030499587$q(electronic bk.)
020 $a 9783030499570$q(paper)
024 7 $a 10.1007/978-3-030-49958-7 $2 doi
035 $a 978-3-030-49958-7
040 $a GP $c GP
041 0 $a eng
050 4 $a QB466.C64 $b K444 2020
072 7 $a PG $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PGC $2 thema
082 0 4 $a 523.2 $2 23
090 $a QB466.C64 $b K26 2020
100 1 $a Kegerreis, Jacob. $3 874649
245 1 0 $a Planetary giant impacts $h [electronic resource] : $b simulating collisions and their consequences / $c by Jacob Kegerreis.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2020.
300 $a xxiii, 125 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Methods -- Uranus Giant Impacts and Convergence -- Atmospheric Erosion -- The Lunar Argon Exosphere -- Conclusions.
520 $a Based on 3D smoothed particle hydrodynamics simulations performed with unprecedented high resolution, this book examines the giant impacts that dominate many planets' late accretion and evolution. The numerical methods developed are now publicly available, greatly facilitating future studies of planetary impacts in our solar system and exoplanetary systems. The book focuses on four main topics: (1) The development of new methods to construct initial conditions as well as a hydrodynamical simulation code to evolve them, using 1000 times more simulation particles than the previous standard. (2) The numerical convergence of giant impact simulations -- standard-resolution simulations fail to converge on even bulk properties like the post-impact rotation period. (3) The collision thought to have knocked over the planet Uranus causing it to spin on its side. (4) The erosion of atmospheres by giant impacts onto terrestrial planets, and the first full 3D simulations of collisions in this regime.
650 0 $a Collisions (Astrophysics) $x Computer simulation. $3 874650
650 1 4 $a Astronomy, Astrophysics and Cosmology. $3 273876
650 2 4 $a Astrophysics and Astroparticles. $3 376943
650 2 4 $a Theoretical, Mathematical and Computational Physics. $3 376743
710 2 $a SpringerLink (Online service) $3 273601
773 0 $t Springer Nature eBook
830 0 $a Springer theses. $3 557607
856 4 0 $u https://doi.org/10.1007/978-3-030-49958-7
950 $a Physics and Astronomy (SpringerNature-11651)