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Linking the formation and fate of exo-Kuiper belts within Solar system analogues
Veras, Dimitri1,2; Reichert, Katja3; Dotti, Francesco Flammini4,5; Cai, Maxwell X.6,7; Mustill, Alexander J.8; Shannon, Andrew9; McDonald, Catriona H.1,2; Zwart, Simon Portegies7; Kouwenhoven, M. B. N.4; Spurzem, Rainer3,10,11,12
2020-04-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume493Issue:4Pages:5062-5078
AbstractEscalating observations of exo-minor planets and their destroyed remnants both passing through the Solar system and within white dwarf planetary systems motivate an understanding of the orbital history and fate of exo-Kuiper belts and planetesimal discs. Here, we explore how the structure of a 40-1000 au annulus of planetesimals orbiting inside of a Solar system analogue that is itself initially embedded within a stellar cluster environment varies as the star evolves through all of its stellar phases. We attempt this computationally challenging link in four parts: (1) by performing stellar cluster simulations lasting 100 Myr, (2) by making assumptions about the subsequent quiescent 11 Gyr main-sequence evolution, (3) by performing simulations throughout the giant branch phases of evolution, and (4) by making assumptions about the belt's evolution during the white dwarf phase. Throughout these stages, we estimate the planetesimals' gravitational responses to analogues of the four Solar system giant planets, as well as to collisional grinding, Galactic tides, stellar flybys, and stellar radiation. We find that the imprint of stellar cluster dynamics on the architecture of greater than or similar to 100 kmsized exo-Kuiper belt planetesimals is retained throughout all phases of stellar evolution unless violent gravitational instabilities are triggered either (1) amongst the giant planets, or (2) due to a close (<< 10(3) au) stellar flyby. In the absence of these instabilities, these minor planets simply double their semimajor axis while retaining their primordial post-cluster eccentricity and inclination distributions, with implications for the free-floating planetesimal population and metal-polluted white dwarfs.
KeywordKuiper belt: general minor planets, asteroids: general planets and satellites: dynamical evolution and stability stars: evolution stars: formation white dwarfs
Funding OrganizationSTFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation ; STFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation ; STFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation ; STFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation
DOI10.1093/mnras/staa559
WOS KeywordMAIN-SEQUENCE EVOLUTION ; STELLAR MASS-LOSS ; YORP BREAK-UP ; WHITE-DWARF ; PLANETARY SYSTEMS ; STAR-CLUSTERS ; COLLISIONAL EVOLUTION ; DEBRIS DISC ; OORT CLOUD ; EXTERNAL PHOTOEVAPORATION
Language英语
Funding ProjectSTFC[ST/P003850/1] ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets'[SP 345/20-1] ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU)[RDF-16-01-16] ; National Natural Science Foundation of China[11673032] ; National Natural Science Foundation of China[11573004] ; Knut and Alice Wallenberg Foundation[2014.0017] ; Swedish Research Council[2017-04945] ; European Research Council under the European Community[669416] ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation[84678/84680]
Funding OrganizationSTFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation ; STFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation ; STFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation ; STFC ; STFC ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; DFG priority program SPP 1992 `Exploring the Diversity of Extrasolar Planets' ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; Research Development Fund of Xi'an Jiaotong-Liverpool University (XJTLU) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Knut and Alice Wallenberg Foundation ; Knut and Alice Wallenberg Foundation ; Swedish Research Council ; Swedish Research Council ; European Research Council under the European Community ; European Research Council under the European Community ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; National Astronomical Observatories of Chinese Academy of Sciences, Silk Road Project ; Volkswagen Foundation ; Volkswagen Foundation
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000539094400035
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/83090
Collection中国科学院国家天文台
Corresponding AuthorVeras, Dimitri
Affiliation1.Univ Warwick, Ctr Exoplanets & Habitabil, Coventry CV4 7AL, W Midlands, England
2.Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
3.Heidelberg Univ, Astron Rechen Inst, Zentrum Astron, Monchhofstr 12-14, D-69120 Heidelberg, Germany
4.Xian Jiaotong Liverpool Univ, Sch Sci, Dept Phys, 111 Renai Rd, Suzhou 215123, Peoples R China
5.Univ Liverpool, Dept Math Sci, Liverpool L69 3BX, Merseyside, England
6.SURFsara, Sci Pk 140, NL-1098 XG Amsterdam, Netherlands
7.Leiden Univ, Leiden Observ, Pob 9513, NL-2300 RA Leiden, Netherlands
8.Lund Univ, Lund Observ, Dept Astron & Theoret Phys, Box 43, SE-22100 Lund, Sweden
9.Univ PSL, LESIA, Observ Paris, CNRS,Sorbonne Univ,Univ Paris, 5 Pl Jules Janssen, F-92195 Meudon, France
10.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100101, Peoples R China
11.Chinese Acad Sci, Key Lab Computat Astrophys, 20A Datun Rd, Beijing 100101, Peoples R China
12.Peking Univ, Kavli Inst Astron & Astrophys, Yiheyuan Lu 5, Beijing 100871, Peoples R China
Recommended Citation
GB/T 7714
Veras, Dimitri,Reichert, Katja,Dotti, Francesco Flammini,et al. Linking the formation and fate of exo-Kuiper belts within Solar system analogues[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,493(4):5062-5078.
APA Veras, Dimitri.,Reichert, Katja.,Dotti, Francesco Flammini.,Cai, Maxwell X..,Mustill, Alexander J..,...&Spurzem, Rainer.(2020).Linking the formation and fate of exo-Kuiper belts within Solar system analogues.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,493(4),5062-5078.
MLA Veras, Dimitri,et al."Linking the formation and fate of exo-Kuiper belts within Solar system analogues".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 493.4(2020):5062-5078.
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