Is There an Earth-like Planet in the Distant Kuiper Belt?

The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N -body computer simulations to investigate the effects of a hypothetical Kuiper Belt planet (KBP) on the orbital structure of TNOs in the distant Kuiper Belt bey...

Celý popis

Uloženo v:
Podrobná bibliografie
Vydáno v:The Astronomical journal Ročník 166; číslo 3; s. 118 - 137
Hlavní autoři: Lykawka, Patryk Sofia, Ito, Takashi
Médium: Journal Article
Jazyk:angličtina
Vydáno: Madison The American Astronomical Society 01.09.2023
IOP Publishing
Témata:
Astronomy
Detached objects
Earth
Gravitational effects
Gravity effects
Kuiper belt
Neptune
Orbital resonances (celestial mechanics)
Orbits
Outer solar system
Perihelions
Perturbation
Planets
Resonant Kuiper belt objects
Scattered disk objects
Solar system
Solar system planets
Terrestrial planets
Trans-Neptunian objects
ISSN:0004-6256, 1538-3881
On-line přístup:Získat plný text
Tagy: Přidat tag
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!
Abstract The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N -body computer simulations to investigate the effects of a hypothetical Kuiper Belt planet (KBP) on the orbital structure of TNOs in the distant Kuiper Belt beyond ∼50 au. We used observations to constrain model results, including the well-characterized Outer Solar System Origins Survey (OSSOS). We determined that an Earth-like planet ( m ∼ 1.5–3 M ⊕ ) located on a distant (semimajor axis a ∼ 250–500 au, perihelion q ∼ 200 au) and inclined ( i ∼ 30°) orbit can explain three fundamental properties of the distant Kuiper Belt: a prominent population of TNOs with orbits beyond Neptune’s gravitational influence (i.e., detached objects with q > 40 au), a significant population of high- i objects ( i > 45°), and the existence of some extreme objects with peculiar orbits (e.g., Sedna). Furthermore, the proposed KBP is compatible with the existence of identified gigayear-stable TNOs in the 2:1, 5:2, 3:1, 4:1, 5:1, and 6:1 Neptunian mean motion resonances. These stable populations are often neglected in other studies. We predict the existence of an Earth-like planet and several TNOs on peculiar orbits in the outer solar system, which can serve as observationally testable signatures of the putative planet’s perturbations.
AbstractList The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N-body computer simulations to investigate the effects of a hypothetical Kuiper Belt planet (KBP) on the orbital structure of TNOs in the distant Kuiper Belt beyond ∼50 au. We used observations to constrain model results, including the well-characterized Outer Solar System Origins Survey (OSSOS). We determined that an Earth-like planet (m ∼ 1.5–3 M⊕) located on a distant (semimajor axis a ∼ 250–500 au, perihelion q ∼ 200 au) and inclined (i ∼ 30°) orbit can explain three fundamental properties of the distant Kuiper Belt: a prominent population of TNOs with orbits beyond Neptune’s gravitational influence (i.e., detached objects with q > 40 au), a significant population of high-i objects (i > 45°), and the existence of some extreme objects with peculiar orbits (e.g., Sedna). Furthermore, the proposed KBP is compatible with the existence of identified gigayear-stable TNOs in the 2:1, 5:2, 3:1, 4:1, 5:1, and 6:1 Neptunian mean motion resonances. These stable populations are often neglected in other studies. We predict the existence of an Earth-like planet and several TNOs on peculiar orbits in the outer solar system, which can serve as observationally testable signatures of the putative planet’s perturbations.
The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N -body computer simulations to investigate the effects of a hypothetical Kuiper Belt planet (KBP) on the orbital structure of TNOs in the distant Kuiper Belt beyond ∼50 au. We used observations to constrain model results, including the well-characterized Outer Solar System Origins Survey (OSSOS). We determined that an Earth-like planet ( m ∼ 1.5–3 M _⊕ ) located on a distant (semimajor axis a ∼ 250–500 au, perihelion q ∼ 200 au) and inclined ( i ∼ 30°) orbit can explain three fundamental properties of the distant Kuiper Belt: a prominent population of TNOs with orbits beyond Neptune’s gravitational influence (i.e., detached objects with q > 40 au), a significant population of high- i objects ( i > 45°), and the existence of some extreme objects with peculiar orbits (e.g., Sedna). Furthermore, the proposed KBP is compatible with the existence of identified gigayear-stable TNOs in the 2:1, 5:2, 3:1, 4:1, 5:1, and 6:1 Neptunian mean motion resonances. These stable populations are often neglected in other studies. We predict the existence of an Earth-like planet and several TNOs on peculiar orbits in the outer solar system, which can serve as observationally testable signatures of the putative planet’s perturbations.
The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N -body computer simulations to investigate the effects of a hypothetical Kuiper Belt planet (KBP) on the orbital structure of TNOs in the distant Kuiper Belt beyond ∼50 au. We used observations to constrain model results, including the well-characterized Outer Solar System Origins Survey (OSSOS). We determined that an Earth-like planet ( m ∼ 1.5–3 M ⊕ ) located on a distant (semimajor axis a ∼ 250–500 au, perihelion q ∼ 200 au) and inclined ( i ∼ 30°) orbit can explain three fundamental properties of the distant Kuiper Belt: a prominent population of TNOs with orbits beyond Neptune’s gravitational influence (i.e., detached objects with q > 40 au), a significant population of high- i objects ( i > 45°), and the existence of some extreme objects with peculiar orbits (e.g., Sedna). Furthermore, the proposed KBP is compatible with the existence of identified gigayear-stable TNOs in the 2:1, 5:2, 3:1, 4:1, 5:1, and 6:1 Neptunian mean motion resonances. These stable populations are often neglected in other studies. We predict the existence of an Earth-like planet and several TNOs on peculiar orbits in the outer solar system, which can serve as observationally testable signatures of the putative planet’s perturbations.
Author Ito, Takashi
Lykawka, Patryk Sofia
Author_xml – sequence: 1
  givenname: Patryk Sofia
  orcidid: 0000-0003-0926-2448
  surname: Lykawka
  fullname: Lykawka, Patryk Sofia
  organization: Kindai University , Shinkamikosaka 228-3, Higashiosaka, Osaka, 577-0813, Japan
– sequence: 2
  givenname: Takashi
  orcidid: 0000-0002-0549-9002
  surname: Ito
  fullname: Ito, Takashi
  organization: Planetary Exploration Research Center , Chiba Institute of Technology, 2-17-1 Tsudanuma, Narashino, 275-0016, Chiba, Japan
BookMark eNp9kc1v1DAQxS3USmxb7hwtwZHQccYfyQlBKbCiUnsoZ8txxqyXEAfHe-C_J0v4kBDqaaSn956efnPGTsY0EmNPBbzERppLobCpsGnEpfPkAjximz_SCdsAgKx0rfRjdjbPewAhGpAb1m5nfr-jTNyN_NrlsquG-IX43eBGKjyOvOyIv41zcWPhHw9xoszf0FBeXbDT4IaZnvy65-zTu-v7qw_Vze377dXrm8pLqUpFWvUdGqUEQA0SHCAqHaAOndR926pggjChVtK1hCYY7DpfByUF1t4bh-dsu_b2ye3tlONXl7_b5KL9KaT82S6zox_ISiJTY5Ad-l72jlroBGFvNKDsWxRL17O1a8rp24HmYvfpkMdlvq0bZSS2DTaLS68un9M8ZwrWx-JKTGPJLg5WgD0it0e-9sjXrsiXIPwT_D33gciLNRLT9HfMA_bn_7EvGITWFu3yVDv1AX8A2TCd9Q
CitedBy_id crossref_primary_10_1093_mnrasl_slaf091
crossref_primary_10_55064_tjaa_1597866
crossref_primary_10_3847_PSJ_addd03
crossref_primary_10_1134_S1063772923110057
crossref_primary_10_3847_1538_3881_ad8dd9
crossref_primary_10_3847_1538_3881_add3ec
crossref_primary_10_3847_2041_8213_ad13eb
crossref_primary_10_3847_1538_4357_ad98f6
crossref_primary_10_3847_2041_8213_ad2686
crossref_primary_10_1038_s41550_025_02595_7
crossref_primary_10_1016_j_icarus_2025_116733
Cites_doi 10.3847/1538-3881/ac2056
10.3847/1538-3881/aad042
10.1088/0004-6256/150/3/73
10.1093/mnras/stu2374
10.1088/2041-8205/744/1/L3
10.1088/0004-6256/135/4/1161
10.3847/1538-3881/aa5be9
10.3847/1538-4365/aab77a
10.1016/j.icarus.2005.11.011
10.1146/annurev-astro-081817-052028
10.1093/mnras/sty1930
10.3847/1538-3881/aab8ff
10.3847/PSJ/acc7a2
10.1016/j.icarus.2020.114122
10.3389/fspas.2017.00028
10.1016/j.physrep.2019.01.009
10.1007/s10569-004-4623-y
10.3847/1538-3881/aa7aed
10.48550/arXiv.1911.03984
10.1038/nature13156
10.1126/science.1238072
10.1088/0004-637X/697/2/L91
10.3847/1538-3881/ab2639
10.3847/1538-4365/ac3914
10.1093/mnrasl/slu084
10.3847/1538-3881/ab2383
10.3847/1538-3881/aac6cd
10.1088/0004-6256/144/1/23
10.1016/C2018-0-00549-6
10.3847/1538-4357/aa7cf6
10.1016/j.icarus.2006.04.001
10.3847/PSJ/ac67e0
10.1016/j.icarus.2006.10.002
10.3847/2041-8213/ac90b9
10.3847/0004-637X/825/2/94
10.3847/1538-3881/153/1/33
10.3847/1538-4357/ac19a4
10.1186/s40562-019-0142-2
10.1016/j.icarus.2007.06.007
10.1146/annurev-astro-120920-010005
10.3847/0004-6256/152/5/133
10.1086/424617
10.1088/2041-8205/742/2/L22
10.1086/452638
10.3847/1538-3881/aa8b65
10.1088/2041-8205/764/1/L2
10.1086/422095
10.1016/j.icarus.2011.07.037
10.3847/1538-3881/ab24e1
10.3847/1538-3881/aa6aa5
10.3847/1538-3881/ab1c4c
10.1016/j.pss.2005.10.006
10.3847/1538-3881/ab0895
10.1093/mnrasl/slx106
10.48550/arXiv.1212.6124
10.1046/j.1365-8711.1999.02379.x
10.1051/0004-6361/201118541
10.3847/0004-6256/152/5/111
10.3847/1538-3881/ab98fb
10.1051/0004-6361/202037919
10.1088/0004-6256/150/3/68
10.3847/1538-3881/152/6/221
10.3847/1538-3881/aac268
10.3847/2041-8205/825/1/L13
10.3847/0004-6256/151/2/22
10.1086/505214
10.1016/j.icarus.2013.03.012
10.1111/j.1365-2966.2011.20264.x
10.3847/1538-3881/153/2/63
10.1016/S0019-1035(02)00056-8
10.1088/0004-6256/142/4/131
10.3847/0004-6256/151/2/31
10.3847/PSJ/abe53e
10.1016/j.icarus.2007.01.001
10.1051/0004-6361/201218874
10.1051/0004-6361/201936183
10.3847/2041-8205/827/2/L24
10.3389/fspas.2018.00014
10.3847/1538-3881/aaa19b
10.3847/0004-6256/152/3/70
10.3847/1538-3881/aa6db5
10.1051/0004-6361/201322041
10.1086/117532
10.3847/2041-8205/827/2/L35
10.1006/icar.2002.6860
10.3847/1538-3881/aa79ff
10.3847/2041-8213/ac9480
ContentType Journal Article
Copyright 2023. The Author(s). Published by the American Astronomical Society.
2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
Copyright_xml – notice: 2023. The Author(s). Published by the American Astronomical Society.
– notice: 2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
DBID O3W
TSCCA
AAYXX
CITATION
7TG
8FD
H8D
KL.
L7M
DOA
DOI 10.3847/1538-3881/aceaf0
DatabaseName Institute of Physics Open Access Journal Titles
IOPscience (Open Access)
CrossRef
Meteorological & Geoastrophysical Abstracts
Technology Research Database
Aerospace Database
Meteorological & Geoastrophysical Abstracts - Academic
Advanced Technologies Database with Aerospace
Directory of Open Access Journals (DOAJ) (Open Access)
DatabaseTitle CrossRef
Aerospace Database
Meteorological & Geoastrophysical Abstracts
Technology Research Database
Advanced Technologies Database with Aerospace
Meteorological & Geoastrophysical Abstracts - Academic
DatabaseTitleList Aerospace Database

CrossRef
Database_xml – sequence: 1
  dbid: DOA
  name: DOAJ Open Access Full Text
  url: https://www.doaj.org/
  sourceTypes: Open Website
– sequence: 2
  dbid: O3W
  name: Institute of Physics Open Access Journal Titles
  url: http://iopscience.iop.org/
  sourceTypes:
    Enrichment Source
    Publisher
DeliveryMethod fulltext_linktorsrc
Discipline Astronomy & Astrophysics
EISSN 1538-3881
ExternalDocumentID oai_doaj_org_article_4ee723f4b3cd4dae90b1e3d76034d931
10_3847_1538_3881_aceaf0
ajaceaf0
GrantInformation_xml – fundername: MEXT ∣ Japan Society for the Promotion of Science (JSPS)
  grantid: JP20K04049
  funderid: https://doi.org/10.13039/501100001691
GroupedDBID -DZ
-~X
123
1JI
23N
4.4
6J9
85S
AAFWJ
AAGCD
AAJIO
ABDNZ
ABHWH
ABXSS
ACBEA
ACGFS
ACHIP
ACNCT
ACYRX
AEFHF
AENEX
AFPKN
AGNAY
AHPAA
AKPSB
ALMA_UNASSIGNED_HOLDINGS
ASPBG
ATQHT
AVWKF
AZFZN
CJUJL
CRLBU
CS3
EBS
F5P
FRP
GROUPED_DOAJ
HF~
IJHAN
IOP
KOT
N5L
O3W
O43
OK1
P2P
PJBAE
RIN
RNP
RNS
ROL
SY9
T37
TR2
TSCCA
UPT
WH7
~02
AAYXX
AEINN
CITATION
7TG
8FD
H8D
KL.
L7M
ID FETCH-LOGICAL-c445t-e65db37551002040a03356f02fb46d995f7f17f254a9e37f73bbc2f54132cc7a3
IEDL.DBID O3W
ISICitedReferencesCount 12
ISICitedReferencesURI http://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=Summon&SrcAuth=ProQuest&DestLinkType=CitingArticles&DestApp=WOS_CPL&KeyUT=001054312700001&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D
ISSN 0004-6256
IngestDate Fri Oct 03 12:52:11 EDT 2025
Wed Aug 13 07:20:16 EDT 2025
Sat Nov 29 05:29:56 EST 2025
Tue Nov 18 21:52:32 EST 2025
Tue Oct 03 22:40:25 EDT 2023
Wed Aug 21 03:40:42 EDT 2024
IsDoiOpenAccess true
IsOpenAccess true
IsPeerReviewed true
IsScholarly true
Issue 3
Language English
License Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c445t-e65db37551002040a03356f02fb46d995f7f17f254a9e37f73bbc2f54132cc7a3
Notes AAS43969
The Solar System, Exoplanets, and Astrobiology
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 14
ORCID 0000-0003-0926-2448
0000-0002-0549-9002
OpenAccessLink https://iopscience.iop.org/article/10.3847/1538-3881/aceaf0
PQID 2857439838
PQPubID 4562438
PageCount 20
ParticipantIDs proquest_journals_2857439838
iop_journals_10_3847_1538_3881_aceaf0
crossref_citationtrail_10_3847_1538_3881_aceaf0
doaj_primary_oai_doaj_org_article_4ee723f4b3cd4dae90b1e3d76034d931
crossref_primary_10_3847_1538_3881_aceaf0
PublicationCentury 2000
PublicationDate 2023-09-01
PublicationDateYYYYMMDD 2023-09-01
PublicationDate_xml – month: 09
  year: 2023
  text: 2023-09-01
  day: 01
PublicationDecade 2020
PublicationPlace Madison
PublicationPlace_xml – name: Madison
PublicationTitle The Astronomical journal
PublicationTitleAbbrev AJ
PublicationTitleAlternate Astron. J
PublicationYear 2023
Publisher The American Astronomical Society
IOP Publishing
Publisher_xml – name: The American Astronomical Society
– name: IOP Publishing
References Gallardo (ajaceaf0bib28) 2006a; 181
Brasser (ajaceaf0bib14) 2013; 225
Gomes (ajaceaf0bib38) 2008
Batygin (ajaceaf0bib9) 2021; 920
de la Fuente Marcos (ajaceaf0bib24) 2014; 443
Shankman (ajaceaf0bib82) 2017b; 153
Malhotra (ajaceaf0bib60) 1995; 110
Yu (ajaceaf0bib94) 2018; 156
Lykawka (ajaceaf0bib55) 2007a; 186
Hahn (ajaceaf0bib40) 2005; 130
Brasil (ajaceaf0bib13) 2014; 564
Lawler (ajaceaf0bib52) 2018b; 155
Lykawka (ajaceaf0bib56) 2007b; 189
Chen (ajaceaf0bib20) 2022; 937
Iorio (ajaceaf0bib42) 2017; 4
Becker (ajaceaf0bib11) 2018; 156
Kavelaars (ajaceaf0bib48) 2020; Vol. 463
Nesvorny (ajaceaf0bib69) 2020; 160
Kaib (ajaceaf0bib44) 2019; 158
Beaudoin (ajaceaf0bib10) 2023
Ito (ajaceaf0bib43) 2019; 7
Santos-Sanz (ajaceaf0bib78) 2012; 541
Shannon (ajaceaf0bib83) 2018; 480
Kaib (ajaceaf0bib47) 2023
Shankman (ajaceaf0bib80) 2017a; 154
Bannister (ajaceaf0bib4) 2016; 152
Shankman (ajaceaf0bib79) 2013; 764
Volk (ajaceaf0bib92) 2019; 158
Huang (ajaceaf0bib41) 2022; 938
Nesvorny (ajaceaf0bib65) 2015a; 150
Crompvoets (ajaceaf0bib23) 2022; 3
Bannister (ajaceaf0bib3) 2018; 236
Gladman (ajaceaf0bib34) 2008
Lawler (ajaceaf0bib51) 2017; 153
Brown (ajaceaf0bib18) 2004; 617
Malhotra (ajaceaf0bib61) 2018
Napier (ajaceaf0bib63) 2021; 2
Petit (ajaceaf0bib74) 2017; 153
Chambers (ajaceaf0bib19) 1999; 304
Gomes (ajaceaf0bib36) 2023; 4
Lykawka (ajaceaf0bib57) 2007c; 192
Gladman (ajaceaf0bib32) 2009; 697
Trujillo (ajaceaf0bib89) 2014; 507
Prialnik (ajaceaf0bib77) 2020
Sheppard (ajaceaf0bib84) 2016; 152
Morbidelli (ajaceaf0bib62) 2004; 128
Gladman (ajaceaf0bib33) 2012; 144
Alexandersen (ajaceaf0bib2) 2016; 152
Gladman (ajaceaf0bib35) 2021; 59
Kaib (ajaceaf0bib45) 2011; 215
Batygin (ajaceaf0bib7) 2016; 151
Clement (ajaceaf0bib22) 2021; 355
Lykawka (ajaceaf0bib58) 2008; 135
de la Fuente Marcos (ajaceaf0bib25) 2017; 471
Bannister (ajaceaf0bib5) 2017; 153
Alexandersen (ajaceaf0bib1) 2013; 341
Gladman (ajaceaf0bib31) 2002; 157
Nesvorny (ajaceaf0bib66) 2015b; 150
Lykawka (ajaceaf0bib54) 2006; 54
Tremaine (ajaceaf0bib88) 2023
Malhora (ajaceaf0bib59) 2019; 6
Brown (ajaceaf0bib17) 2021; 162
Lawler (ajaceaf0bib50) 2019; 157
Bernardinelli (ajaceaf0bib12) 2022; 258
Brasser (ajaceaf0bib15) 2015; 446
Lykawka (ajaceaf0bib53) 2012; 1
Petit (ajaceaf0bib73) 2011; 142
Sheppard (ajaceaf0bib86) 2019; 157
Volk (ajaceaf0bib91) 2017; 154
Lawler (ajaceaf0bib49) 2018a; 5
Pal (ajaceaf0bib72) 2012; 541
Farkas-Takacs (ajaceaf0bib26) 2020; 638
Sheppard (ajaceaf0bib85) 2016; 825
Volk (ajaceaf0bib93) 2018; 155
Batygin (ajaceaf0bib8) 2012; 744
Nesvorny (ajaceaf0bib67) 2018; 56
Nesvorny (ajaceaf0bib68) 2016; 825
Pike (ajaceaf0bib75) 2017; 153
van Laerhoven (ajaceaf0bib90) 2019; 158
Brasser (ajaceaf0bib16) 2012; 420
Silsbee (ajaceaf0bib87) 2018; 155
Gomes (ajaceaf0bib39) 2005; 91
Shankman (ajaceaf0bib81) 2016; 151
Gladman (ajaceaf0bib30) 2006; 643
Kaib (ajaceaf0bib46) 2016; 152
Nesvorny (ajaceaf0bib70) 2017; 845
Gomes (ajaceaf0bib37) 2003; 161
Chen (ajaceaf0bib21) 2016; 827
Fienga (ajaceaf0bib27) 2020; 640
Nesvorny (ajaceaf0bib71) 2016; 827
Batygin (ajaceaf0bib6) 2019; 805
Pike (ajaceaf0bib76) 2017; 154
Gallardo (ajaceaf0bib29) 2006b; 184
Nesvorny (ajaceaf0bib64) 2011; 742
References_xml – volume: 162
  start-page: 219
  year: 2021
  ident: ajaceaf0bib17
  publication-title: AJ
  doi: 10.3847/1538-3881/ac2056
– volume: 156
  start-page: 81
  year: 2018
  ident: ajaceaf0bib11
  publication-title: AJ
  doi: 10.3847/1538-3881/aad042
– volume: 150
  start-page: 73
  year: 2015b
  ident: ajaceaf0bib66
  publication-title: AJ
  doi: 10.1088/0004-6256/150/3/73
– start-page: 45
  year: 2018
  ident: ajaceaf0bib61
– volume: 446
  start-page: 3788
  year: 2015
  ident: ajaceaf0bib15
  publication-title: MNRAS
  doi: 10.1093/mnras/stu2374
– volume: 744
  start-page: L3
  year: 2012
  ident: ajaceaf0bib8
  publication-title: ApJL
  doi: 10.1088/2041-8205/744/1/L3
– volume: 135
  start-page: 1161
  year: 2008
  ident: ajaceaf0bib58
  publication-title: AJ
  doi: 10.1088/0004-6256/135/4/1161
– volume: 153
  start-page: 127
  year: 2017
  ident: ajaceaf0bib75
  publication-title: AJ
  doi: 10.3847/1538-3881/aa5be9
– volume: 236
  start-page: 18
  year: 2018
  ident: ajaceaf0bib3
  publication-title: ApJS
  doi: 10.3847/1538-4365/aab77a
– volume: 181
  start-page: 205
  year: 2006a
  ident: ajaceaf0bib28
  publication-title: Icar
  doi: 10.1016/j.icarus.2005.11.011
– volume: 56
  start-page: 137
  year: 2018
  ident: ajaceaf0bib67
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-081817-052028
– volume: 480
  start-page: 1870
  year: 2018
  ident: ajaceaf0bib83
  publication-title: MNRAS
  doi: 10.1093/mnras/sty1930
– volume: 155
  start-page: 197
  year: 2018b
  ident: ajaceaf0bib52
  publication-title: AJ
  doi: 10.3847/1538-3881/aab8ff
– volume: 4
  start-page: 66
  year: 2023
  ident: ajaceaf0bib36
  publication-title: PSJ
  doi: 10.3847/PSJ/acc7a2
– volume: 355
  start-page: 114122
  year: 2021
  ident: ajaceaf0bib22
  publication-title: Icar
  doi: 10.1016/j.icarus.2020.114122
– volume: 4
  start-page: 28
  year: 2017
  ident: ajaceaf0bib42
  publication-title: FrASS
  doi: 10.3389/fspas.2017.00028
– volume: 805
  start-page: 1
  year: 2019
  ident: ajaceaf0bib6
  publication-title: PhR
  doi: 10.1016/j.physrep.2019.01.009
– volume: 91
  start-page: 109
  year: 2005
  ident: ajaceaf0bib39
  publication-title: CeMDA
  doi: 10.1007/s10569-004-4623-y
– volume: 154
  start-page: 50
  year: 2017a
  ident: ajaceaf0bib80
  publication-title: AJ
  doi: 10.3847/1538-3881/aa7aed
– volume: 7
  start-page: 1
  year: 2019
  ident: ajaceaf0bib43
  publication-title: MEEP
  doi: 10.48550/arXiv.1911.03984
– volume: 507
  start-page: 471
  year: 2014
  ident: ajaceaf0bib89
  publication-title: Natur
  doi: 10.1038/nature13156
– volume: 341
  start-page: 994
  year: 2013
  ident: ajaceaf0bib1
  publication-title: Sci
  doi: 10.1126/science.1238072
– volume: 697
  start-page: L91
  year: 2009
  ident: ajaceaf0bib32
  publication-title: ApJL
  doi: 10.1088/0004-637X/697/2/L91
– volume: 158
  start-page: 64
  year: 2019
  ident: ajaceaf0bib92
  publication-title: AJ
  doi: 10.3847/1538-3881/ab2639
– volume: 258
  start-page: 41
  year: 2022
  ident: ajaceaf0bib12
  publication-title: ApJS
  doi: 10.3847/1538-4365/ac3914
– volume: 443
  start-page: L59
  year: 2014
  ident: ajaceaf0bib24
  publication-title: MNRASL
  doi: 10.1093/mnrasl/slu084
– volume: 158
  start-page: 43
  year: 2019
  ident: ajaceaf0bib44
  publication-title: AJ
  doi: 10.3847/1538-3881/ab2383
– volume: 156
  start-page: 33
  year: 2018
  ident: ajaceaf0bib94
  publication-title: AJ
  doi: 10.3847/1538-3881/aac6cd
– volume: 144
  start-page: 23
  year: 2012
  ident: ajaceaf0bib33
  publication-title: AJ
  doi: 10.1088/0004-6256/144/1/23
– year: 2020
  ident: ajaceaf0bib77
  doi: 10.1016/C2018-0-00549-6
– volume: 845
  start-page: 27
  year: 2017
  ident: ajaceaf0bib70
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa7cf6
– volume: 184
  start-page: 29
  year: 2006b
  ident: ajaceaf0bib29
  publication-title: Icar
  doi: 10.1016/j.icarus.2006.04.001
– volume: 3
  start-page: 113
  year: 2022
  ident: ajaceaf0bib23
  publication-title: PSJ
  doi: 10.3847/PSJ/ac67e0
– volume: 186
  start-page: 331
  year: 2007a
  ident: ajaceaf0bib55
  publication-title: Icar
  doi: 10.1016/j.icarus.2006.10.002
– volume: 937
  start-page: L22
  year: 2022
  ident: ajaceaf0bib20
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac90b9
– volume: 825
  start-page: 94
  year: 2016
  ident: ajaceaf0bib68
  publication-title: ApJ
  doi: 10.3847/0004-637X/825/2/94
– volume: 153
  start-page: 33
  year: 2017
  ident: ajaceaf0bib51
  publication-title: AJ
  doi: 10.3847/1538-3881/153/1/33
– volume: 920
  start-page: 148
  year: 2021
  ident: ajaceaf0bib9
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac19a4
– volume: 6
  start-page: 12
  year: 2019
  ident: ajaceaf0bib59
  publication-title: GSL
  doi: 10.1186/s40562-019-0142-2
– year: 2023
  ident: ajaceaf0bib88
– volume: 192
  start-page: 238
  year: 2007c
  ident: ajaceaf0bib57
  publication-title: Icar
  doi: 10.1016/j.icarus.2007.06.007
– volume: 59
  start-page: 203
  year: 2021
  ident: ajaceaf0bib35
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-120920-010005
– volume: 152
  start-page: 133
  year: 2016
  ident: ajaceaf0bib46
  publication-title: AJ
  doi: 10.3847/0004-6256/152/5/133
– volume: 128
  start-page: 2564
  year: 2004
  ident: ajaceaf0bib62
  publication-title: AJ
  doi: 10.1086/424617
– volume: 742
  start-page: L22
  year: 2011
  ident: ajaceaf0bib64
  publication-title: ApJL
  doi: 10.1088/2041-8205/742/2/L22
– volume: 130
  start-page: 2392
  year: 2005
  ident: ajaceaf0bib40
  publication-title: AJ
  doi: 10.1086/452638
– volume: 154
  start-page: 171
  year: 2017
  ident: ajaceaf0bib76
  publication-title: AJ
  doi: 10.3847/1538-3881/aa8b65
– volume: 764
  start-page: L2
  year: 2013
  ident: ajaceaf0bib79
  publication-title: ApJL
  doi: 10.1088/2041-8205/764/1/L2
– volume: 617
  start-page: 645
  year: 2004
  ident: ajaceaf0bib18
  publication-title: ApJ
  doi: 10.1086/422095
– year: 2023
  ident: ajaceaf0bib10
– volume: 215
  start-page: 491
  year: 2011
  ident: ajaceaf0bib45
  publication-title: Icar
  doi: 10.1016/j.icarus.2011.07.037
– volume: 158
  start-page: 49
  year: 2019
  ident: ajaceaf0bib90
  publication-title: AJ
  doi: 10.3847/1538-3881/ab24e1
– volume: 153
  start-page: 236
  year: 2017
  ident: ajaceaf0bib74
  publication-title: AJ
  doi: 10.3847/1538-3881/aa6aa5
– volume: 157
  start-page: 253
  year: 2019
  ident: ajaceaf0bib50
  publication-title: AJ
  doi: 10.3847/1538-3881/ab1c4c
– volume: 54
  start-page: 87
  year: 2006
  ident: ajaceaf0bib54
  publication-title: P&SS
  doi: 10.1016/j.pss.2005.10.006
– volume: 157
  start-page: 139
  year: 2019
  ident: ajaceaf0bib86
  publication-title: AJ
  doi: 10.3847/1538-3881/ab0895
– volume: 471
  start-page: L61
  year: 2017
  ident: ajaceaf0bib25
  publication-title: MNRASL
  doi: 10.1093/mnrasl/slx106
– volume: 1
  start-page: 121
  year: 2012
  ident: ajaceaf0bib53
  publication-title: MEEP
  doi: 10.48550/arXiv.1212.6124
– volume: 304
  start-page: 793
  year: 1999
  ident: ajaceaf0bib19
  publication-title: MNRAS
  doi: 10.1046/j.1365-8711.1999.02379.x
– volume: 541
  start-page: A92
  year: 2012
  ident: ajaceaf0bib78
  publication-title: A&A
  doi: 10.1051/0004-6361/201118541
– volume: 152
  start-page: 111
  year: 2016
  ident: ajaceaf0bib2
  publication-title: AJ
  doi: 10.3847/0004-6256/152/5/111
– volume: 160
  start-page: 46
  year: 2020
  ident: ajaceaf0bib69
  publication-title: AJ
  doi: 10.3847/1538-3881/ab98fb
– volume: 640
  start-page: A6
  year: 2020
  ident: ajaceaf0bib27
  publication-title: A&A
  doi: 10.1051/0004-6361/202037919
– volume: 150
  start-page: 68
  year: 2015a
  ident: ajaceaf0bib65
  publication-title: AJ
  doi: 10.1088/0004-6256/150/3/68
– volume: 152
  start-page: 221
  year: 2016
  ident: ajaceaf0bib84
  publication-title: AJ
  doi: 10.3847/1538-3881/152/6/221
– volume: 155
  start-page: 260
  year: 2018
  ident: ajaceaf0bib93
  publication-title: AJ
  doi: 10.3847/1538-3881/aac268
– volume: 825
  start-page: L13
  year: 2016
  ident: ajaceaf0bib85
  publication-title: ApJL
  doi: 10.3847/2041-8205/825/1/L13
– volume: Vol. 463
  start-page: 61
  year: 2020
  ident: ajaceaf0bib48
– volume: 151
  start-page: 22
  year: 2016
  ident: ajaceaf0bib7
  publication-title: AJ
  doi: 10.3847/0004-6256/151/2/22
– volume: 643
  start-page: L135
  year: 2006
  ident: ajaceaf0bib30
  publication-title: ApJ
  doi: 10.1086/505214
– volume: 225
  start-page: 40
  year: 2013
  ident: ajaceaf0bib14
  publication-title: Icar
  doi: 10.1016/j.icarus.2013.03.012
– volume: 420
  start-page: 3396
  year: 2012
  ident: ajaceaf0bib16
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2011.20264.x
– volume: 153
  start-page: 63
  year: 2017b
  ident: ajaceaf0bib82
  publication-title: AJ
  doi: 10.3847/1538-3881/153/2/63
– start-page: 43
  year: 2008
  ident: ajaceaf0bib34
– volume: 161
  start-page: 404
  year: 2003
  ident: ajaceaf0bib37
  publication-title: Icar
  doi: 10.1016/S0019-1035(02)00056-8
– volume: 142
  start-page: 131
  year: 2011
  ident: ajaceaf0bib73
  publication-title: AJ
  doi: 10.1088/0004-6256/142/4/131
– volume: 151
  start-page: 31
  year: 2016
  ident: ajaceaf0bib81
  publication-title: AJ
  doi: 10.3847/0004-6256/151/2/31
– volume: 2
  start-page: 59
  year: 2021
  ident: ajaceaf0bib63
  publication-title: PSJ
  doi: 10.3847/PSJ/abe53e
– year: 2023
  ident: ajaceaf0bib47
– volume: 189
  start-page: 213
  year: 2007b
  ident: ajaceaf0bib56
  publication-title: Icar
  doi: 10.1016/j.icarus.2007.01.001
– volume: 541
  start-page: L6
  year: 2012
  ident: ajaceaf0bib72
  publication-title: A&A
  doi: 10.1051/0004-6361/201218874
– volume: 638
  start-page: A23
  year: 2020
  ident: ajaceaf0bib26
  publication-title: A&A
  doi: 10.1051/0004-6361/201936183
– volume: 827
  start-page: L24
  year: 2016
  ident: ajaceaf0bib21
  publication-title: ApJL
  doi: 10.3847/2041-8205/827/2/L24
– volume: 5
  start-page: 14
  year: 2018a
  ident: ajaceaf0bib49
  publication-title: FrASS
  doi: 10.3389/fspas.2018.00014
– volume: 155
  start-page: 75
  year: 2018
  ident: ajaceaf0bib87
  publication-title: AJ
  doi: 10.3847/1538-3881/aaa19b
– volume: 152
  start-page: 70
  year: 2016
  ident: ajaceaf0bib4
  publication-title: AJ
  doi: 10.3847/0004-6256/152/3/70
– volume: 153
  start-page: 262
  year: 2017
  ident: ajaceaf0bib5
  publication-title: AJ
  doi: 10.3847/1538-3881/aa6db5
– volume: 564
  start-page: A44
  year: 2014
  ident: ajaceaf0bib13
  publication-title: A&A
  doi: 10.1051/0004-6361/201322041
– volume: 110
  start-page: 420
  year: 1995
  ident: ajaceaf0bib60
  publication-title: AJ
  doi: 10.1086/117532
– volume: 827
  start-page: L35
  year: 2016
  ident: ajaceaf0bib71
  publication-title: ApJL
  doi: 10.3847/2041-8205/827/2/L35
– volume: 157
  start-page: 269
  year: 2002
  ident: ajaceaf0bib31
  publication-title: Icar
  doi: 10.1006/icar.2002.6860
– volume: 154
  start-page: 62
  year: 2017
  ident: ajaceaf0bib91
  publication-title: AJ
  doi: 10.3847/1538-3881/aa79ff
– start-page: 259
  year: 2008
  ident: ajaceaf0bib38
– volume: 938
  start-page: L23
  year: 2022
  ident: ajaceaf0bib41
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac9480
SSID ssj0011804
Score 2.5278325
Snippet The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N -body computer...
The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N-body computer...
The orbits of trans-Neptunian objects (TNOs) can indicate the existence of an undiscovered planet in the outer solar system. Here we used N -body computer...
SourceID doaj
proquest
crossref
iop
SourceType Open Website
Aggregation Database
Enrichment Source
Index Database
Publisher
StartPage 118
SubjectTerms Astronomy
Detached objects
Earth
Gravitational effects
Gravity effects
Kuiper belt
Neptune
Orbital resonances (celestial mechanics)
Orbits
Outer solar system
Perihelions
Perturbation
Planets
Resonant Kuiper belt objects
Scattered disk objects
Solar system
Solar system planets
Terrestrial planets
Trans-Neptunian objects
SummonAdditionalLinks – databaseName: Directory of Open Access Journals (DOAJ) (Open Access)
  dbid: DOA
  link: http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwrV1La9wwEBYh9NBL6JNsmhQd2kIPZmVLsqRTSdKEloSQQwu5CUkeEZOtd1k7hf77jmRvmlBIL70ZM9bj-yzNjB4zhLyTDnhjmC-MCFAID7LQtfOF46wJLqAChsz0ubq40FdX5vJeqq90JmwMDzwCNxcAquJReB4a0TjAckssXtWMi8bkG9QVU2bjTE37B6VmYtyU5Dj9zvOw5lqXcxfARfZACeVY_aha2uXqrwk5a5nTZ2RnMg_p4dis52QLuhdk97BPC9bLH7_oB5qfx_WI_iUxX3uKTK-Buo6eYG-ui0V7AzTlIoKBth1FA49-TkZiN9Cz23YFa3oEi-HTK_L99OTb8ZdiyoZQIGJyKKCWjecKLZx8oZU5xrmsI6uiF3VjjIwqliqiw-cMcBUV9z5UUaKWqkJQjr8m292yg11CU9oxhwPTVQ4NKCE1A9RSvvIq8shknJH5Bh4bplDhKWPFwqLLkAC1CVCbALUjoDPy8e6L1Rgm4xHZo4T4nVwKcJ1fIO12ot3-i_YZeY982WnA9Y9UdvBADqsp69py9Hy0XTXY1f0N43-EKi2Tn6a53vsfbX1DnqYk9ePJtH2yPaxv4YA8CT-Htl-_zT_ub_0s7yM
  priority: 102
  providerName: Directory of Open Access Journals
Title Is There an Earth-like Planet in the Distant Kuiper Belt?
URI https://iopscience.iop.org/article/10.3847/1538-3881/aceaf0
https://www.proquest.com/docview/2857439838
https://doaj.org/article/4ee723f4b3cd4dae90b1e3d76034d931
Volume 166
WOSCitedRecordID wos001054312700001&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D
hasFullText 1
inHoldings 1
isFullTextHit
isPrint
journalDatabaseRights – providerCode: PRVAON
  databaseName: DOAJ Open Access Full Text
  customDbUrl:
  eissn: 1538-3881
  dateEnd: 99991231
  omitProxy: false
  ssIdentifier: ssj0011804
  issn: 0004-6256
  databaseCode: DOA
  dateStart: 20220101
  isFulltext: true
  titleUrlDefault: https://www.doaj.org/
  providerName: Directory of Open Access Journals
– providerCode: PRVIOP
  databaseName: Institute of Physics Open Access Journal Titles
  customDbUrl:
  eissn: 1538-3881
  dateEnd: 99991231
  omitProxy: false
  ssIdentifier: ssj0011804
  issn: 0004-6256
  databaseCode: O3W
  dateStart: 19980101
  isFulltext: true
  titleUrlDefault: http://iopscience.iop.org/
  providerName: IOP Publishing
link http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3Nb9UwDI-mjQMXNr60xz6UAyBxKC-tkyYVB7TBJhBocACxW5Skjnji0ff02k3af4_Tdg9NoAmJW1S5dfuzHdtJYzP2VDmEuhI-q2TATHpUmSmdzxyIOrhADhh7SX_UZ2fm_Lz6vMFerc_CLJbj1P-ShkOh4AHCZN9Ac-m0t1EwJp-6gC5Svr4Fhtw4KfMn-LbeQsiNGEowC5lRkD_uUf71CTd8Ul-6nzwNsf9jfu6dzun2f73uDrs3xpr8aCC9zzawecB2j9q0-r34ecWf8348LG60D1n1vuWkNivkruEnxOF7Np_9QJ4aG2HHZw2naJG_TRFn0_EPF7MlrvgxzrvXj9jX05Mvb95lY2uFjOBXXYalqj1oCpf607HCCQBVRlFEL8u6qlTUMdeRskdXIeiowftQREUurwhBO3jMNptFg7uMpx5mjqzcFY6iMamMQHJ5vvA6QhQqTtj0Glwbxrrjqf3F3FL-kRCyCSGbELIDQhP2Yn3Hcqi5cQvtcZLXmi5Vy-4vkCjsKAorEXUBUXoItawdkm7mpKK6FCDrCvIJe0bSs6P1trcwO7hBR2zysrRAaZSxy5o-df9aX34TFUalpM-AefKPbPbY3dTUfviTbZ9tdqsLPGB3wmU3a1eH_arBYa_rvwA00_sS
linkProvider IOP Publishing
linkToPdf http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3db9QwDI9gIMQL42vawTbyAEg8hEubpEmfpo3txLTp2AOIvUVJ6ogTR-907ZD473Ha7tAEmibxFlVuHflnx3bS2IS8Vg5EVXLPShmASQ-KmcJ55gSvggvogKFD-kxPp-biojwf-px2d2EWy2Hpf4_DvlBwL8Jk3wLX0nFno8KYbOwCuMjHyyreJfdSnZKk1p_E1_UxQmZ4X4aZS4aB_nBO-c-vXPNLXfl-9DY4hb_W6M7xTDb_e8qPyaMh5qQHPfkTcgfqp2T7oEm74Isfv-hb2o37TY7mGSlPGorqswLqanqMXL6x-ew70NTgCFo6qylGjfQoRZ51S08vZ0tY0UOYt_vPyZfJ8ecPH9nQYoEhDKplUKjKC41hU3dLljsuhCoiz6OXRVWWKuqY6YhZpCtB6KiF9yGPCl1fHoJ2Yots1IsatglNvcwcWrvLHUZlUhkO6Pp87nUUkas4IuMrAdsw1B9PbTDmFvOQJCWbpGSTlGwvpRF5t35j2dfeuIH2MGG2pktVs7sHCIcd4LASQOciSi9CJSsHqKMZqqouuJBVKbIReYMI2sGKmxuY7V6jQzZZUViB6ZSxCO2I7FzpzB-i3KiU_BlhXtySzSvy4PxoYs9OpqcvycPU577_uW2HbLSrS9gl98PPdtas9jql_w1zBf-F
openUrl ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Is+There+an+Earth-like+Planet+in+the+Distant+Kuiper+Belt%3F&rft.jtitle=The+Astronomical+journal&rft.au=Lykawka%2C+Patryk+Sofia&rft.au=Ito%2C+Takashi&rft.date=2023-09-01&rft.pub=The+American+Astronomical+Society&rft.issn=0004-6256&rft.eissn=1538-3881&rft.volume=166&rft.issue=3&rft_id=info:doi/10.3847%2F1538-3881%2Faceaf0&rft.externalDocID=ajaceaf0
thumbnail_l http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0004-6256&client=summon
thumbnail_m http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0004-6256&client=summon
thumbnail_s http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0004-6256&client=summon