FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2891194629> ?p ?o ?g. }

• W2891194629 endingPage "882" @default.
• W2891194629 startingPage "878" @default.
• W2891194629 abstract "The orbital distribution of trans-Neptunian objects provides strong evidence for the radial migration of Neptune1,2. The outer planets’ orbits are thought to have become unstable during the early stages3, with Jupiter having scattering encounters with a Neptune-class planet4. As a consequence, Jupiter jumped inwards by a fraction of an au, as required from inner Solar System constraints5,6, and obtained its current orbital eccentricity. The timing of these events is often linked to the lunar Late Heavy Bombardment that ended ~700 Myr after the dispersal of the protosolar nebula (t0)7,8. Here, we show instead that planetary migration started shortly after t0. Such early migration is inferred from the survival of the Patroclus–Menoetius binary Jupiter Trojan9. The binary formed at t ≲ t010,11 within a massive planetesimal disk once located beyond Neptune12,13. The longer the binary stayed in the disk, the greater the likelihood that collisions would strip its components from one another. The simulations of its survival indicate that the disk had to have been dispersed by migrating planets within ≲100 Myr of t0. This constraint implies that the planetary migration is unrelated to the formation of the youngest lunar basins. The Patroclus–Menoetius Jupiter Trojan binary could survive its travel from the Kuiper belt to Jupiter’s orbit only if the giant planets’ migrations happened within ~100 Myr after the birth of the Solar System and not after ~700 Myr, as suggested instead by the Late Heavy Bombardment." @default.
• W2891194629 created "2018-09-27" @default.
• W2891194629 creator A5004357384 @default.
• W2891194629 creator A5015258205 @default.
• W2891194629 creator A5028875386 @default.
• W2891194629 creator A5086074623 @default.
• W2891194629 date "2018-09-10" @default.
• W2891194629 modified "2023-10-15" @default.
• W2891194629 title "Evidence for very early migration of the Solar System planets from the Patroclus–Menoetius binary Jupiter Trojan" @default.
• W2891194629 cites W1673830338 @default.
• W2891194629 cites W1677261409 @default.
• W2891194629 cites W1942307606 @default.
• W2891194629 cites W1965374270 @default.
• W2891194629 cites W1970508912 @default.
• W2891194629 cites W1971212684 @default.
• W2891194629 cites W1972360949 @default.
• W2891194629 cites W1981500148 @default.
• W2891194629 cites W1989033868 @default.
• W2891194629 cites W1989809636 @default.
• W2891194629 cites W1990388558 @default.
• W2891194629 cites W1990610608 @default.
• W2891194629 cites W2014422618 @default.
• W2891194629 cites W2017171309 @default.
• W2891194629 cites W2026396557 @default.
• W2891194629 cites W2030648912 @default.
• W2891194629 cites W2035721686 @default.
• W2891194629 cites W2041775599 @default.
• W2891194629 cites W2043247258 @default.
• W2891194629 cites W2047421713 @default.
• W2891194629 cites W2048781153 @default.
• W2891194629 cites W2054401882 @default.
• W2891194629 cites W2075415607 @default.
• W2891194629 cites W2091145190 @default.
• W2891194629 cites W2094454497 @default.
• W2891194629 cites W2118061876 @default.
• W2891194629 cites W2126530639 @default.
• W2891194629 cites W2130350225 @default.
• W2891194629 cites W2782794416 @default.
• W2891194629 cites W3098069294 @default.
• W2891194629 cites W3098211898 @default.
• W2891194629 cites W3098814595 @default.
• W2891194629 cites W3099686661 @default.
• W2891194629 cites W3100301833 @default.
• W2891194629 cites W3101062331 @default.
• W2891194629 cites W3101319390 @default.
• W2891194629 cites W3103536328 @default.
• W2891194629 cites W3104398746 @default.
• W2891194629 cites W3104538763 @default.
• W2891194629 cites W3105108296 @default.
• W2891194629 cites W3105873797 @default.
• W2891194629 cites W3106204382 @default.
• W2891194629 doi "https://doi.org/10.1038/s41550-018-0564-3" @default.
• W2891194629 hasPublicationYear "2018" @default.
• W2891194629 type Work @default.
• W2891194629 sameAs 2891194629 @default.
• W2891194629 citedByCount "97" @default.
• W2891194629 countsByYear W28911946292018 @default.
• W2891194629 countsByYear W28911946292019 @default.
• W2891194629 countsByYear W28911946292020 @default.
• W2891194629 countsByYear W28911946292021 @default.
• W2891194629 countsByYear W28911946292022 @default.
• W2891194629 countsByYear W28911946292023 @default.
• W2891194629 crossrefType "journal-article" @default.
• W2891194629 hasAuthorship W2891194629A5004357384 @default.
• W2891194629 hasAuthorship W2891194629A5015258205 @default.
• W2891194629 hasAuthorship W2891194629A5028875386 @default.
• W2891194629 hasAuthorship W2891194629A5086074623 @default.
• W2891194629 hasBestOaLocation W28911946292 @default.
• W2891194629 hasConcept C100905312 @default.
• W2891194629 hasConcept C121332964 @default.
• W2891194629 hasConcept C127313418 @default.
• W2891194629 hasConcept C1276947 @default.
• W2891194629 hasConcept C174333608 @default.
• W2891194629 hasConcept C175207232 @default.
• W2891194629 hasConcept C22268893 @default.
• W2891194629 hasConcept C2780118271 @default.
• W2891194629 hasConcept C2780909310 @default.
• W2891194629 hasConcept C29829512 @default.
• W2891194629 hasConcept C44870925 @default.
• W2891194629 hasConcept C51244244 @default.
• W2891194629 hasConcept C539450922 @default.
• W2891194629 hasConcept C66279824 @default.
• W2891194629 hasConcept C87355193 @default.
• W2891194629 hasConcept C93436676 @default.
• W2891194629 hasConceptScore W2891194629C100905312 @default.
• W2891194629 hasConceptScore W2891194629C121332964 @default.
• W2891194629 hasConceptScore W2891194629C127313418 @default.
• W2891194629 hasConceptScore W2891194629C1276947 @default.
• W2891194629 hasConceptScore W2891194629C174333608 @default.
• W2891194629 hasConceptScore W2891194629C175207232 @default.
• W2891194629 hasConceptScore W2891194629C22268893 @default.
• W2891194629 hasConceptScore W2891194629C2780118271 @default.
• W2891194629 hasConceptScore W2891194629C2780909310 @default.
• W2891194629 hasConceptScore W2891194629C29829512 @default.
• W2891194629 hasConceptScore W2891194629C44870925 @default.
• W2891194629 hasConceptScore W2891194629C51244244 @default.
• W2891194629 hasConceptScore W2891194629C539450922 @default.
• W2891194629 hasConceptScore W2891194629C66279824 @default.

• next