FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1495684518> ?p ?o ?g. }

• W1495684518 endingPage "557" @default.
• W1495684518 startingPage "549" @default.
• W1495684518 abstract "Simple “solar systems” are generated with planetary orbital radiirdistributed uniformly random in logrbetween 0.2 and 50 AU, with masses and order identical to our own Solar System. A conservative stability criterion is imposed by requiring that adjacent planets are separated by a minimum distance ofktimes the sum of their Hill radii for values ofkranging from 0 to 8. Least-squares fits of these systems to generalized Bode laws are performed and compared to the fit of our own Solar System. We find that this stability criterion and other “radius-exclusion” laws generally produce approximately geometrically spaced planets that fit a Titius–Bode law about as well as our own Solar System. We then allow the random systems the same exceptions that have historically been applied to our own Solar System. Namely, one gap may be inserted, similar to the gap between Mars and Jupiter, and up to 3 planets may be “ignored,” similar to how some forms of Bode's law ignore Mercury, Neptune, and Pluto. With these particular exceptions, we find that our Solar System fits significantly better than the random ones. However, we believe that this choice of exceptions, designed specifically to give our own Solar System a better fit, gives it an unfair advantage that would be lost if other exception rules were used. We compare our results to previous work that uses a “law of increasing differences” as a basis for judging the significance of Bode's law. We note that the law of increasing differences is not physically based and is probably too stringent a constraint for judging the significance of Bode's law. We conclude that the significance of Bode's law is simply that stable planetary systems tend to be regularly spaced and conjecture that this conclusion could be strengthened by the use of more rigorous methods of rejecting unstable planetary systems, such as long-term orbit integrations." @default.
• W1495684518 created "2016-06-24" @default.
• W1495684518 creator A5028882289 @default.
• W1495684518 creator A5083154228 @default.
• W1495684518 date "1998-10-01" @default.
• W1495684518 modified "2023-09-27" @default.
• W1495684518 title "Fitting Selected Random Planetary Systems to Titius–Bode Laws" @default.
• W1495684518 cites W1584875893 @default.
• W1495684518 cites W1609133230 @default.
• W1495684518 cites W1649224703 @default.
• W1495684518 cites W1967245741 @default.
• W1495684518 cites W1969515303 @default.
• W1495684518 cites W1973398885 @default.
• W1495684518 cites W1976860825 @default.
• W1495684518 cites W1992637546 @default.
• W1495684518 cites W1997828263 @default.
• W1495684518 cites W2004651075 @default.
• W1495684518 cites W2015537456 @default.
• W1495684518 cites W2020298162 @default.
• W1495684518 cites W2024453749 @default.
• W1495684518 cites W2037521690 @default.
• W1495684518 cites W2043880644 @default.
• W1495684518 cites W2055770340 @default.
• W1495684518 cites W2057848283 @default.
• W1495684518 cites W2062149527 @default.
• W1495684518 cites W2065584453 @default.
• W1495684518 cites W2070955095 @default.
• W1495684518 cites W2088702447 @default.
• W1495684518 cites W3104231256 @default.
• W1495684518 cites W4251585788 @default.
• W1495684518 doi "https://doi.org/10.1006/icar.1998.5999" @default.
• W1495684518 hasPublicationYear "1998" @default.
• W1495684518 type Work @default.
• W1495684518 sameAs 1495684518 @default.
• W1495684518 citedByCount "72" @default.
• W1495684518 countsByYear W14956845182012 @default.
• W1495684518 countsByYear W14956845182013 @default.
• W1495684518 countsByYear W14956845182014 @default.
• W1495684518 countsByYear W14956845182015 @default.
• W1495684518 countsByYear W14956845182016 @default.
• W1495684518 countsByYear W14956845182017 @default.
• W1495684518 countsByYear W14956845182018 @default.
• W1495684518 countsByYear W14956845182019 @default.
• W1495684518 countsByYear W14956845182020 @default.
• W1495684518 countsByYear W14956845182021 @default.
• W1495684518 countsByYear W14956845182022 @default.
• W1495684518 countsByYear W14956845182023 @default.
• W1495684518 crossrefType "journal-article" @default.
• W1495684518 hasAuthorship W1495684518A5028882289 @default.
• W1495684518 hasAuthorship W1495684518A5083154228 @default.
• W1495684518 hasConcept C121332964 @default.
• W1495684518 hasConcept C121864883 @default.
• W1495684518 hasConcept C17744445 @default.
• W1495684518 hasConcept C199539241 @default.
• W1495684518 hasConcept C2780263841 @default.
• W1495684518 hasConcept C44870925 @default.
• W1495684518 hasConcept C51244244 @default.
• W1495684518 hasConcept C525488444 @default.
• W1495684518 hasConcept C539450922 @default.
• W1495684518 hasConcept C83260615 @default.
• W1495684518 hasConcept C87355193 @default.
• W1495684518 hasConceptScore W1495684518C121332964 @default.
• W1495684518 hasConceptScore W1495684518C121864883 @default.
• W1495684518 hasConceptScore W1495684518C17744445 @default.
• W1495684518 hasConceptScore W1495684518C199539241 @default.
• W1495684518 hasConceptScore W1495684518C2780263841 @default.
• W1495684518 hasConceptScore W1495684518C44870925 @default.
• W1495684518 hasConceptScore W1495684518C51244244 @default.
• W1495684518 hasConceptScore W1495684518C525488444 @default.
• W1495684518 hasConceptScore W1495684518C539450922 @default.
• W1495684518 hasConceptScore W1495684518C83260615 @default.
• W1495684518 hasConceptScore W1495684518C87355193 @default.
• W1495684518 hasIssue "2" @default.
• W1495684518 hasLocation W14956845181 @default.
• W1495684518 hasOpenAccess W1495684518 @default.
• W1495684518 hasPrimaryLocation W14956845181 @default.
• W1495684518 hasRelatedWork W1660865073 @default.
• W1495684518 hasRelatedWork W1667492772 @default.
• W1495684518 hasRelatedWork W1967961449 @default.
• W1495684518 hasRelatedWork W2143921922 @default.
• W1495684518 hasRelatedWork W2602488060 @default.
• W1495684518 hasRelatedWork W2883059866 @default.
• W1495684518 hasRelatedWork W2946568669 @default.
• W1495684518 hasRelatedWork W2967134422 @default.
• W1495684518 hasRelatedWork W3157609106 @default.
• W1495684518 hasRelatedWork W4313500100 @default.
• W1495684518 hasVolume "135" @default.
• W1495684518 isParatext "false" @default.
• W1495684518 isRetracted "false" @default.
• W1495684518 magId "1495684518" @default.
• W1495684518 workType "article" @default.