FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2619820255> ?p ?o ?g. }

• W2619820255 endingPage "3229" @default.
• W2619820255 startingPage "3217" @default.
• W2619820255 abstract "One long-standing problem for the potential habitability of planets within M dwarf systems is their likelihood to be tidally locked in a synchronously rotating spin state. This problem thus far has largely been addressed only by considering two objects: the star and the planet itself. However, many systems have been found to harbour multiple planets, with some in or very near to mean motion resonances. The presence of a planetary companion near a mean motion resonance can induce oscillatory variations in the mean motion of the planet, which we demonstrate can have significant effects on the spin state of an otherwise synchronously rotating planet. In particular, we find that a planetary companion near a mean motion resonance can excite the spin states of planets in the habitable zone of small, cool stars, pushing otherwise synchronously rotating planets into higher amplitude librations of the spin state, or even complete circulation resulting in effective stellar days with full surface coverage on the order of years or decades. This increase in illuminated area can have potentially dramatic influences on climate, and thus on habitability. We also find that the resultant spin state can be very sensitive to initial conditions due to the chaotic nature of the spin state at early times within certain regimes. We apply our model to two hypothetical planetary systems inspired by the K00255 and TRAPPIST-1 systems, both of which have Earth-sized planets in mean motion resonances orbiting cool stars." @default.
• W2619820255 created "2017-06-05" @default.
• W2619820255 creator A5024534230 @default.
• W2619820255 creator A5039246525 @default.
• W2619820255 date "2017-08-16" @default.
• W2619820255 modified "2023-09-27" @default.
• W2619820255 title "On the spin states of habitable zone exoplanets around M dwarfs: the effect of a near-resonant companion" @default.
• W2619820255 cites W1548710445 @default.
• W2619820255 cites W1641616920 @default.
• W2619820255 cites W1778582658 @default.
• W2619820255 cites W1966763439 @default.
• W2619820255 cites W1974677212 @default.
• W2619820255 cites W1996303783 @default.
• W2619820255 cites W2016680615 @default.
• W2619820255 cites W2032480060 @default.
• W2619820255 cites W2033279767 @default.
• W2619820255 cites W2035697154 @default.
• W2619820255 cites W2060943325 @default.
• W2619820255 cites W2079647818 @default.
• W2619820255 cites W2093634884 @default.
• W2619820255 cites W2107047551 @default.
• W2619820255 cites W2115689791 @default.
• W2619820255 cites W2120409697 @default.
• W2619820255 cites W2125574420 @default.
• W2619820255 cites W2128965561 @default.
• W2619820255 cites W2145612370 @default.
• W2619820255 cites W2152320386 @default.
• W2619820255 cites W2156723360 @default.
• W2619820255 cites W2157771386 @default.
• W2619820255 cites W2163377996 @default.
• W2619820255 cites W2164932327 @default.
• W2619820255 cites W2590741408 @default.
• W2619820255 cites W2594379411 @default.
• W2619820255 cites W2963604282 @default.
• W2619820255 cites W3037252605 @default.
• W2619820255 cites W3098551150 @default.
• W2619820255 cites W3098732753 @default.
• W2619820255 cites W3099971028 @default.
• W2619820255 cites W3100897102 @default.
• W2619820255 cites W3102433056 @default.
• W2619820255 cites W3102557014 @default.
• W2619820255 cites W3102817586 @default.
• W2619820255 cites W3103265921 @default.
• W2619820255 cites W3103276181 @default.
• W2619820255 cites W3103278752 @default.
• W2619820255 cites W3103893120 @default.
• W2619820255 cites W3104625650 @default.
• W2619820255 cites W3104774050 @default.
• W2619820255 cites W3106362850 @default.
• W2619820255 cites W4237204345 @default.
• W2619820255 doi "https://doi.org/10.1093/mnras/stx2100" @default.
• W2619820255 hasPublicationYear "2017" @default.
• W2619820255 type Work @default.
• W2619820255 sameAs 2619820255 @default.
• W2619820255 citedByCount "37" @default.
• W2619820255 countsByYear W26198202552017 @default.
• W2619820255 countsByYear W26198202552018 @default.
• W2619820255 countsByYear W26198202552019 @default.
• W2619820255 countsByYear W26198202552020 @default.
• W2619820255 countsByYear W26198202552021 @default.
• W2619820255 countsByYear W26198202552022 @default.
• W2619820255 countsByYear W26198202552023 @default.
• W2619820255 crossrefType "journal-article" @default.
• W2619820255 hasAuthorship W2619820255A5024534230 @default.
• W2619820255 hasAuthorship W2619820255A5039246525 @default.
• W2619820255 hasBestOaLocation W26198202552 @default.
• W2619820255 hasConcept C100905312 @default.
• W2619820255 hasConcept C121332964 @default.
• W2619820255 hasConcept C1276947 @default.
• W2619820255 hasConcept C162053735 @default.
• W2619820255 hasConcept C163479331 @default.
• W2619820255 hasConcept C197464742 @default.
• W2619820255 hasConcept C36293798 @default.
• W2619820255 hasConcept C42704618 @default.
• W2619820255 hasConcept C44870925 @default.
• W2619820255 hasConcept C51244244 @default.
• W2619820255 hasConcept C51553727 @default.
• W2619820255 hasConcept C87355193 @default.
• W2619820255 hasConcept C97355855 @default.
• W2619820255 hasConceptScore W2619820255C100905312 @default.
• W2619820255 hasConceptScore W2619820255C121332964 @default.
• W2619820255 hasConceptScore W2619820255C1276947 @default.
• W2619820255 hasConceptScore W2619820255C162053735 @default.
• W2619820255 hasConceptScore W2619820255C163479331 @default.
• W2619820255 hasConceptScore W2619820255C197464742 @default.
• W2619820255 hasConceptScore W2619820255C36293798 @default.
• W2619820255 hasConceptScore W2619820255C42704618 @default.
• W2619820255 hasConceptScore W2619820255C44870925 @default.
• W2619820255 hasConceptScore W2619820255C51244244 @default.
• W2619820255 hasConceptScore W2619820255C51553727 @default.
• W2619820255 hasConceptScore W2619820255C87355193 @default.
• W2619820255 hasConceptScore W2619820255C97355855 @default.
• W2619820255 hasIssue "3" @default.
• W2619820255 hasLocation W26198202551 @default.
• W2619820255 hasLocation W26198202552 @default.
• W2619820255 hasOpenAccess W2619820255 @default.
• W2619820255 hasPrimaryLocation W26198202551 @default.
• W2619820255 hasRelatedWork W2015270436 @default.

• next