FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2044921750> ?p ?o ?g. }

• W2044921750 endingPage "101" @default.
• W2044921750 startingPage "101" @default.
• W2044921750 abstract "We present N-body simulations of resonant planets with inclined orbits that show chaotically evolving eccentricities and inclinations that can persist for at least 10 Gyr. A wide range of behavior is possible, from fast, low amplitude variations to systems in which eccentricities reach 0.9999 and inclinations 179.9 degrees. While the orbital elements evolve chaotically, at least one resonant argument always librates. We show that the HD 73526, HD 45364 and HD 60532 systems may be in chaotically-evolving resonances. Chaotic evolution is apparent in the 2:1, 3:1 and 3:2 resonances, and for planetary masses from lunar- to Jupiter-mass. In some cases, orbital disruption occurs after several Gyr, implying the mechanism is not rigorously stable, just long-lived relative to the main sequence lifetimes of solar-type stars. Planet-planet scattering appears to yield planets in inclined resonances that evolve chaotically in about 0.5% of cases. These results suggest that 1) approximate methods for identifying unstable orbital architectures may have limited applicability, 2) the observed close-in exoplanets may be produced during the high eccentricity phases induced by inclined resonances, 3) those exoplanets' orbital planes may be misaligned with the host star's spin axis, 4) systems with resonances may be systematically younger than those without, 5) the distribution of period ratios of adjacent planets detected via transit may be skewed due to inclined resonances, and 6) potentially habitable planets in resonances may have dramatically different climatic evolution than the Earth. The GAIA spacecraft is capable of discovering giant planets in these types of orbits." @default.
• W2044921750 created "2016-06-24" @default.
• W2044921750 creator A5003918379 @default.
• W2044921750 creator A5023148685 @default.
• W2044921750 creator A5045650283 @default.
• W2044921750 creator A5056051251 @default.
• W2044921750 creator A5090192488 @default.
• W2044921750 date "2015-03-11" @default.
• W2044921750 modified "2023-10-18" @default.
• W2044921750 title "LONG-LIVED CHAOTIC ORBITAL EVOLUTION OF EXOPLANETS IN MEAN MOTION RESONANCES WITH MUTUAL INCLINATIONS" @default.
• W2044921750 cites W1608563462 @default.
• W2044921750 cites W169934384 @default.
• W2044921750 cites W1970337487 @default.
• W2044921750 cites W1977426157 @default.
• W2044921750 cites W1982883618 @default.
• W2044921750 cites W1987364463 @default.
• W2044921750 cites W1992486633 @default.
• W2044921750 cites W1994256085 @default.
• W2044921750 cites W1998144402 @default.
• W2044921750 cites W1999144124 @default.
• W2044921750 cites W2003638614 @default.
• W2044921750 cites W2004523188 @default.
• W2044921750 cites W2009848492 @default.
• W2044921750 cites W2010339488 @default.
• W2044921750 cites W2015270436 @default.
• W2044921750 cites W2024785675 @default.
• W2044921750 cites W2025566423 @default.
• W2044921750 cites W2026074191 @default.
• W2044921750 cites W2035225535 @default.
• W2044921750 cites W2035697154 @default.
• W2044921750 cites W2038770923 @default.
• W2044921750 cites W2040091043 @default.
• W2044921750 cites W2044302728 @default.
• W2044921750 cites W2046327126 @default.
• W2044921750 cites W2047751764 @default.
• W2044921750 cites W2049273242 @default.
• W2044921750 cites W2053123602 @default.
• W2044921750 cites W2054749235 @default.
• W2044921750 cites W2063848988 @default.
• W2044921750 cites W2065294336 @default.
• W2044921750 cites W2069498556 @default.
• W2044921750 cites W2074535863 @default.
• W2044921750 cites W2075397551 @default.
• W2044921750 cites W2075454570 @default.
• W2044921750 cites W2076986137 @default.
• W2044921750 cites W2083553011 @default.
• W2044921750 cites W2088017846 @default.
• W2044921750 cites W2093541015 @default.
• W2044921750 cites W2108004335 @default.
• W2044921750 cites W2109435540 @default.
• W2044921750 cites W2115923209 @default.
• W2044921750 cites W2120585843 @default.
• W2044921750 cites W2129323876 @default.
• W2044921750 cites W2134217601 @default.
• W2044921750 cites W2136808562 @default.
• W2044921750 cites W2143439529 @default.
• W2044921750 cites W2155028161 @default.
• W2044921750 cites W2158415587 @default.
• W2044921750 cites W2166321478 @default.
• W2044921750 cites W2200200051 @default.
• W2044921750 cites W2916017046 @default.
• W2044921750 cites W3099164202 @default.
• W2044921750 cites W3099191470 @default.
• W2044921750 cites W3099359476 @default.
• W2044921750 cites W3099481686 @default.
• W2044921750 cites W3100972102 @default.
• W2044921750 cites W3101086176 @default.
• W2044921750 cites W3101667268 @default.
• W2044921750 cites W3104104914 @default.
• W2044921750 cites W3105384520 @default.
• W2044921750 cites W3105595896 @default.
• W2044921750 cites W3124435578 @default.
• W2044921750 cites W3124700370 @default.
• W2044921750 cites W4248405238 @default.
• W2044921750 cites W4291158282 @default.
• W2044921750 cites W4292679241 @default.
• W2044921750 cites W4292925941 @default.
• W2044921750 doi "https://doi.org/10.1088/0004-637x/801/2/101" @default.
• W2044921750 hasPublicationYear "2015" @default.
• W2044921750 type Work @default.
• W2044921750 sameAs 2044921750 @default.
• W2044921750 citedByCount "39" @default.
• W2044921750 countsByYear W20449217502015 @default.
• W2044921750 countsByYear W20449217502016 @default.
• W2044921750 countsByYear W20449217502017 @default.
• W2044921750 countsByYear W20449217502018 @default.
• W2044921750 countsByYear W20449217502019 @default.
• W2044921750 countsByYear W20449217502020 @default.
• W2044921750 countsByYear W20449217502022 @default.
• W2044921750 crossrefType "journal-article" @default.
• W2044921750 hasAuthorship W2044921750A5003918379 @default.
• W2044921750 hasAuthorship W2044921750A5023148685 @default.
• W2044921750 hasAuthorship W2044921750A5045650283 @default.
• W2044921750 hasAuthorship W2044921750A5056051251 @default.
• W2044921750 hasAuthorship W2044921750A5090192488 @default.
• W2044921750 hasBestOaLocation W20449217502 @default.
• W2044921750 hasConcept C100905312 @default.
• W2044921750 hasConcept C121332964 @default.

• next