Results 1 to 10 of about 90,567 (226)
Planet heating prevents inward migration of planetary cores [PDF]
Nature, 2015 Planetary systems are born in the disks of gas, dust and rocky fragments that surround newly formed stars. Solid content assembles into ever-larger rocky fragments that eventually become planetary embryos. These then continue their growth by accreting leftover material in the disc.
Frederic Masset
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Terrestrial planetary plants: Essential preparations for interstellar migration
Current Plant BiologyInterstellar migration offers great potential for expanding human habitable space. As a powerful entropy-reducing system, plants convert simple, disordered chemical elements into complex, ordered organic macromolecules.
Xiumei Luo +3 more
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Planetary migration to large radii [PDF]
Monthly Notices of the Royal Astronomical Society, 2007 Accepted for publication in ...
R. G. Martin +3 more
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Is planetary migration inevitable? [PDF]
, 2003 According to current theories, tidal interactions between a disk and an embedded planet may lead to the rapid migration of the protoplanet on a timescale shorter than the disk lifetime or estimated planetary formation timescales. Therefore, planets can form only if there is a mechanism to hold at least some of the cores back on their way in.
Caroline Terquem
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Metallicity, planetary formation and migration [PDF]
Monthly Notices of the Royal Astronomical Society, 2003 Recent observations show a clear correlation between the probability of hosting a planet and the metallicity of the parent star. Since radial velocity surveys are biased, however, towards detecting planets with short orbital periods, the probability-metallicity correlation could merely reflect a dependence of migration rates on metallicity.
Mario Livio, J. E. Pringle
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Planetary Migration and Plutino Orbital Inclinations [PDF]
The Astronomical Journal, 2000 I investigate which mechanisms could have acted during Neptune's past radial migration to excite plutino orbital inclinations to their present values. These processes include Kozai resonance and the ν18 secular resonance, both before and after the plutino's capture into the 2 : 3 mean motion resonance with Neptune. In the case that ν18 acted before the
R. S. Gomes
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Brownian Motion in Planetary Migration [PDF]
The Astrophysical Journal, 2006 A residual planetesimal disk of mass 10-100 Earth masses remained in the outer solar system following the birth of the giant planets, as implied by the existence of the Oort cloud, coagulation requirements for Pluto, and inefficiencies in planet formation. Upon gravitationally scattering planetesimal debris, planets migrate.
Ruth A. Murray‐Clay, Eugene I. Chiang
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Arthropod-borne disease challenges from planetary warming, urbanization, and migration [PDF]
Virology JournalAs the world confronts simultaneous climate and health emergencies, the spread of emerging infectious diseases, particularly arboviruses, underscores the intersection of planetary health, global mobility, and disease risk. Viral pathogens like Oropouche,
Maggie L. Bartlett +3 more
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Unconditional hospitality: art and commons under planetary migration
Journal of Aesthetics & Culture, 2022 In both European and non-European cities, public spaces are formed by racist and segregative politics that influence everyday life. Planetary migration flows and recently implemented border politics tend to leave the most vulnerable in precarious ...
Pelin Tan
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Percolative sulfide core formation in oxidized planetary bodies [PDF]
Nature CommunicationsModels of planetary core formation traditionally involve the fractionation of Fe,Ni-metal melts from silicate mantles after extensive silicate melting.
Samuel D. Crossley +9 more
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