FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3098206564> ?p ?o ?g. }

• W3098206564 endingPage "514" @default.
• W3098206564 startingPage "502" @default.
• W3098206564 abstract "We calculate the theoretical evolution of the radii of all 14 of the known transiting extrasolar giant planets (EGPs) for a variety of assumptions concerning atmospheric opacity, dense inner core masses, and possible internal power sources. We incorporate the effects of stellar irradiation and customize such effects for each EGP and star. Looking collectively at the family as a whole, we find that there are in fact two radius anomalies to be explained. Not only are the radii of a subset of the known transiting EGPs larger than expected from previous theory, but many of the other objects are smaller than the default theory would allow. We suggest that the larger EGPs can be explained by invoking enhanced atmospheric opacities that naturally retain internal heat. This explanation might obviate the necessity for an extra internal power source. We explain the smaller radii by the presence in perhaps all the known transiting EGPs of dense cores, such as have been inferred for Saturn and Jupiter. Importantly, we derive a rough correlation between the masses of our best-fit cores and the stellar metallicity that seems to buttress the core-accretion model of their formation. Although many caveats and uncertainties remain, the resulting comprehensive theory that incorporates enhanced-opacity atmospheres and dense cores is in reasonable accord with all the current structural data for the known transiting giant planets." @default.
• W3098206564 created "2020-11-23" @default.
• W3098206564 creator A5008924957 @default.
• W3098206564 creator A5043683398 @default.
• W3098206564 creator A5058962721 @default.
• W3098206564 creator A5086989488 @default.
• W3098206564 date "2007-05-20" @default.
• W3098206564 modified "2023-09-30" @default.
• W3098206564 title "Possible Solutions to the Radius Anomalies of Transiting Giant Planets" @default.
• W3098206564 cites W1939930449 @default.
• W3098206564 cites W1971588807 @default.
• W3098206564 cites W1984886505 @default.
• W3098206564 cites W1990807991 @default.
• W3098206564 cites W2001363009 @default.
• W3098206564 cites W2006842164 @default.
• W3098206564 cites W2014203933 @default.
• W3098206564 cites W2024909325 @default.
• W3098206564 cites W2026586306 @default.
• W3098206564 cites W2028506786 @default.
• W3098206564 cites W2032506573 @default.
• W3098206564 cites W2034766327 @default.
• W3098206564 cites W2039556889 @default.
• W3098206564 cites W2041932094 @default.
• W3098206564 cites W2045315671 @default.
• W3098206564 cites W2055210280 @default.
• W3098206564 cites W2055588986 @default.
• W3098206564 cites W2057825380 @default.
• W3098206564 cites W2059365121 @default.
• W3098206564 cites W2061019537 @default.
• W3098206564 cites W2061169145 @default.
• W3098206564 cites W2063056462 @default.
• W3098206564 cites W2063886350 @default.
• W3098206564 cites W2072587396 @default.
• W3098206564 cites W2076564794 @default.
• W3098206564 cites W2084110269 @default.
• W3098206564 cites W2087667004 @default.
• W3098206564 cites W2095015809 @default.
• W3098206564 cites W2096390283 @default.
• W3098206564 cites W2098263921 @default.
• W3098206564 cites W2101755019 @default.
• W3098206564 cites W2107003980 @default.
• W3098206564 cites W2119351603 @default.
• W3098206564 cites W2125174972 @default.
• W3098206564 cites W2126063541 @default.
• W3098206564 cites W2135739790 @default.
• W3098206564 cites W2140611633 @default.
• W3098206564 cites W2146009459 @default.
• W3098206564 cites W2160318948 @default.
• W3098206564 cites W2162157272 @default.
• W3098206564 cites W2596914018 @default.
• W3098206564 cites W2963640325 @default.
• W3098206564 cites W3037008719 @default.
• W3098206564 cites W3098895462 @default.
• W3098206564 cites W3099054713 @default.
• W3098206564 cites W3099469292 @default.
• W3098206564 cites W3099823468 @default.
• W3098206564 cites W3100509799 @default.
• W3098206564 cites W3102407746 @default.
• W3098206564 cites W3102694870 @default.
• W3098206564 cites W3102938219 @default.
• W3098206564 cites W3103990027 @default.
• W3098206564 cites W3104302064 @default.
• W3098206564 cites W3104382587 @default.
• W3098206564 cites W3104691555 @default.
• W3098206564 cites W3105032004 @default.
• W3098206564 cites W3105190422 @default.
• W3098206564 cites W4244551766 @default.
• W3098206564 cites W4292508310 @default.
• W3098206564 cites W4300479344 @default.
• W3098206564 cites W4301910499 @default.
• W3098206564 doi "https://doi.org/10.1086/514326" @default.
• W3098206564 hasPublicationYear "2007" @default.
• W3098206564 type Work @default.
• W3098206564 sameAs 3098206564 @default.
• W3098206564 citedByCount "337" @default.
• W3098206564 countsByYear W30982065642012 @default.
• W3098206564 countsByYear W30982065642013 @default.
• W3098206564 countsByYear W30982065642014 @default.
• W3098206564 countsByYear W30982065642015 @default.
• W3098206564 countsByYear W30982065642016 @default.
• W3098206564 countsByYear W30982065642017 @default.
• W3098206564 countsByYear W30982065642018 @default.
• W3098206564 countsByYear W30982065642019 @default.
• W3098206564 countsByYear W30982065642020 @default.
• W3098206564 countsByYear W30982065642021 @default.
• W3098206564 countsByYear W30982065642022 @default.
• W3098206564 countsByYear W30982065642023 @default.
• W3098206564 crossrefType "journal-article" @default.
• W3098206564 hasAuthorship W3098206564A5008924957 @default.
• W3098206564 hasAuthorship W3098206564A5043683398 @default.
• W3098206564 hasAuthorship W3098206564A5058962721 @default.
• W3098206564 hasAuthorship W3098206564A5086989488 @default.
• W3098206564 hasBestOaLocation W30982065642 @default.
• W3098206564 hasConcept C100905312 @default.
• W3098206564 hasConcept C120665830 @default.
• W3098206564 hasConcept C121332964 @default.
• W3098206564 hasConcept C1276947 @default.
• W3098206564 hasConcept C129716092 @default.

• next