FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2122237670> ?p ?o ?g. }

• W2122237670 endingPage "3423" @default.
• W2122237670 startingPage "3404" @default.
• W2122237670 abstract "We examine formation conditions for the Galilean satellites in the context of models of late-stage giant planet accretion and satellite-disk interactions. We first reevaluate the current standard, in which the satellites form from a minimum mass subnebula disk, obtained by augmenting the mass of the current satellites to solar abundance and resulting in a disk mass containing about 2% of Jupiter's mass. Conditions in such a massive and gas-rich disk are difficult to reconcile with both the icy compositions of Ganymede and Callisto and the protracted formation time needed to explain Callisto's apparent incomplete differentiation. In addition, we argue that disk torques in such a gas-rich disk would cause large satellites to be lost to inward decay onto the planet. These issues have prevented us from identifying a self-consistent scenario for the formation and survival of the Galilean satellites using the standard model. We then consider an alternative, in which the satellites form in a circumplanetary accretion disk produced during the very end stages of gas accretion onto Jupiter. In this case, an amount of gas and solids of at least ∼0.02 Jovian masses must still be processed through the disk during the satellite formation era, but this amount need not have been present all at once. We find that an accretion disk produced by a slow inflow of gas and solids, e.g., 2 × 10-7 Jovian masses per year, is most consistent with conditions needed to form the Galilean satellites, including disk temperatures low enough for ices and protracted satellite accretion times of ≥105 yr. Such a gas-starved disk has an orders-of-magnitude lower gas surface density than the minimum mass subnebula (and for many cases is optically thin). Solids delivered to the disk build up over many disk viscous cycles, resulting in a greatly reduced gas-to-solids ratio during the final stages of satellite accretion. This allows for the survival of Galilean-sized satellites against disk torques over a wide range of plausible conditions." @default.
• W2122237670 created "2016-06-24" @default.
• W2122237670 creator A5072309602 @default.
• W2122237670 creator A5082077092 @default.
• W2122237670 date "2002-12-01" @default.
• W2122237670 modified "2023-10-12" @default.
• W2122237670 title "Formation of the Galilean Satellites: Conditions of Accretion" @default.
• W2122237670 cites W1496423403 @default.
• W2122237670 cites W1566550384 @default.
• W2122237670 cites W1654550887 @default.
• W2122237670 cites W1963722072 @default.
• W2122237670 cites W1970567661 @default.
• W2122237670 cites W1972551044 @default.
• W2122237670 cites W1973351361 @default.
• W2122237670 cites W1974486269 @default.
• W2122237670 cites W1974947904 @default.
• W2122237670 cites W1984310872 @default.
• W2122237670 cites W1985663566 @default.
• W2122237670 cites W1990409096 @default.
• W2122237670 cites W1991294021 @default.
• W2122237670 cites W1993008858 @default.
• W2122237670 cites W1995394048 @default.
• W2122237670 cites W1995474717 @default.
• W2122237670 cites W1995532941 @default.
• W2122237670 cites W2001281840 @default.
• W2122237670 cites W2002166777 @default.
• W2122237670 cites W2006357369 @default.
• W2122237670 cites W2013232421 @default.
• W2122237670 cites W2015949279 @default.
• W2122237670 cites W2016680615 @default.
• W2122237670 cites W2017382842 @default.
• W2122237670 cites W2018652096 @default.
• W2122237670 cites W2019052401 @default.
• W2122237670 cites W2034380097 @default.
• W2122237670 cites W2039427272 @default.
• W2122237670 cites W2041685615 @default.
• W2122237670 cites W2044654720 @default.
• W2122237670 cites W2045730088 @default.
• W2122237670 cites W2046128110 @default.
• W2122237670 cites W2063886350 @default.
• W2122237670 cites W2066986330 @default.
• W2122237670 cites W2067190381 @default.
• W2122237670 cites W2071749249 @default.
• W2122237670 cites W2072326464 @default.
• W2122237670 cites W2084698693 @default.
• W2122237670 cites W2085220852 @default.
• W2122237670 cites W2086345762 @default.
• W2122237670 cites W2089818471 @default.
• W2122237670 cites W2090401230 @default.
• W2122237670 cites W2092693142 @default.
• W2122237670 cites W2100285830 @default.
• W2122237670 cites W2111874509 @default.
• W2122237670 cites W2112648881 @default.
• W2122237670 cites W2116952160 @default.
• W2122237670 cites W2124817707 @default.
• W2122237670 cites W2129743734 @default.
• W2122237670 cites W2130374446 @default.
• W2122237670 cites W2133770234 @default.
• W2122237670 cites W2140611633 @default.
• W2122237670 cites W2159057538 @default.
• W2122237670 cites W2164979235 @default.
• W2122237670 cites W2317160589 @default.
• W2122237670 cites W2916017046 @default.
• W2122237670 cites W3003186255 @default.
• W2122237670 cites W3098041279 @default.
• W2122237670 cites W3098885964 @default.
• W2122237670 cites W3101634830 @default.
• W2122237670 cites W3104527955 @default.
• W2122237670 cites W343244306 @default.
• W2122237670 cites W4246363448 @default.
• W2122237670 cites W4253834182 @default.
• W2122237670 doi "https://doi.org/10.1086/344684" @default.
• W2122237670 hasPublicationYear "2002" @default.
• W2122237670 type Work @default.
• W2122237670 sameAs 2122237670 @default.
• W2122237670 citedByCount "365" @default.
• W2122237670 countsByYear W21222376702012 @default.
• W2122237670 countsByYear W21222376702013 @default.
• W2122237670 countsByYear W21222376702014 @default.
• W2122237670 countsByYear W21222376702015 @default.
• W2122237670 countsByYear W21222376702016 @default.
• W2122237670 countsByYear W21222376702017 @default.
• W2122237670 countsByYear W21222376702018 @default.
• W2122237670 countsByYear W21222376702019 @default.
• W2122237670 countsByYear W21222376702020 @default.
• W2122237670 countsByYear W21222376702021 @default.
• W2122237670 countsByYear W21222376702022 @default.
• W2122237670 countsByYear W21222376702023 @default.
• W2122237670 crossrefType "journal-article" @default.
• W2122237670 hasAuthorship W2122237670A5072309602 @default.
• W2122237670 hasAuthorship W2122237670A5082077092 @default.
• W2122237670 hasBestOaLocation W21222376701 @default.
• W2122237670 hasConcept C100905312 @default.
• W2122237670 hasConcept C104060986 @default.
• W2122237670 hasConcept C118873486 @default.
• W2122237670 hasConcept C121332964 @default.
• W2122237670 hasConcept C1276947 @default.
• W2122237670 hasConcept C163479331 @default.

• next