Matches in SemOpenAlex for { <https://semopenalex.org/work/W4385371382> ?p ?o ?g. }
- W4385371382 endingPage "A109" @default.
- W4385371382 startingPage "A109" @default.
- W4385371382 abstract "Context. White dwarfs are the last evolutionary stage for the majority of main-sequence stars. With nuclear burning having ceased, these stars are slowly cooling. There is observational evidence indicating that planetary remnants, and possibly even planets, orbit a considerable fraction of the known white dwarf population. These objects are interesting targets for transit observations due to their large planet-to-star radius ratio. Especially interesting is the possible outgassing from such objects and their eventual observational prospects. Aims. Here, we investigate whether electromagnetic induction heating can drive additional volcanic outgassing from small planetary remnants orbiting white dwarfs. This mechanism can be important for such bodies in addition to tidal heating due to the extremely strong magnetic fields of some white dwarfs and close orbital distances of planets to their host stars. Methods. We calculated the heating and related magmatic effects for a Moon-sized body around a magnetized white dwarf using an analytical model for induction heating and a numerical model for interior processes. We also calculated induction heating inside asteroid-sized bodies. Results. We show that induction heating can melt the mantle of a Moon-sized object within a geologically short time and contribute to desiccation of small asteroids on extremely tight orbits. These findings can have important implications for the evolution of rocky bodies orbiting white dwarfs and the potential detection of their outgassing." @default.
- W4385371382 created "2023-07-29" @default.
- W4385371382 creator A5010008961 @default.
- W4385371382 creator A5042375264 @default.
- W4385371382 creator A5050798999 @default.
- W4385371382 creator A5079437698 @default.
- W4385371382 creator A5079907626 @default.
- W4385371382 creator A5084098015 @default.
- W4385371382 creator A5091779429 @default.
- W4385371382 date "2023-09-01" @default.
- W4385371382 modified "2023-09-23" @default.
- W4385371382 title "Induction heating of planetary interiors in white dwarf systems" @default.
- W4385371382 cites W1515675433 @default.
- W4385371382 cites W1594412726 @default.
- W4385371382 cites W1650578900 @default.
- W4385371382 cites W1678890861 @default.
- W4385371382 cites W1900616430 @default.
- W4385371382 cites W1964621123 @default.
- W4385371382 cites W1965690370 @default.
- W4385371382 cites W1974683840 @default.
- W4385371382 cites W1994880739 @default.
- W4385371382 cites W1997368455 @default.
- W4385371382 cites W1999892058 @default.
- W4385371382 cites W2001159851 @default.
- W4385371382 cites W2003474969 @default.
- W4385371382 cites W2006136210 @default.
- W4385371382 cites W2009708249 @default.
- W4385371382 cites W2020908136 @default.
- W4385371382 cites W2025467069 @default.
- W4385371382 cites W2029640176 @default.
- W4385371382 cites W2034051951 @default.
- W4385371382 cites W2036892144 @default.
- W4385371382 cites W2039919643 @default.
- W4385371382 cites W2041797061 @default.
- W4385371382 cites W2041984726 @default.
- W4385371382 cites W2042726507 @default.
- W4385371382 cites W2050756326 @default.
- W4385371382 cites W2064407202 @default.
- W4385371382 cites W2076202084 @default.
- W4385371382 cites W2078276168 @default.
- W4385371382 cites W2081543727 @default.
- W4385371382 cites W2085375544 @default.
- W4385371382 cites W2088500402 @default.
- W4385371382 cites W2089822037 @default.
- W4385371382 cites W2090849864 @default.
- W4385371382 cites W2094346776 @default.
- W4385371382 cites W2113945936 @default.
- W4385371382 cites W2132661748 @default.
- W4385371382 cites W2162021011 @default.
- W4385371382 cites W2163704918 @default.
- W4385371382 cites W2170555783 @default.
- W4385371382 cites W2271699978 @default.
- W4385371382 cites W2299087642 @default.
- W4385371382 cites W2333498558 @default.
- W4385371382 cites W2341342933 @default.
- W4385371382 cites W2481759643 @default.
- W4385371382 cites W2488365274 @default.
- W4385371382 cites W2546142438 @default.
- W4385371382 cites W2585829147 @default.
- W4385371382 cites W2590344143 @default.
- W4385371382 cites W2599368048 @default.
- W4385371382 cites W2616642533 @default.
- W4385371382 cites W2741907017 @default.
- W4385371382 cites W2747874630 @default.
- W4385371382 cites W2760809953 @default.
- W4385371382 cites W2913858408 @default.
- W4385371382 cites W2924119666 @default.
- W4385371382 cites W2989836337 @default.
- W4385371382 cites W3016885607 @default.
- W4385371382 cites W3085786719 @default.
- W4385371382 cites W3098698975 @default.
- W4385371382 cites W3099133876 @default.
- W4385371382 cites W3099383823 @default.
- W4385371382 cites W3100791356 @default.
- W4385371382 cites W3101309368 @default.
- W4385371382 cites W3102693680 @default.
- W4385371382 cites W3105117928 @default.
- W4385371382 cites W3105285378 @default.
- W4385371382 cites W3105724682 @default.
- W4385371382 cites W3105887797 @default.
- W4385371382 cites W3106004582 @default.
- W4385371382 cites W3106259933 @default.
- W4385371382 cites W3120221220 @default.
- W4385371382 cites W3133757340 @default.
- W4385371382 cites W3171581241 @default.
- W4385371382 cites W3175813211 @default.
- W4385371382 cites W3208953154 @default.
- W4385371382 cites W3212511494 @default.
- W4385371382 cites W3212739334 @default.
- W4385371382 cites W3214247466 @default.
- W4385371382 cites W4210925827 @default.
- W4385371382 cites W4288102915 @default.
- W4385371382 cites W4288278696 @default.
- W4385371382 doi "https://doi.org/10.1051/0004-6361/202245225" @default.
- W4385371382 hasPublicationYear "2023" @default.
- W4385371382 type Work @default.
- W4385371382 citedByCount "0" @default.
- W4385371382 crossrefType "journal-article" @default.