학술논문

Solar System Ice Giants: Exoplanets in our Backyard
Document Type
Working Paper
Author
Rymer, AbigailMandt, KathleenHurley, DanaLisse, CareyIzenberg, NoamSmith, H. ToddWestlake, JosephBunce, EmmaArridge, ChristopherMasters, AdamHofstadter, MarkSimon, AmyBrandt, PontusClark, GeorgeCohen, IanAllen, RobertVine, SarahHansen, KennethHospodarsky, GeorgeKurth, WilliamRomani, PaulLamy, LaurentZarka, PhilippeCao, HaoPaty, CarolHedman, MatthewRoussos, EliasCruikshank, DaleFarrell, WilliamFieseler, PaulCoates, AndrewYelle, RogerParkinson, ChristopherMilitzer, BurkhardGrodent, DenisKollmann, PeterMcNutt, RalphAndré, NicolasStrange, NathanBarnes, JasonDones, LukeDenk, TilmannRathbun, JulieLunine, JonathanDesai, RaviCochrane, CoreySayanagi, Kunio M.Postberg, FrankEbert, RobertHill, ThomasMueller-Wodarg, IngoRegoli, LeonardoPontius, DuaneStanley, SabineGreathouse, ThomasSaur, JoachimMarouf, EssamBergman, JanHiggins, ChuckJohnson, RobertThomsen, MichelleSoderlund, KristaJia, XianzheWilson, RobertEnglander, JacobBurch, JimNordheim, TomGrava, CesareBaines, KevinQuick, LynnaeRussell, ChristopherCravens, ThomasCecconi, BaptisteAslam, ShahidBray, VeronicaGarcia-Sage, KatherineRichardson, JohnClark, JohnHsu, SeanAchterberg, RichardSergis, NickPaganelli, FloraKempf, SashaOrton, GlennPortyankina, GannaJones, GeraintEconomou, ThanasisLivengood, TimothyKrimigi, StamatiosSzalay, JamesJackman, CatrionaValek, PhillipLecacheux, AlainColwell, JoshuaJasinski, JamieTosi, FedericoSulaiman, AliGaland, MarinaKotova, AnnaKhurana, KrishanKivelson, MargaretStrobel, DarrellRadiota, AikaterinaEstrada, PaulLivi, StefanoAzari, AbigailYates, JaphethAllegrini, FredericVogt, MarissaFelici, MariannaLuhmann, JanetFilacchione, GianricoMoore, Luke
Source
2020n3i176
Subject
Astrophysics - Earth and Planetary Astrophysics
Language
Abstract
Future remote sensing of exoplanets will be enhanced by a thorough investigation of our solar system Ice Giants (Neptune-size planets). What can the configuration of the magnetic field tell us (remotely) about the interior, and what implications does that field have for the structure of the magnetosphere; energy input into the atmosphere, and surface geophysics (for example surface weathering of satellites that might harbour sub-surface oceans). How can monitoring of auroral emission help inform future remote observations of emission from exoplanets? Our Solar System provides the only laboratory in which we can perform in-situ experiments to understand exoplanet formation, dynamos, systems and magnetospheres.
Comment: Exoplanet Science Strategy White Paper, submitted to the National Academies of Sciences, Engineering and Medicine, Space Studies Board, 9 March 2018