| Title: |
Solar System Ice Giants: Exoplanets in our Backyard |
| Authors: |
Rymer, A; Mandt, K; Hurley, D; Lisse, C; Izenberg, N; Smith, HT; Westlake, J; Bunce, E; Arridge, C; Masters, A; Hofstadter, M; Simon, A; Brandt, P; Clark, G; Cohen, I; Allen, R; Vine, S; Hansen, K; Hospodarsky, G; Kurth, W; Romani, P; Lamy, L; Zarka, P; Cao, H; Paty, C; Hedman, M; Roussos, E; Cruikshank, D; Farrell, W; Fieseler, P; Coates, A; Yelle, R; Parkinson, C; Militzer, B; Grodent, D; Kollmann, P; McNutt, R; André, N; Strange, N; Barnes, J; Dones, L; Denk, T; Rathbun, J; Lunine, J; Desai, R; Cochrane, C; Sayanagi, KM; Postberg, F; Ebert, R; Hill, T; Mueller-Wodarg, I; Regoli, L; Pontius, D; Stanley, S; Greathouse, T; Saur, J; Marouf, E; Bergman, J; Higgins, C; Johnson, R; Thomsen, M; Soderlund, K; Jia, X; Wilson, R; Englander, J; Burch, J; Nordheim, T; Grava, C; Baines, K; Quick, L; Russell, C; Cravens, T; Cecconi, B; Aslam, S; Bray, V; Garcia-Sage, K; Richardson, J; Clark, J; Hsu, S; Achterberg, R; Sergis, N; Paganelli, F; Kempf, S; Orton, G; Portyankina, G; Jones, G; Economou, T; Livengood, T; Krimigi, S; Szalay, J; Jackman, C; Valek, P; Lecacheux, A; Colwell, J; Jasinski, J; Tosi, F; Sulaiman, A; Galand, M; Kotova, A; Khurana, K; Kivelson, M; Strobel, D; Radiota, A; Estrada, P; Livi, S; Azari, A; Yates, J; Allegrini, F; Vogt, M; Felici, M; Luhmann, J; Filacchione, G; Moore, L |
| Publication Year: |
2019 |
| Collection: |
Imperial College London: Spiral |
| Subject Terms: |
astro-ph.EP |
| Description: |
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. |
| Document Type: |
report |
| Language: |
unknown |
| Relation: |
http://hdl.handle.net/10044/1/65724 |
| Availability: |
http://hdl.handle.net/10044/1/65724 |
| Rights: |
© 2018 The Authors |
| Accession Number: |
edsbas.911AF3FA |
| Database: |
BASE |