dc.contributor.author | Kopparapu, R | |
dc.contributor.author | Hebrard, E | |
dc.contributor.author | Belikov, R | |
dc.contributor.author | Batalha, NM | |
dc.contributor.author | Mulders, GD | |
dc.contributor.author | Stark, C | |
dc.contributor.author | Teal, D | |
dc.contributor.author | Domagal-Goldman, S | |
dc.contributor.author | Gelino, D | |
dc.contributor.author | Mandell, A | |
dc.contributor.author | Roberge, A | |
dc.contributor.author | Rinehart, S | |
dc.contributor.author | Kane, SR | |
dc.contributor.author | Hasegawa, Y | |
dc.contributor.author | Henning, W | |
dc.contributor.author | Hicks, B | |
dc.contributor.author | Adibekyan, V | |
dc.contributor.author | Schwieterman, EW | |
dc.contributor.author | Kohler, E | |
dc.contributor.author | Teske, J | |
dc.contributor.author | Hinkel, N | |
dc.contributor.author | Nixon, C | |
dc.contributor.author | France, K | |
dc.contributor.author | Danchi, W | |
dc.contributor.author | Haqq-Misra, J | |
dc.contributor.author | Wolf, ET | |
dc.contributor.author | Guzewich, SD | |
dc.contributor.author | Charnay, B | |
dc.contributor.author | Arney, G | |
dc.contributor.author | Hartnett, HE | |
dc.contributor.author | Lopez, ED | |
dc.contributor.author | Minniti, D | |
dc.contributor.author | Renaud, J | |
dc.contributor.author | Airapetian, V | |
dc.contributor.author | Dong, C | |
dc.contributor.author | Genio, ADD | |
dc.contributor.author | Trainer, M | |
dc.contributor.author | Rau, G | |
dc.contributor.author | Jensen, A | |
dc.contributor.author | Way, M | |
dc.contributor.author | Lisse, CM | |
dc.contributor.author | Lyra, W | |
dc.contributor.author | Marchis, F | |
dc.contributor.author | Jontof-Hutter, D | |
dc.contributor.author | Young, P | |
dc.contributor.author | Pierrehumbert, R | |
dc.contributor.author | Harman, CE | |
dc.contributor.author | Fortney, J | |
dc.contributor.author | Moore, B | |
dc.contributor.author | Beckwith, S | |
dc.contributor.author | Shock, E | |
dc.contributor.author | Desch, S | |
dc.contributor.author | Mandt, KE | |
dc.contributor.author | Izenberg, N | |
dc.contributor.author | Ford, EB | |
dc.contributor.author | Curry, S | |
dc.contributor.author | Scharf, C | |
dc.contributor.author | Anbar, A | |
dc.date.accessioned | 2018-03-23T11:43:28Z | |
dc.date.issued | 2018 | |
dc.description.abstract | This white paper discusses the diversity of exoplanets that could be detected by future observations, so that comparative exoplanetology can be performed in the upcoming era of large space-based flagship missions. The primary focus will be on characterizing Earth-like worlds around Sun-like stars. However, we will also be able to characterize companion planets in the system simultaneously. This will not only provide a contextual picture with regards to our Solar system, but also presents a unique opportunity to observe size dependent planetary atmospheres at different orbital distances. We propose a preliminary scheme based on chemical behavior of gases and condensates in a planet's atmosphere that classifies them with respect to planetary radius and incident stellar flux. | en_GB |
dc.identifier.uri | http://hdl.handle.net/10871/32207 | |
dc.language.iso | en | en_GB |
dc.publisher | NASA Goddard/University of Maryland | en_GB |
dc.relation.url | http://sites.nationalacademies.org/SSB/CurrentProjects/SSB_180659 | en_GB |
dc.title | Exoplanet diversity in the era of space-based direct imaging missions | en_GB |
dc.type | Working Paper | en_GB |
dc.date.available | 2018-03-23T11:43:28Z | |
dc.description | Community White Paper: submitted to the National Academy of Sciences Exoplanet Science Strategy | en_GB |
refterms.dateFOA | 2023-03-31T14:16:16Z | |