Abstract
Brown dwarfs have masses intermediate to stars and planets, but their atmospheres can span planetary plasma conditions as they cool over time. They are more directly observable than the currently known extrasolar planets. In this paper, we provide a brief summary of the atmospheric properties of brown dwarfs, and apply this knowledge to predict the thermal and spectral properties of extrasolar planets.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 247-252 |
| Number of pages | 6 |
| Journal | European Space Agency, (Special Publication) ESA SP |
| Issue number | 539 |
| State | Published - Apr 2003 |
| Externally published | Yes |
| Event | Proceedings of the Conference - Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets - Heidelberg, Germany Duration: Apr 22 2003 → Apr 25 2003 |
ASJC Scopus subject areas
- Aerospace Engineering
- Space and Planetary Science