| Abstract |
Within the 10 years, next generation telescopes such as TPF
and will be capable of directly observation Extrasolar planets and
collecting spectrography data from them. The theoretical framework for
interpreting that data needs a strong foundation based on comparisons
to the solar system planets. In this presentation I discuss preliminary
observations performed at Hiroshima Observatory and plans for future
Antarctic observations, which together will create a planet observation
library for comparison with Extrasolar planet simulations and
observations. |
Spring
2008 Schedule