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(100) ). ῎῍῏ῌ ´µ 2007, TU 5 c¶·&f ¸ Ida S., Lin D. N. C., 2004, ApJ 604, 388 Ida S., Lin D. N. C., 2008, ApJ 685, 584 Ida S., Lin D. N. C., 2005, ApJ 626, 1045 Tanaka H., Takauchi T., Ward W., 2002, ApJ 565, 1257 Masset F. S., Morbidelli A., Crida A., Ferreira J., 2006, ApJ 642, 478 7) Herbst W., Mundt R., 2005, ApJ 633, 967. 1) 2) 3) 4) 5) 6). |w ("D }
(101) "& VWX 5" ~% r=BBo " ywO o" "w )NOz[ Q ,( M X5"D G _`D OL"=1=vI= >2v= LM' Q )" "=1=vI=D ij5"D c῍VWT" . $. *N+ ij5. { az Q !" 5D" VW" w¡¢(N" £¤z o" "w. º 102 ». º3¼. Theory of Extrasolar Terrestrial Planets ῌῌFrom Super-Earths Shigeru IDA Tokyo Institute of Technology, 2῍12῍1, I2῍10 Ookayama, Meguro-ku, Tokyo 152῍8551, Japan Abstract : Super-Earths, rocky planets with mass of several to ¹20 earth massesare being observed. The observed data suggest that they have diversity in orbits as well as extrasolar Jovian planets, which stimulates further observations and formation/evolution theories of planets. Discussions of habitability will expand to Earth and life sciences through astronomy.. 183.
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