株式会社極東書店トップ ＞ 商品一覧 ＞ Satellites of the Outer Solar System: Exchange Processes Involving the Interiors. 2010 ed.
商品詳細
Satellites of the Outer Solar System: Exchange Processes Involving the Interiors. 2010 ed.
・ISBN 978-1-4614-2780-3 paper EUR 199.99
￥53,456.- (税込) ※（※）価格はご注文時の参考価格となります。
納品価格につきましては書籍の入荷時点で確定となります。
版元の原価改定、外国為替の変動等により異なる場合がございますので、予めご了承下さい。
お気に入り
★★★
| 著者・編者 | Grasset, O. / Blanc, M. / Coustenis, A. / Durham, William / Hussmann, H. / Pappalardo, R. / Turrini, D. (eds.), |
|---|---|
| シリーズ | (Space Sciences Series of ISSI) |
| 出版社 | (Springer-Verlag New York Inc., US) |
| 出版年月 | 2013 |
| ページ数 | 536 pp. |
| 言語 | ENG |
| ニュース番号 | ＜A05-53226＞ |
解説
Recent space missions to the outer solar system, Galileo (1996-2003) and Cassini-Huygens (2004-today), together with ground observations, have revealed that the moons of the outer solar system are enigmatic objects, introducing extraordinary challenges for geologists, astrobiologists, organic chemists, and planetologists. Chemical exchange exists through the different layers that form their interiors, and also from the interior to the surface. The most convincing evidence is certainly the discovery of water vapour and ice particles emerging from Enceladus's active south polar region. Evidence for exchange with a subsurface liquid ocean has also been provided by the inference of hydrated salts on the surfaces of Jupiter's moons, Europa and Ganymede, as well as the detection of sodium salts in particles originating in Enceladus's plumes. Aqueous exchange with the rocky core may also be possible, considering that 40Ar has been observed in the plumes of Enceladus during one flyby of Cassini and in the atmosphere of Titan. The ongoing CH4 replenishment in Titan's atmosphere is additional striking evidence of exchange processes within the moons.