チタニア_(衛星)
[Wikipedia|▼Menu]
□記事を途中から表示しています
[最初から表示]

^ Lassell, W. (1850). “Bright Satellites of Uranus”. Monthly Notices of the Royal Astronomical Society 10 (6): 135. Bibcode: 1850MNRAS..10..135L. doi:10.1093/mnras/10.6.135. 
^ a b c d e f g h i j Grundy, W. M.; Young, L. A.; Spencer, J. R.; Johnson, R. E.; Young, E. F.; Buie, M. W. (2006-10). “Distributions of H2O and CO2 ices on Ariel, Umbriel, Titania, and Oberon from IRTF/SpeX observations”. Icarus 184 (2): 543?555. arXiv:0704.1525. Bibcode: 2006Icar..184..543G. doi:10.1016/j.icarus.2006.04.016. 
^ Ness, Norman F.; Acuna, Mario H.; Behannon, Kenneth W.; Burlaga, Leonard F.; Connerney, John E. P.; Lepping, Ronald P.; Neubauer, Fritz M. (1986-07). “Magnetic Fields at Uranus”. Science 233 (4759): 85?89. Bibcode: 1986Sci...233...85N. doi:10.1126/science.233.4759.85. PMID 17812894. 
^ Miller, C.; Chanover, N. J. (2009-03). “Resolving dynamic parameters of the August 2007 Titania and Ariel occultations by Umbriel”. Icarus 200 (1): 343?346. Bibcode: 2009Icar..200..343M. doi:10.1016/j.icarus.2008.12.010. 
^ a b c Tittemore, W. C. (1990-09). “Tidal heating of Ariel”. Icarus 87 (1): 110?139. Bibcode: 1990Icar...87..110T. doi:10.1016/0019-1035(90)90024-4. 
^ a b c d e f Hussmann, Hauke; Sohl, Frank; Spohn, Tilman (November 2006). “Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects”. Icarus 185 (1): 258?273. Bibcode: 2006Icar..185..258H. doi:10.1016/j.icarus.2006.06.005. https://www.researchgate.net/profile/Tilman_Spohn/publication/225019299_Subsurface_Oceans_and_Deep_Interiors_of_Medium-Sized_Outer_Planet_Satellites_and_Large_Trans-Neptunian_Objects/links/55018a3a0cf24cee39f7b952.pdf. 
^ a b c d Bell III, J.F.; McCord, T. B. (1991). A search for spectral units on the Uranian satellites using color ratio images. Lunar and Planetary Science Conference, 21st, March 12?16, 1990. Houston, TX, United States: Lunar and Planetary Sciences Institute. pp. 473?489. Bibcode:1991LPSC...21..473B。
^ a b c d e f g h i Plescia, J. B. (December 30, 1987). “Cratering history of the Uranian satellites: Umbriel, Titania and Oberon”. Journal of Geophysical Research 92 (A13): 14,918?14,932. Bibcode: 1987JGR....9214918P. doi:10.1029/JA092iA13p14918. ISSN 0148-0227. 
^ a b Buratti, Bonnie J.; Mosher, Joel A. (March 1991). “Comparative global albedo and color maps of the Uranian satellites”. Icarus 90 (1): 1?13. Bibcode: 1991Icar...90....1B. doi:10.1016/0019-1035(91)90064-Z. ISSN 0019-1035. 
^ a b c d e Croft, S. K. (1989). New geological maps of Uranian satellites Titania, Oberon, Umbriel and Miranda. Proceeding of Lunar and Planetary Sciences. Vol. 20. Lunar and Planetary Sciences Institute, Houston. p. 205C. Bibcode:1989LPI....20..205C。
次ページ
記事の検索
おまかせリスト
▼オプションを表示
ブックマーク登録
mixiチェック!
Twitterに投稿
オプション/リンク一覧
話題のニュース
列車運行情報
暇つぶしWikipedia

Size:79 KB
出典: フリー百科事典『ウィキペディア(Wikipedia)
担当:undef