オベロン_(衛星) - 暇つぶしWikipedia

オベロン_(衛星)

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^ a b 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.
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^ “No access | Nature Research”. Nature (2010年4月29日). 2019年1月16日閲覧。
^ a b c Bell, J. F., III; McCord, T. B. (1991). A search for spectral units on the Uranian satellites using color ratio images. Lunar and Planetary Science Conference, 21st, Mar. 12?16, 1990 (Conference Proceedings). Houston, TX, United States: Lunar and Planetary Sciences Institute. pp. 473?489. Bibcode:1991LPSC...21..473B。
^ a b c Helfenstein, P.; Hillier, J.; Weitz, C.; Veverka, J. (March 1990). “Oberon: Color Photometry and its Geological Implications”. Abstracts of the Lunar and Planetary Science Conference (Lunar and Planetary Sciences Institute, Houston) 21: 489?490. Bibcode: 1990LPI....21..489H.
^ 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 f g h Plescia, J.B. (1987). “Cratering history of the Uranian satellites: Umbriel, Titania and Oberon”. Journal of Geophysical Research 92 (A13): 14,918–32. doi:10.1029/JA092iA13p14918. https://ui.adsabs.harvard.edu/abs/1987JGR....9214918P/abstract.
^ a b Moore, Jeffrey M.; Schenk, Paul M.; Bruesch, Lindsey S.; Asphaug, Erik; McKinnon, William B. (October 2004). ⇒“Large impact features on middle-sized icy satellites” (PDF). Icarus 171 (2): 421?443. Bibcode: 2004Icar..171..421M. doi:10.1016/j.icarus.2004.05.009. ⇒http://planets.oma.be/ISY/pdf/article_Icy.pdf.
^ a b c d 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, Hoston. pp. 205C.
^ “Oberon: Mommur”. Gazetteer of Planetary Nomenclature. USGS Astrogeology. 2009年8月30日閲覧。
^ a b c Mousis, O. (2004). “Modeling the thermodynamical conditions in the Uranian subnebula ? Implications for regular satellite composition”. Astronomy & Astrophysics 413: 373?380. Bibcode: 2004A&A...413..373M. doi:10.1051/0004-6361:20031515.
^ a b Squyres, S. W.; Reynolds, Ray T.; Summers, Audrey L.; Shung, Felix (1988). “Accretional Heating of the Satellites of Saturn and Uranus”. Journal of Geophysical Research 93 (B8): 8779?8794. Bibcode: 1988JGR....93.8779S. doi:10.1029/JB093iB08p08779.

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