首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Determining a tilt in Titan’s north-south albedo asymmetry from Cassini images
Authors:Michael T Roman  Robert A West  Peter J Gierasch  Conor A Nixon
Institution:a Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
b MS 169-237, Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
c Department of Astronomy, University of Maryland, College Park, MD 20742, USA
Abstract:Analysis of Titan’s hemispheric brightness asymmetry from mapped Cassini images reveals an axis of symmetry that is tilted with respect to the rotational axis of the solid body. Twenty images taken from 2004 through 2007 show a mean axial offset of 3.8 ± 0.9° relative to the solid body’s pole, directed 79 ± 24° to the west of the sub-solar longitude. These values are consistent with recent measurements of an implied atmospheric spin axis determined from isothermal mapping by Achterberg, R.K., Conrath, B.J., Gierasch, P.J., Flasar, F.M., Nixon, C.A., 2008. Icarus 197, 549-555].
Keywords:Titan  Atmospheres  dynamics  Atmospheres  structure
本文献已被 ScienceDirect 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号