Gravity Field, Shape, and Moment of Inertia of Titan

被引:154
作者
Iess, Luciano [1 ]
Rappaport, Nicole J. [2 ]
Jacobson, Robert A. [2 ]
Racioppa, Paolo [1 ]
Stevenson, David J. [3 ]
Tortora, Paolo [4 ]
Armstrong, John W. [2 ]
Asmar, Sami W. [2 ]
机构
[1] Univ Roma La Sapienza, Dipartimento Ingn Aerospaziale & Astronaut, I-00184 Rome, Italy
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] CALTECH, Pasadena, CA 91125 USA
[4] Univ Bologna, DIEM II Fac Ingn, I-47100 Forli, Italy
关键词
AMMONIUM-SULFATE; SATELLITES;
D O I
10.1126/science.1182583
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Precise radio tracking of the spacecraft Cassini has provided a determination of Titan's mass and gravity harmonics to degree 3. The quadrupole field is consistent with a hydrostatically relaxed body shaped by tidal and rotational effects. The inferred moment of inertia factor is about 0.34, implying incomplete differentiation, either in the sense of imperfect separation of rock from ice or a core in which a large amount of water remains chemically bound in silicates. The equilibrium figure is a triaxial ellipsoid whose semi-axes a, b, and c differ by 410 meters (a - c) and 103 meters (b - c). The nonhydrostatic geoid height variations (up to 19 meters) are small compared to the observed topographic anomalies of hundreds of meters, suggesting a high degree of compensation appropriate to a body that has warm ice at depth.
引用
收藏
页码:1367 / 1369
页数:3
相关论文
共 12 条
  • [1] Constraints on gas giant satellite formation from the interior states of partially differentiated satellites
    Barr, Amy C.
    Canup, Robin M.
    [J]. ICARUS, 2008, 198 (01) : 163 - 177
  • [2] Ammonium sulfate on Titan: Possible origin and role in cryovolcanism
    Fortes, A. D.
    Grindrod, P. M.
    Trickett, S. K.
    Vocadlo, L.
    [J]. ICARUS, 2007, 188 (01) : 139 - 153
  • [3] The long-term stability of a possible aqueous ammonium sulfate ocean inside Titan
    Grindrod, P. M.
    Fortes, A. D.
    Nimmo, F.
    Feltham, D. L.
    Brodholt, J. P.
    Vocadlo, L.
    [J]. ICARUS, 2008, 197 (01) : 137 - 151
  • [4] Heiskanen W A, 1979, Physical Geodesy
  • [5] The gravity field of the Saturnian system from satellite observations and spacecraft tracking data
    Jacobson, R. A.
    Antreasian, P. G.
    Bordi, J. J.
    Criddle, K. E.
    Ionasescu, R.
    Jones, J. B.
    Mackenzie, R. A.
    Meek, M. C.
    Parcher, D.
    Pelletier, F. J.
    Owen, W. M., Jr.
    Roth, D. C.
    Roundhill, I. M.
    Stauch, J. R.
    [J]. ASTRONOMICAL JOURNAL, 2006, 132 (06) : 2520 - 2526
  • [6] Kaula WM., 1966, THEORY SATELLITE GEO, DOI DOI 10.1016/j.epsl.2014.05.003
  • [7] Rivers, Lakes, Dunes, and Rain: Crustal Processes in Titan's Methane Cycle
    Lunine, Jonathan I.
    Lorenz, Ralph D.
    [J]. ANNUAL REVIEW OF EARTH AND PLANETARY SCIENCES, 2009, 37 : 299 - 320
  • [8] Murray C.D., 1999, Solar System Dynamics
  • [9] Doppler measurements of the quadrupole moments of titan
    Rappaport, N
    Bertotti, B
    Giampieri, G
    Anderson, JD
    [J]. ICARUS, 1997, 126 (02) : 313 - 323
  • [10] The Galilean satellites
    Showman, AP
    Malhotra, R
    [J]. SCIENCE, 1999, 286 (5437) : 77 - 84