Planetary seismology

Annual Review of Earth and Planetary Sciences

Volumn 33, Issue , 2005, Pages 571-604

  Lognonné, Philippe ^a  

^a INSTITUT DE PHYSIQUE DU GLOBE DE PARIS   (France)

Author keywords

Interior; Mars; Moon; Terrestrial planets

Indexed keywords

DATA ACQUISITION; DATA REDUCTION; PLANETS;

APOLLO SEISMIC NETWORK; SEISMIC DATA; SEISMIC NOISE; TERRESTRIAL PLANETS;

SEISMOLOGY;

CORE (PLANETARY); MARS; MOON; SEISMOLOGY;

EID: 20744457236     PISSN: 00846597     EISSN: None     Source Type: Book Series    
DOI: 10.1146/annurev.earth.33.092203.122604     Document Type: Review

References (150)

1. Anderson DL, Miller WF, Latham GV, Nakamura Y, Toksoz MN, et al. 1977. Seismology on Mars. J. Geophys. Res. 82:4524-46
2. Artru J, Farges T, Lognonné P. 2004. Acoustic waves generated from seismic surface waves: propagation properties determined from Doppler sounding observation and normal-modes modeling. Geophys. J. Int. 158:1067-77
3. Ball AJ, Lognonné P, Seiferlin K, Pätzold M, Spohn T. 2004. Lander and penetrator science for NEO mitigation studies. In Mitigation of Hazardous Impacts Due to Asteroids and Comets, ed. MJS Belton, DKYeomans, TH Morgan, 266:291. Cambridge, UK: Cambridge Univ. Press
4. Banerdt B, Chicarro AF, Coradini M, Federico F, Greeley R, et al. 1996. InterMarsnet, Phase A study report. ESA Publ. SCI(96)2
5. Banerdt WB, Lognonné P. 2003. An autonomous instrument package for providing "Pathfinder" network measurements on the surface of Mars. Int. Conf. Mars, 6th, Pasadena, July 20-25, 2003, Abstr. No. 3221. Houston, TX: Lunar Planet. Inst.
6. Banerdt WB, Pike WT. 2001. A miniaturized seismometer for subsurface probing on Mars. Conf. Geophys. Detect. Subsurf. Water Mars, Houston, August 6-10, 2001, Abstr. No. 7056. Houston, TX: Lunar Planet. Inst.
7. Beauduin R, Lognonné P, Montagner JP, Cacho S, Karczewski JF, Morand M. 1996. The effect of the atmospheric pressure changes on seismic signals or how to improve the quality of a station. Bull. Seism. Soc. Am. 86:1760-69
8. Bills BG, Ferrari AJ. 1977. A lunar density consistent with topographic, gravitational, librational and seismic data. J. Geophys. Res. 82:1306-14
9. Bills BG, Rubincam DP. Constraints on density models from radial moments: applications to Earth, Moon, and Mars. J. Geophys. Res. 100:26305-16
10. Buck WR, Toksoz MN. 1980. The bulk composition of the Moon based on geophysical constraints. Proc. Lunar Planet. Sci. Conf., 11th, 3:2043-58. Houston, TX: Lunar Planet. Inst.
11. Butler C. 2003. France purges space programme in bid to survive budget crisis. Nature 423:103
12. Canup RM, Righter K, eds. 2000. Origin of the Earth and Moon. Tucson: Univ. Ariz. Press
13. Carr MH, Belton MJS, Chapman CR, Davies ME, Geissler P, et al. 1998. Evidence for a subsurface ocean on Europa. Nature 391:363
14. Chenet H. 2003. Etude de la structure interne de la Lune. PhD thesis. IPGP Univ. Paris Denis Diderot. http://tel.ccsd.cnrs.fr/ documents/archives0/00/00/58/39/index_fr.html
15. Chenet H, Lognonné P, Wieczorek MA, Mizutani H. 2004. A first crustal thickness map of the Moon with Apollo seismic data. Lunar Planet. Sci. Conf., 35th, Abstr. 1581. Houston, TX: Lunar Planet. Inst.
16. Cheng CH, Toksöz MN. 1978. Tidal stresses in the Moon. J. Geophys. Res. 83:854-53
17. Chicarro AF, Coradini M, Fulchignoni M, Hiller K, Knudsen JM, et al. 1993. Marsnet, phase A study report. ESA Publ. SCI(93)2
18. Chicarro AF, Coradini M, Fulchignoni M, Liede I, Lognonné P, et al. 1991. Marsnet, assessment study report. ESA Publ. SCI(91)6
19. Cooper MR, Kovach RL, Watkins JS. 1974. Lunar near surface structure. Rev. Geophys. Space Phys. 12:291-308
20. Dainty AM, Toksöz MN, Anderson KR, Pines PJ, Nakamura Y, Latham G. 1974. Seismic scattering and shallow structure of the Moon in Oceanus Procellarum. Moon 9:11-29
21. Davis PM. 1993. Meteoroid impacts as seismic sources on Mars. Icarus 105:469-78
22. Dehant V, Lognonné P, Sotin C. 2004. Netlander: a European mission to study the planet Mars. Planet. Space Sci. 52:977-85
23. Dreibus G, Wanke H. 1985. A volatile-rich planet. Meteoritics 20:367-82
24. Ducic V, Artru J, Lognonné P. 2003. Ionospheric remote sensing of the Denali Earthquake Rayleigh surface waves. Geophys. Res. Lett. doi:10.1029/2003GL017812
25. Duennebier F, Sutton GH. 1974. Thermal Moonquakes. J. Geophys. Res. 79:4351-64
26. Dziewonski AM, Anderson DL. 1981. Preliminary reference Earth model. Phys. Earth Planet. Int. 25:297-356
27. Gagnepain-Beyneix J, Gabsi T, Dayre P, Lognonné P. 2002. Apollo seismic data in mini-seed. http://ganymede.ipgp.jussieu.fr/GB/donnees/
28. Goins NR, Dainty AM, Toksöz MN. 1981a. Seismic energy release of the Moon. J. Geophys. Res. 86:378-88
29. Goins NR, Dainty AM, Toksöz N. 1981b Structure of the lunar highlands site Apollo 16. Geophys. Res. Lett. 8:29-32
30. Goins NR, Dainty AM, Toksöz MN. 1981c. Lunar seismology: the internal structure of the Moon. J. Geophys. Res. 86:5061-74
31. Goins NR, Lazarewicz AR. 1979. Martian seismicity. Geophys. Res. Lett. 6:368-70
32. Golombek MP, Banerdt WB, Tanaka KL, Tralli DM. 1992. A prediction of Mars seismicity from surface faulting. Science 258:979-81
33. Grasset O, Sotin C, Deschamps F. 2000. On the internal structure and dynamics of Titan. Planet. Space Sci. 48:617-36
34. Grimm RE. 2002. The Naiades: A Mars scout proposal for electromagnetic and seismic groundwater exploration. Presented at Am. Geophys. Union, Fall Meet., 2002, Abstr. #Pl2A-0368, San Fransisco
35. Gudkova TV, Zharkov VN. 1996a. The exploration of Martian interiors using the spheroidal oscillation method. Planet. Space Sci. 44:1223-30
36. Gudkova TV, Zharkov VN. 1996b. On investigation of Martian crust structure using the free oscillation method. Planet. Space Sci. 44:1231-36
37. Gudkova TV, Zharkov VN. 2002. The exploration of the lunar interior using torsional oscillations. Planet. Space Sci. 50:1037-48
38. Gudkova TV, Zharkov VN. 2004. Mars: interior structure and excitation of free oscillations. Phys. Earth Planet. Int. 142:1-22
39. Harder H, Christensen UR. 1996. A one plume model of martian mantle convection. Nature 380:507-9
40. Hartmann WK, Philllips RJ, Taylor GJ, eds. 1984. Origin of the Moon. Houston, TX: Lunar Planet. Inst.
41. Hillgren VJ, Gessmann CK, Li J. 2000. An experimental perspective on the light element in Earth's core. See Canup & Righter 2000, pp. 245-64
42. Hood LL. 1986. Geophysical constraints on the lunar interior. See Hartmann et al. 1984, pp. 361-410
43. Hood LL, Jones JH. 1987. Geophysical constraints on lunar bulk composition and structure: a reassessment. J. Geophys. Res. 92: E396-410
44. Hood LL, Mitchell DL, Lin RP, Acuna MH, Binder AB. 1999. Initial measurements of the lunar induced magnetic dipole moment using Lunar Prospector magnetometer data. Geophys. Res. Lett. 26:2327-30
45. Hood LL, Zuber MT. 2000. Recent refinements in geophysical constraints on lunar origin and evolution. See Canup & Righter 2000, pp.397-409
46. Horvath P, Latham GV, Nakamura Y, Dorman HJ. 1980. Lunar near surface shear wave velocities at the Apollo landing sites as inferred from spectral amplitude ratios. J. Geophys. Res. 85:6572-78
47. Khan A, Mosegaard K. 2001. New information on the deep lunar interior from an inversion of lunar free oscillation periods, Geophys. Res. Lett. 28:1791-94
48. Khan A, Mosegaard K. 2002. An inquiry into the lunar interior - A non-linear inversion of the Apollo seismic data. J. Geophy. Res. 107:doi:10.1029/2001JE001658
49. Khan AK, Mosegaard, Rasmussen KL. 2000. A new seismic velocity model for the Moon from a Monte Carlo inversion of the Apollo lunar seismic data. Geophys. Res. Lett. 27: 1591-94
50. Khan A, Mosegaard K, Williams JG, Lognonné P. 2004. Does the Moon possess a molten core? Probing the deep lunar interior using results from LLR and lunar prospector. J. Geophys. Res. 109:E09007, doi: 10.1029/2004JE002294
51. Khan A, Mosegaard K, Lognonne P, Wieczorek M. 2004. A look at the interior of Mars. Lunar Planet. Sci. Conf, 35th, Abstr. No. 1631. League City, TX: Lunar Planet. Inst.
52. Kobayashi N, Nishida K. 1998. Atmospheric excitation of planetary free oscillations. J. Physics: Cond. Matter 10:11557-60
53. Kovach RL, Chyba CF. 2001. Seismic detectability of a subsurface ocean on Europa. Icarus 150:279-87
54. Koyama J, Nakamura Y. 1979. Re-examination of the lunar seismic velocity structure based on the complete data set. Lunar Planet. Sci. Conf., 10th, pp. 685-87. Houston, TX: Lunar Planet. Inst.
55. Kuskov OL. 1995. Constitution of the Moon: 3. Composition of middle mantle from seismic data. Phys. Earth Planet. Int. 90:55-74
56. Kuskov OL. 1997. Composition of the Moon: 4. Composition of the mantle from seismic data. Phys. Earth Planet. Int. 102:239-57
57. Kuskov OL, Fabrichnaya OB. 1994. Constitution of the Moon: 2. Composition and seismic properties of the lower mantle. Phys. Earth Planet. Int. 83:197-216
58. Kuskov OL, Kronrod VA. 1998. Constitution of the Moon: 5. Constraints on composition, density, temperature and radius of a core. Phys. Earth. Planet. Int. 107:285-306
59. Kuskov OL, Kronrod VA. 2001. Core sizes and internal structure of Earth's and Jupiter's satellites. Icarus 151:204-27
60. Kuskov OL, Kronrod VA, Hood LL. 2002. Geochemical constraints on the seismic properties of the lunar mantle. Phys. Earth. Planet. Int. 134:175-89
61. Lammlein D. 1977. Lunar seismicity and tectonics. Phys. Earth Planet. Int. 14:224-73
62. Lammlein D, Latham GV, Dorman J, Nakamura Y, Ewing M. 1974. Lunar seismicity, structure and tectonics. Rev. Geophys. Space Phys. 12:1-21
63. Larmat CS, Capdeville Y, Montagner J, Banerdt B, Lognonné P, Vilotte J. 2002. Simulation of the effect of topography and crustal thickness on the Martian seismograms by the coupled method. Am. Geophys. Union Fall Meet., Abstr. #P62A-0367, San Francisco
64. Larson EWF, Ekström G. 2002. Determining surface wave arrival angle anomalies. J. Geophys. Res. 107:doi: 10.1029/2000JB000048
65. Latham G, Ewing M, Press F, Sutton G. 1969. The Apollo passive seismic experiment. Science 165:241-50
66. Latham GV, Ewing M, Dorman J, Press F, Toksöz N, et al. 1970. Seismic data from man-made impacts on the Moon. Science 170:620-26
67. Latham GV, Ewing M, Dorman J, Lammlein D, Press F, et al. 1971. Moonquakes. Science 174:687-92
68. Lee S, Zanolin M, Thode AM, Pappalardo RT, Makris NC. 2003. Probing Europa's interior with natural sound sources. Icarus 165:144-67
69. Lehner FE, Witt EO, Miller WF, Gurney RD. 1962. A seismometer for lunar experiments. J. Geophys. Res. 67:4779-86
70. Linkin V, Harri AM, Lipatov A, Belostotskaja K, Derbunovich B, et al. 1998. A sophisticated lander for scientific exploration of Mars: Scientific objectives and implementation of the Mars96 Small Station. Planet. Space Sci. 46:717-37
71. Lodders K, Fegley B. 1997. An oxygen isotope model for the composition of Mars. Icarus 126:373-94
72. Lognonné P, Banerdt WB. 2003. Rationale for seismic measurements on Mars by a single station. Int. Conf. Mars, 6th, Pasadena, Abstr. No. 3225. Houston, TX: Lunar Planet. Inst.
73. Lognonné P, Clévédé E. 2002. Chapter 10: Normal modes of the Earth and planets. In Handbook on Earthquake and Engineering Seismology, IASPEI Centen. Publ., Int. Geophys. Ser. 81A, ed. H Kanamori, P Jennings, W Lee. San Diego, CA: Academic Press
74. Lognonné P, Zharkov VN, Karczewski JF, Romanowicz B, Menvielle M, et al. 1998a. The seismic optimism experiment. Planet. Space Sci. 46:739-47
75. Lognonné P, Clévédé C, Kanamori H. 1998b. Normal mode summation of seismograms and barograms in an spherical Earth with realistic atmosphere. Geophys. J. Int. 135:388-406
76. Lognonné P, Gagnepain-Beyneix J, Banerdt WB, Cacho S, Karczewski JF, Morand M. 1996. An ultra-broad band seismometer on InterMarsnet. Planet. Space Sci. 44:1237-49
77. Lognonné P, Gagnepain-Beyneix J, Chenet H. 2003a. A new seismic model of the Moon: implication in terms of structure, formation and evolution. Earth Planet. Sci. Lett. 6637:1-18
78. Lognonné P, Garcia R, Romanowicz B, Banerdt B. 2003b. A new concept for seismology on Venus using orbiting radar instead of landers. Am. Geophys. Union Fall Meet. Abstr., San Francisco
79. Lognonné P, Giardini D, Banerdt B, Gagnepain-Beyneix J, Mocquet A, et al. 2000. The NetLander very broad band seismometer. Planet. Space Sci. 48:1289-302
80. Lognonné P, Mosser B. 1993. Planetary seismology. Surv. Geophys. 14:239-302
81. Lognonné P, Mosser B, Dahlen FA. 1994. Excitation of the Jovian seismic waves by the Shoemaker-Levy 9 cometary impact. Icarus 110:186-95
82. Lognonné P, Spohn T, Giardini D. 2003c. Mars in depth. Astron. Astrophys. 44:15
83. Lognonné P, Gagnepain-Beyneix J, Chenet H, Spohn T. 2004. Constraints on the temperature and mineralogy of the Moon from a joint inversion of Apollo seismic, geodetic data and LP-clementine gravity data. Presented at Am. Geophys. Union, Fall Meet., 2004, Abstr. #G43A-0803, San Francisco
84. Lombardi D, Lognonné P, Gagnepain-Beyneix J, Gudkova T. 2002. Calibration des impacts naturels et artificiels sur la Lune ou Mercure. Colloq. Programme Natl. Planétol., Nantes, pp. 58-59
85. Loudin MG, Alexander SS. 1978. Observed estimates of spheroidal free oscillations of the Moon and their interpretation. EOS Trans. Am. Geophys. Union 59:1124
86. Marinangeli LL, Baines K, Garcia R, Drossart P, Piccioni G, et al. 2004. Venus surface investigation using VIRTIS onboard the ESA/Venus express mission. Lunar Planetary Sci. Conf., 35th, League City, TX, Abstr. No. 1363
87. Mark N, Sutton GH. 1975. Lunar shear velocity structure at Apollo sites 12, 14, and 15. J. Geophys. Res. 80:4932-38
88. Mizutani H. 1995. Lunar interior exploration by Japanese lunar penetrator mission, Lunar-A. J. Phys. Earth 43:657-70
89. Mizutani H, Fujimura, A, Tanaka S, Shiraishi H, Nakajima T. 2003. Lunar-A mission: goals and status. Adv. Space Res. 31:2315-21
90. Mocquet A. 1998. A search for the minimum number of stations needed for seismic networking on Mars. 1999. Planet. Space Sci. 47:397-409
91. Mocquet A, Vacher P, Grasset O, Sotin C. 1996. Theoretical seismic models of Mars: the importance of the iron content of the mantle. Planet. Space Sci. 44:1251-68
92. Mueller S, Taylor GJ, Phillips RJ. 1988. Lunar composition: a geophysical and petrological synthesis. J. Geophys. Res. 93:6338-52
93. Nakamura Y. 1976. Seismic energy transmission in the lunar surface zone determined from signals generated by movement of lunar rovers. Bull. Seismol. Soc. Am. 66:593-606
94. Nakamura Y. 1977a. Seismic energy transmission in an intensely scattering environment. J. Geophys. Res. 43:389-99
95. Nakamura Y. 1977b. HFT events - shallow Moonquakes. Phys. Earth Planet. Int. 14: 217-23
96. Nakamura Y. 1978. A1 Moonquakes: source distribution and mechanisms. Proc. Lunar Sci. Conf. 9:3589-607
97. Nakamura Y. 1983. Seismic velocity structure of the lunar mantle. J. Geophys. Res. 88:677-86
98. Nakamura Y. 2003. New identification of deep Moonquakes in the Apollo lunar seismic data. Phys. Earth Planet. Int. 139:197-205
99. Nakamura Y. 2005. Far-side deep Moonquakes and deep interior of the Moon. J. Geophys. Res. 110:E01001, doi: 10.1029/2004JE002332
100. Nakamura Y, Anderson DL. 1979. Martian wind activity detected by a seismometer at Viking lander 2 site. Geophys. Res. Lett. 6: 499-502
101. Nakamura Y, Dorman J, Duennebier F, Lammlein D, Latham G. 1975. Shallow lunar structure determined from the passive seismic experiment. Moon 13:57-66
102. Nakamura Y, Latham G, Lammlein D, Ewing M, Duennebier F, Dorman J. 1974. Deep lunar interior inferred from recent seismic data. Geophys. Res. Lett. 1:137-40
103. Nataf H, Ricard Y. 1996. 3SMAC: An a priori tomographic model of the upper mantle based on geophysical modeling. Phys. Earth Planet. Int. 95:101-22
104. Neal CR, Banerdt WB, Chenet H, Gagnepain-Beyneix J, Hood L, et al. 2004. The lunar seismic network: mission update. Lunar Planet. Sci. Conf., 35th, Abstr. No. 2093. Houston, TX: Lunar Planet. Inst.
105. Oberst J. 1987. Unusually high stress drop associated with shallow Moonquakes. J. Geophys. Res. 92:1397-405
106. Oberst J, Deuchler C, Wählisch M, Hauber E, Knapmeyer M, Spohn T. 2004. Where do the Mars quakes occur? Eur Geosci. Union EGU04-A-02939 (Abstr.)
107. Oberst J, Mizutani H. 2002. A new inventory of deep Moonquake nests visible at Apollo 12 area. Lunar Planet. Sci. Conf, 33th, Abstr. No. 1704. Houston, TX: Lunar Planet. Inst.
108. Oberst J, Nakamura Y. 1987. Distinct meteoroid families identified on the lunar seismograms. J. Geophys. Res. 92:E769-73
109. Oberst J, Nakamura Y. 1991. A search for clustering among the meteoroid impacts detected by the Apollo lunar seismic network. Icarus 91:315-25
110. Okal E, Anderson DJ. 1978. Theoretical models for Mars and their seismic properties Icarus 33:514-28
111. Phillips RJ. 1991. Expected rate of Marsquakes. In Scientific Rationale and Requirements for a Global Seismic Network on Mars, LPI Tech. Rep. 91-02, pp. 35-38. Houston: Lunar Planet. Inst.
112. Press F, Buwalda P, Neugebauer M. 1960. A lunar seismic experiment. J. Geophys. Res. 65:3097-105
113. Rhie A, Romanowicz B. 2004. Excitations of the Earth's incessant free oscillation by atmosphere/ocean/solid Earth coupling. Nature 431:552-56
114. Richardson JE, Melosh HJ, Greenberg R. 2004. Impact-induced seismic activity on asteroid 433 Eros: a surface modification. Science 306:1526-29
115. Righter K, Walker RJ, Warren PH. 2000. Significance of highly siderophile elements and osmium isotopes in the Lunar and terrestrial mantles. See Canup & Righter 2000, pp. 291-322
116. Ringwood AE, Essene E. 1970. Petrogenesis of Apollo 11 basalts, internal composition and origin of the Moon. Apollo 11 Lunar Sci. Conf. Proc., Geochim. Cosmochim. Acta 34:769-99
117. Sanloup C, Guyot F, Gillet P, Fei Y. 2002. Physical properties of liquid Fe alloys at high pressure and their bearings on the nature of metallic planetary cores. J. Geophys. Res. 107:doi: 10.1029/2001JB000808
118. Sanloup C, Jambon A, Gillet P. 1999. A simple chondritic model of Mars. Phys. Earth Planet. Int. 112:43-54
119. Sellers P. 1992. Seismic evidence for a low-velocity lunar core. J. Geophys. Res. 97: 11,663-72
120. Sohl F, Hussmann H, Schwentker B, Spohn T, Lorenz RD. 2003. Interior structure models and tidal Love numbers of Titan. J. Geophys. Res. 108:doi:10.1029/2003JE002044
121. Sohl F, Spohn T. 1997. The interior structure of Mars: implications from SNC meteorids. J. Geophys. Res. 102:1613-36
122. Sohl F, Spohn T, Breuer D, Nagel K. 2002. Implications from Galileo observations on the interior structure and chemistry of the Galilean satellites. Icarus 157:104-19
123. Solomon SC, Anderson DL, Banerdt WB, Butler RG, Davis PM, et al. 1991. Scientific rationale and requirements for a global nesimic network on Mars. LPI Tech. Rpt. 91-02, Lunar Planet. Inst., Houston, Tex. 51 pp.
124. Sotin, C, Rocad F, Lognonné P. 2000. Summary of the internationnal conference of Mars exploration program and sample return mission. Planet. Space Sci. 48:1143-44
125. Spohn T, Sohl F, Breuer D. 1998. Mars. Astron. Astrophys. Rev. 8:181-236
126. Stegman DR, Richards M, Jellinek M, Manga M, Baumgardner J. 2004. Response of stagnant-lid convection to sudden dichotomy formation. Presented at Am. Geophys. Union, Spring Meet. Abstr. #P33B-04
127. Stevenson DJ. 2001. Mars' core and magnetism. Nature 412:214-19
128. Stofan ER, Saunders RS, Senske D, Nock K, Tralli D, et al. 1993. Venus interior structure mission (VISM): Establishing a seismic network on Venus. Lunar Planet. Inst., Worksh. Adv. Technol. Planet. Instr., Part 1, pp. 23-24 (SEE N93-28764 11-91). Houston, TX: Lunar Planet. Inst.
129. Suda N, Mitani C, Kobayashi N, Nishida K. 2002. Theoretical calculation of Mars' background free oscillations. Am. Geophys. Union, Fall Meet., Abstr. #S12A-1186, San Francisco
130. Surkov Y.1989. Exploration of Terrestrial Planets from Spacecraft, pp. 372-73. New York: Ellis Horwood. 390 pp.
131. Tanimoto T. 2001. Continuous free oscillations: atmosphere-solid Earth coupling. Annu. Rev. Earth Planet. Sci. 29:563-84
132. Tanimoto T. 2005. The oceanic excitation hypothesis for the continuous oscillations of the Earth. Geophys. J. Int. 160:276-88, doi: 10.1111/j.1365-246X.2004.02484.x
133. Taylor SR. 1986. The origin of the Moon: geochemical considerations. In Origin of the Moon, ed. WK Hartmann, RJ Philllips, GJ Taylor, pp. 125-43. Houston, TX: Lunar Planet. Inst.
134. Taylor SR. 1987. The unique lunar composition and its bearing on the origin of the Moon. Geochim. Cosmochim. Acta 51:1297-309
135. Toksöz MN, Press F, Anderson K, Dainty A, Latham G, et al. 1972a. on. Lunar crust: structural and composition. Science 176:1012-16
136. Toksöz MN, Press F, Anderson K, Dainty A, Latham G, et al. 1972b. Velocity structure and properties of the lunar crust. Earth Moon Planets 4:490-504
137. Toksöz MN. 1974. Geophysical data and the interior of the Moon. Annu. Rev. Earth Planet. Sci. 2:151-77
138. Toksöz MN. 1975. Lunar and planetary seismology. Rev. Geophys. Space Phys. 13: 306
139. Toksöz MN. 1979. Planetary seismology and interiors. Rev. Geophys. Space Phys. 17: 1641-55
140. Toksöz MN, Dainty AM, Solomon SC, Anderson KR. 1974. Structure of the Moon. Rev. Geophys. Space Phys. 12:539-67
141. Yoder CF, Konopliv AS, Yuan DN, Standish EM, Folkner WM. 2003. Fluid core size of Mars from detection of the solar tide. Science 300:299-303
142. Vinnik L, Chenet H, Gagnepain-Beyneix J, Lognonné P. 2001. First seismic receiver functions on the Moon. Geophys. Res. Lett. 28:3031-34
143. Van Hoolst T, Dehant V, Roosbeek F, Lognonné P. 2003. Tidally induced surface displacements, external potential variations, and gravity variations on Mars. Icarus 161:281-96
144. Verhoeven O, Rivoldini A, Vacher P, Mocquet A, Choblet G, et al. 2004. Planetary interiors structure inferred from electromagnetic, geodetic and seismic network science. I: Forward problem and the case of Mars. J. Geophys. Res. In press
145. Walker JD, Huebner WF. 2004. Seismological investigation of asteroid and comet interiors. In Mitigation of Hazardous Impacts Due to Asteroids and Comets, ed. MJS Belton, DK Yeomans, TH Morgan, 234:265. Cambridge, UK: Cambridge Univ. Press
146. Wieczorek MA, Zuber MT. 2004. Thickness of the Martian crust: Improved constraints from geoid-to-topography ratios. J. Geophys. Res. 109:doi: 10.1029/2003JE002153
147. Williams JG, Boogs DH, Yoder CF, Racliff JT, Dickey JO. 2001. Lunar rotational dissipation in solid body and molten core. J. Geophys. Res. 106:27933-68
148. Zharkov VN, Gudkova TV. 1997. On the dissipative factor of Martian interiors. Planet. Space Sci. 45:401-7
149. Zharkov VN, Gudkova TV. 2000. Interior structure models, Fe/Si ratio and parameters of figure for Mars. Phys. Earth Planet. Int. 117:407-20
150. Zuber MT. 2001. The crust and mande of Mars. Nature 412:237-44