Duration and extent of lunar volcanism: Comparison of 3D convection models to mare basalt ages
暂无分享,去创建一个
[1] E. Takahashi. Speculations on the Archean mantle: Missing link between komatiite and depleted garnet peridotite , 1990 .
[2] Ralf Jaumann,et al. Ages of Mare Basalts on the Lunar Nearside: A Synthesis , 2000 .
[3] D. Tritton,et al. Physical Fluid Dynamics , 1977 .
[4] Roger J. Phillips,et al. Potential anomalies on a sphere: Applications to the thickness of the lunar crust , 1998 .
[5] Stefano Mottola,et al. European Planetary Science Congress 2006 , 2008 .
[6] Alfred S. McEwen,et al. Lunar impact basins: New data for the western limb and far side (Orientale and South Pole‐Aitken Basins) from the first Galileo flyby , 1993 .
[7] L. Hood,et al. Limits on the lunar temperature profile , 1982 .
[8] G. Schubert,et al. Subsolidus convective cooling histories of terrestrial planets , 1979 .
[9] Stephen J. Mackwell,et al. 37th Annual Lunar and Planetary Science Conference , 2003 .
[10] T. Spohn,et al. The Longevity of Lunar Volcanism: Implications of Thermal Evolution Calculations with 2D and 3D Mantle Convection Models , 2001 .
[11] Alfred Edward Ringwood,et al. Origin of the Earth and Moon , 1979 .
[12] H. Haack,et al. Effects of regolith/megaregolith insulation on the cooling histories of differentiated asteroids , 1990 .
[13] P. Christensen,et al. Thermal conductivity measurements of particulate materials 2. Results , 1997 .
[14] James W. Head,et al. Lunar volcanism in space and time. , 1976 .
[15] A. Coradini,et al. Earth and Mars: early thermal profiles , 1983 .
[16] G. Schubert,et al. Whole planet cooling and the radiogenic heat source contents of the Earth and Moon , 1980 .
[17] P. Schultheiss,et al. Heat and fluid flux through sediment on the western flank of the Mid‐Atlantic Ridge: A hydrogeological study of North Pond , 1992 .
[18] L. Taylor,et al. Pre-4.2 AE mare-basalt volcanism in the lunar highlands , 1983 .
[19] Matthew E. Pritchard,et al. The Constitution and Structure of the Lunar Interior , 2006 .
[20] T. Spohn. Mantle differentiation and thermal evolution of Mars, Mercury, and Venus , 1991 .
[21] P. Spudis,et al. Beginning and end of lunar mare volcanism , 1983, Nature.
[22] Paul H. Warren,et al. Megaregolith thickness, heat flow, and the bulk composition of the Moon , 1985, Nature.
[23] Hood,et al. Improved gravity field of the moon from lunar prospector , 1998, Science.
[24] D. Breuer,et al. Influence of a variable thermal conductivity on the thermochemical evolution of Mars , 2006 .
[25] R. Jaumann,et al. Ages and stratigraphy of mare basalts in Oceanus Procellarum, Mare Nubium, Mare Cognitum, and Mare Insularum , 2003 .
[26] J. Vaisnys,et al. Contact thermal conductivity in lunar aggregates. , 1973 .
[27] J. Makino,et al. Evolution of a Circumterrestrial Disk and Formation of a Single Moon , 1999 .
[28] H. Wänke,et al. Early differentiation of the Moon: Evidence from trace elements in plagioclase , 1984 .
[29] David A. Yuen,et al. Various influences on plumes and dynamics in time-dependent, compressible mantle convection in 3-D spherical shell , 1996 .
[30] J. Kasting,et al. Evolution of a steam atmosphere during Earth's accretion. , 1988, Icarus.
[31] M. Robinson,et al. Constraints on the depth and variability of the lunar regolith , 2003 .
[32] M. Wieczorek,et al. Crustal thickness of the Moon: New constraints from gravity inversions using polyhedral shape models , 2007 .
[33] Roger J. Phillips,et al. The “Procellarum KREEP Terrane”: Implications for mare volcanism and lunar evolution , 2000 .
[34] Stephen J. Keihm,et al. Lunar Thermal Regime to 500 KM , 1977 .
[35] R. Canup,et al. Accretion of the Moon from an Impact-Generated Disk , 1995 .
[36] G. Schubert,et al. Magnetism and thermal evolution of the terrestrial planets , 1983 .
[37] W. Hartmann,et al. Origin of the Moon , 1986 .
[38] S. Taylor. Planetary science: A lunar perspective , 1982 .
[39] Tilman Spohn,et al. Thermal history of Mars and the sulfur content of its core , 1990 .
[40] Basaltic Volcanism Study. Basaltic volcanism on the terrestrial planets , 1981 .
[41] L. Taylor,et al. Petrologic constraints on the origin of the Moon , 1984 .
[42] Ulrich R. Christensen,et al. Some effects of lateral viscosity variations on geoid and surface velocities induced by density anomalies in the mantle , 1993 .
[43] Doris Breuer,et al. Three dimensional models of Martian mantle convection with phase transitions , 1998 .
[44] J. L. Chute,et al. Apollo 15 measurement of lunar surface brightness temperatures thermal conductivity of the upper 1 1/2 meters of regolith , 1973 .
[45] D. Tozer. The present thermal state of the terrestrial planets , 1972 .
[46] Philip R. Christensen,et al. Thermal conductivity measurements of particulate materials 1. A review , 1997 .
[47] R. Phillips,et al. Lunar Multiring Basins and the Cratering Process , 1999 .
[48] J. Head,et al. Definition and detailed characterization of lunar surface units using remote observations , 1976 .
[49] F. D. Stacey. Physics of the earth , 1977 .
[50] M. Ashby,et al. Micromechanisms of flow and fracture, and their relevance to the rheology of the upper mantle , 1978, Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences.
[51] A. Hagermann,et al. Derivation of globally averaged lunar heat flow from the local heat flow values and the Thorium distribution at the surface: expected improvement by the LUNAR-A Mission , 2001 .
[52] B. Jolliff,et al. New views of the Moon , 2006 .
[53] David J. Stevenson,et al. Origin of the Moon-The Collision Hypothesis , 1987 .
[54] J. Whitehead. Fluid models of geological hotspots , 1988 .
[55] H. Haack,et al. Megaregolith insulation and the duration of cooling to isotopic closure within differentiated asteroids and the Moon , 1990 .
[56] A. G. W. Cameron,et al. The origin of the moon and the single-impact hypothesis III. , 1991 .
[57] P. E. van Keken,et al. Cooling of the earth in the Archaean: Consequences of pressure-release melting in a hotter mantle , 1994 .
[58] Tilman Spohn,et al. Line heat-source measurements of the thermal conductivity of porous H2O ice, CO2 ice and mineral powders under space conditions , 1996 .
[59] H. Harder. Mantle convection and the dynamic geoid of Mars , 2000 .
[60] Lunar,et al. Concepts and Approaches for Mars Exploration , 2000 .
[61] P. C. Hess. Diapirism and the origin of high TiO2 mare glasses , 1991 .
[62] M. Nafi Toksöz,et al. Structure of the Moon , 1974 .
[63] J. Head,et al. Lunar mare volcanism: Stratigraphy, eruption conditions, and the evolution of secondary crusts , 1992 .
[64] S. Keihm,et al. The Revised Lunar Heat Flow Values , 1976 .
[65] T. Spohn,et al. Thermal history of the Moon: Implications for an early core dynamo and post-accertional magmatism , 1997 .
[66] G. Ryder. Lunar ferroan anorthosites and mare basalt sources: The mixed connection , 1991 .
[67] A. Konopliv,et al. Recent Gravity Models as a Result of the Lunar Prospector Mission , 2001 .
[68] L. Cathles,et al. The Viscosity of the Earth's Mantle , 1975 .
[69] K. Rasmussen,et al. Megaregolith insulation, internal temperatures, and bulk uranium content of the moon , 1987 .
[70] M. G. Langseth,et al. Surface brightness temperatures at the Apollo 17 heat flow site - Thermal conductivity of the upper 15 cm of regolith , 1973 .