An improved solution of the gravity field of Mars (GMM‐2B) from Mars Global Surveyor

By F. LeMoine, David E. Smith, D. Rowlands, Maria T. Zuber, G. Neumann, D. Chinn, D. Pavlis. 2001

287 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/476ae14e6cc20b165cd81ec01a6e6e6247168ab5

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In Astronomy and Astrophysics

Citations in the corpus

Mars high resolution gravity fields from MRO, Mars seasonal gravity, and other dynamical parameters (2011, methodology): “…altitude of the MRO spacecraft (255 km periapse) enables a higher resolution gravity field model determination than previous models (Smith et al., 1999a; Lemoine et al., 2001; Yuan et al., 2001; Konopliv et al., 2006; Marty et al., 2009) based upon the higher altitude MGS and Mars Odyssey orbits.”
Orbit determination of the Lunar Reconnaissance Orbiter (2012, methodology): “Compared to the MOLA analysis (Lemoine et al. 2001), the maximum slope was relaxed (from 0.”
Thickness of the Martian crust: Improved constraints from geoid-to-topography ratios (2004, methodology): “A number of such studies have been performed, especially since the Mars Global Surveyor (MGS) mission dramatically improved our knowledge of both the gravity field [Lemoine et al., 2001; Yuan et al., 2001] and topography [Smith et al.”
Constraints on the Martian lithosphere from gravity and topography data and implication for volcanism and possible mantle heterogeneities (2005, methodology): “, 2001], and the employed gravity model is jgm85h02 [Lemoine et al., 2001].”
Correction to “Localized gravity/topography admittance and correlation spectra on Mars: Implications for regional and global evolution” (2004, methodology): “In this paper, we use potential field expansion mgm1025 [Lemoine et al., 2001].”
High‒degree gravity models from GRAIL primary mission data (2013, methodology): “GEODYN has previously been used to analyze planetary orbiter tracking data to the Moon and Mars [Lemoine et al., 1997, 2001; Mazarico et al., 2009, 2010; Matsumoto et al., 2010; Goossens et al., 2011a].”
Crustal structure of Mars from gravity and topography (2004, methodology): “[ 71 ] At 400+ mGal amplitude, the Noachian-age Isidis impact basin forms one of the largest mascon gravity highs in the solar system [ Lemoine et al. , 2001].”
Gravity and Topography of the Terrestrial Planets (2015, background): “A major improvement in the gravity solutions came with the acquisition of data from the MGS mission (see Konopliv et al., 2006; Lemoine et al., 2001; Yuan et al., 2001).”
Ages of very large impact basins on Mars: Implications for the late heavy bombardment in the inner solar system (2008, background): “, 2004] and separately in gravity models as a pronounced circular anomaly [Lemoine et al., 2001].”