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      GRGM900C: A degree 900 lunar gravity model from GRAIL primary and extended mission data

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          Abstract

          We have derived a gravity field solution in spherical harmonics to degree and order 900, GRGM900C, from the tracking data of the Gravity Recovery and Interior Laboratory (GRAIL) Primary (1 March to 29 May 2012) and Extended Missions (30 August to 14 December 2012). A power law constraint of 3.6 ×10 −4/ 2 was applied only for degree greater than 600. The model produces global correlations of gravity, and gravity predicted from lunar topography of ≥ 0.98 through degree 638. The model's degree strength varies from a minimum of 575–675 over the central nearside and farside to 900 over the polar regions. The model fits the Extended Mission Ka-Band Range Rate data through 17 November 2012 at 0.13 μm/s RMS, whereas the last month of Ka-Band Range-Rate data obtained from altitudes of 2–10 km fit at 0.98 μm/s RMS, indicating that there is still signal inherent in the tracking data beyond degree 900.

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          The crust of the Moon as seen by GRAIL.

          High-resolution gravity data obtained from the dual Gravity Recovery and Interior Laboratory (GRAIL) spacecraft show that the bulk density of the Moon's highlands crust is 2550 kilograms per cubic meter, substantially lower than generally assumed. When combined with remote sensing and sample data, this density implies an average crustal porosity of 12% to depths of at least a few kilometers. Lateral variations in crustal porosity correlate with the largest impact basins, whereas lateral variations in crustal density correlate with crustal composition. The low-bulk crustal density allows construction of a global crustal thickness model that satisfies the Apollo seismic constraints, and with an average crustal thickness between 34 and 43 kilometers, the bulk refractory element composition of the Moon is not required to be enriched with respect to that of Earth.
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            Gravity field of the Moon from the Gravity Recovery and Interior Laboratory (GRAIL) mission.

            Spacecraft-to-spacecraft tracking observations from the Gravity Recovery and Interior Laboratory (GRAIL) have been used to construct a gravitational field of the Moon to spherical harmonic degree and order 420. The GRAIL field reveals features not previously resolved, including tectonic structures, volcanic landforms, basin rings, crater central peaks, and numerous simple craters. From degrees 80 through 300, over 98% of the gravitational signature is associated with topography, a result that reflects the preservation of crater relief in highly fractured crust. The remaining 2% represents fine details of subsurface structure not previously resolved. GRAIL elucidates the role of impact bombardment in homogenizing the distribution of shallow density anomalies on terrestrial planetary bodies.
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              Venus Gravity: 180th Degree and Order Model

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                Author and article information

                Journal
                Geophys Res Lett
                Geophys Res Lett
                grl
                Geophysical Research Letters
                BlackWell Publishing Ltd (Oxford, UK )
                0094-8276
                1944-8007
                28 May 2014
                29 May 2014
                : 41
                : 10
                : 3382-3389
                Affiliations
                [1 ]NASA Goddard Space Flight Center Greenbelt, Maryland, USA
                [2 ]CRESST, University of Maryland, Baltimore County Baltimore, Maryland, USA
                [3 ]Emergent Space Technologies Greenbelt, Maryland, USA
                [4 ]Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology Cambridge, Massachusetts, USA
                [5 ]Stinger Ghaffarian Technologies Inc. Greenbelt, Maryland, USA
                Author notes
                Correspondence to: F. G. Lemoine, Frank.G.Lemoine@ 123456nasa.gov

                Citation: Lemoine, F. G., et al. (2014), GRGM900C: A degree 900 lunar gravity model from GRAIL primary and extended mission data

                Article
                10.1002/2014GL060027
                4459205
                9c67bd76-ce05-48d1-a419-17fd589a84ae
                ©2014. The Authors.

                This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.

                History
                : 25 March 2014
                : 27 April 2014
                Categories
                Research Letters

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