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      Descent trajectory reconstruction and landing site positioning of Chang’E-4 on the lunar farside

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          Abstract

          Chang’E-4 (CE-4) was the first mission to accomplish the goal of a successful soft landing on the lunar farside. The landing trajectory and the location of the landing site can be effectively reconstructed and determined using series of images obtained during descent when there were no Earth-based radio tracking and the telemetry data. Here we reconstructed the powered descent trajectory of CE-4 using photogrammetrically processed images of the CE-4 landing camera, navigation camera, and terrain data of Chang’E-2. We confirmed that the precise location of the landing site is 177.5991°E, 45.4446°S with an elevation of −5935 m. The landing location was accurately identified with lunar imagery and terrain data with spatial resolutions of 7 m/p, 5 m/p, 1 m/p, 10 cm/p and 5 cm/p. These results will provide geodetic data for the study of lunar control points, high-precision lunar mapping, and subsequent lunar exploration, such as by the Yutu-2 rover.

          Abstract

          The Chang’E-4 mission in January 2019 had the major challenge to land on the lunar far side without traditional radiometric techniques due to the missing line-of-sight. The authors here describe landing trajectory reconstruction and positioning techniques based upon the Moon’s digital terrain model that allowed reproducing the entire process of a successful landing.

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          Interior structure and seasonal mass redistribution of Mars from radio tracking of Mars Pathfinder.

          Doppler and range measurements to the Mars Pathfinder lander made using its radio communications system have been combined with similar measurements from the Viking landers to estimate improved values of the precession of Mars' pole of rotation and the variation in Mars' rotation rate. The observed precession of -7576 +/- 35 milliarc seconds of angle per year implies a dense core and constrains possible models of interior composition. The estimated annual variation in rotation is in good agreement with a model of seasonal mass exchange of carbon dioxide between the atmosphere and ice caps.
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            GRGM900C: A degree 900 lunar gravity model from GRAIL primary and extended mission data

            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/ℓ 2 was applied only for degree ℓ 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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              Martian precession and rotation from Viking lander range data

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                Author and article information

                Contributors
                licl@nao.cas.cn
                Journal
                Nat Commun
                Nat Commun
                Nature Communications
                Nature Publishing Group UK (London )
                2041-1723
                24 September 2019
                24 September 2019
                2019
                : 10
                : 4229
                Affiliations
                [1 ]ISNI 0000000119573309, GRID grid.9227.e, Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, , Chinese Academy of Sciences, ; Beijing, 100101 China
                [2 ]ISNI 0000 0004 1797 8419, GRID grid.410726.6, School of Astronomy and Space Science, University of Chinese Academy of Sciences, ; Beijing, 100049 China
                [3 ]ISNI 0000 0001 0243 138X, GRID grid.464215.0, China Academy of Space Technology, ; Beijing, 100094 China
                Author information
                http://orcid.org/0000-0002-2418-4495
                http://orcid.org/0000-0002-7560-6707
                http://orcid.org/0000-0002-0817-2742
                http://orcid.org/0000-0002-2516-1439
                http://orcid.org/0000-0002-9421-7387
                Article
                12278
                10.1038/s41467-019-12278-3
                6760200
                31551413
                0c383fa6-c21f-4c38-b677-d7aab5a4f748
                © The Author(s) 2019

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 23 January 2019
                : 23 August 2019
                Funding
                Funded by: FundRef https://doi.org/10.13039/501100001809, National Natural Science Foundation of China (National Science Foundation of China);
                Award ID: 11941002
                Award ID: 11941002
                Award ID: 11941002
                Award ID: 11941002
                Award Recipient :
                Funded by: National Natural Science Foundation of China (Grant No.11941002)
                Categories
                Article
                Custom metadata
                © The Author(s) 2019

                Uncategorized
                rings and moons,planetary science
                Uncategorized
                rings and moons, planetary science

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