Literature DB >> 32454532

Improving the geometry of Kaguya extended mission data through refined orbit determination using laser altimetry.

Sander Goossens1,2, Erwan Mazarico2, Yoshiaki Ishihara3, Brent Archinal4, Lisa Gaddis4.   

Abstract

The Japan Aerospace Exploration Agency's (JAXA) Kaguya spacecraft carried a suite of instruments to map the Moon and its environment globally. During its extended mission, the average altitude was 50 km or lower, and Kaguya science products using these data hence have an increased spatial resolution. However, the geodetic position quality of these products is much worse than that of those acquired during the primary mission (at an altitude of 100 km) because of reduced radiometric tracking and frequent thrusting to maintain spacecraft attitude after the loss of momentum wheels. We have analyzed the Kaguya tracking data using gravity models based on the Gravity Recovery and Interior Laboratory (GRAIL) mission, and by making use of a new data type based on laser altimeter data collected by Kaguya: we adjust the spacecraft orbit such that the altimetry tracks fit a precise topographic basemap based on the Lunar Reconnaissance Orbiter's (LRO) Lunar Orbiter Laser Altimeter (LOLA) data. This results in geodetically accurate orbits tied to the precise LOLA/LRO frame. Whereas previously archived orbits show errors at the level of several a level of several tens of meters. When altimetry data are not available, the combination of GRAIL gravity and radio tracking results in an orbit precision of around several hundreds of meters for the low-altitude phase of the extended mission. Our greatly improved orbits result in better geolocation of the Kaguya extended mission data set.

Keywords:  Moon; data reduction techniques; orbit determination

Year:  2019        PMID: 32454532      PMCID: PMC7243822          DOI: 10.1016/j.icarus.2019.113454

Source DB:  PubMed          Journal:  Icarus        ISSN: 0019-1035            Impact factor:   3.508


  10 in total

1.  The shape of 433 eros from the NEAR-shoemaker laser rangefinder

Authors: 
Journal:  Science       Date:  2000-09-22       Impact factor: 47.728

2.  Constraints on the volatile distribution within Shackleton crater at the lunar south pole.

Authors:  Maria T Zuber; James W Head; David E Smith; Gregory A Neumann; Erwan Mazarico; Mark H Torrence; Oded Aharonson; Alexander R Tye; Caleb I Fassett; Margaret A Rosenburg; H Jay Melosh
Journal:  Nature       Date:  2012-06-20       Impact factor: 49.962

3.  Global distribution of large lunar craters: implications for resurfacing and impactor populations.

Authors:  James W Head; Caleb I Fassett; Seth J Kadish; David E Smith; Maria T Zuber; Gregory A Neumann; Erwan Mazarico
Journal:  Science       Date:  2010-09-17       Impact factor: 47.728

4.  The LCROSS cratering experiment.

Authors:  Peter H Schultz; Brendan Hermalyn; Anthony Colaprete; Kimberly Ennico; Mark Shirley; William S Marshall
Journal:  Science       Date:  2010-10-22       Impact factor: 47.728

5.  Lunar global shape and polar topography derived from Kaguya-LALT laser altimetry.

Authors:  H Araki; S Tazawa; H Noda; Y Ishihara; S Goossens; S Sasaki; N Kawano; I Kamiya; H Otake; J Oberst; C Shum
Journal:  Science       Date:  2009-02-13       Impact factor: 47.728

6.  Orbit determination of the Lunar Reconnaissance Orbiter: Status after Seven Years.

Authors:  Erwan Mazarico; Gregory A Neumann; Michael K Barker; Sander Goossens; David E Smith; Maria T Zuber
Journal:  Planet Space Sci       Date:  2017-10-12       Impact factor: 2.030

7.  Gravity field of the Moon from the Gravity Recovery and Interior Laboratory (GRAIL) mission.

Authors:  Maria T Zuber; David E Smith; Michael M Watkins; Sami W Asmar; Alexander S Konopliv; Frank G Lemoine; H Jay Melosh; Gregory A Neumann; Roger J Phillips; Sean C Solomon; Mark A Wieczorek; James G Williams; Sander J Goossens; Gerhard Kruizinga; Erwan Mazarico; Ryan S Park; Dah-Ning Yuan
Journal:  Science       Date:  2012-12-05       Impact factor: 47.728

8.  Farside gravity field of the moon from four-way Doppler measurements of SELENE (Kaguya).

Authors:  Noriyuki Namiki; Takahiro Iwata; Koji Matsumoto; Hideo Hanada; Hirotomo Noda; Sander Goossens; Mina Ogawa; Nobuyuki Kawano; Kazuyoshi Asari; Sei-Itsu Tsuruta; Yoshiaki Ishihara; Qinghui Liu; Fuyuhiko Kikuchi; Toshiaki Ishikawa; Sho Sasaki; Chiaki Aoshima; Kosuke Kurosawa; Seiji Sugita; Tadashi Takano
Journal:  Science       Date:  2009-02-13       Impact factor: 47.728

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

Authors:  Frank G Lemoine; Sander Goossens; Terence J Sabaka; Joseph B Nicholas; Erwan Mazarico; David D Rowlands; Bryant D Loomis; Douglas S Chinn; Gregory A Neumann; David E Smith; Maria T Zuber
Journal:  Geophys Res Lett       Date:  2014-05-29       Impact factor: 4.720

10.  Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements.

Authors:  Gregory A Neumann; Maria T Zuber; Mark A Wieczorek; James W Head; David M H Baker; Sean C Solomon; David E Smith; Frank G Lemoine; Erwan Mazarico; Terence J Sabaka; Sander J Goossens; H Jay Melosh; Roger J Phillips; Sami W Asmar; Alexander S Konopliv; James G Williams; Michael M Sori; Jason M Soderblom; Katarina Miljković; Jeffrey C Andrews-Hanna; Francis Nimmo; Walter S Kiefer
Journal:  Sci Adv       Date:  2015-10-30       Impact factor: 14.136

  10 in total

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