Show simple item record

dc.contributor.authorLemoine, Frank G.
dc.contributor.authorGoossens, Sander
dc.contributor.authorSabaka, Terence J.
dc.contributor.authorNicholas, Joseph B.
dc.contributor.authorMazarico, Erwan Matias
dc.contributor.authorRowlands, David D.
dc.contributor.authorLoomis, Bryant D.
dc.contributor.authorChinn, Douglas S.
dc.contributor.authorNeumann, Gregory A.
dc.contributor.authorSmith, David Edmund
dc.contributor.authorZuber, Maria
dc.date.accessioned2015-07-31T12:30:00Z
dc.date.available2015-07-31T12:30:00Z
dc.date.issued2014-05
dc.date.submitted2014-03
dc.identifier.issn00948276
dc.identifier.urihttp://hdl.handle.net/1721.1/97930
dc.description.abstractWe 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[superscript −4]/ℓ[superscript 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.en_US
dc.language.isoen_US
dc.publisherAmerican Geophysical Union (AGU)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1002/2014GL060027en_US
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs Licenseen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/en_US
dc.sourceAmerican Geophysical Unionen_US
dc.titleGRGM900C: A degree 900 lunar gravity model from GRAIL primary and extended mission dataen_US
dc.typeArticleen_US
dc.identifier.citationLemoine, Frank G., Sander Goossens, Terence J. Sabaka, Joseph B. Nicholas, Erwan Mazarico, David D. Rowlands, Bryant D. Loomis, et al. “GRGM900C: A Degree 900 Lunar Gravity Model from GRAIL Primary and Extended Mission Data.” Geophysical Research Letters 41, no. 10 (May 28, 2014): 3382–3389.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorMazarico, Erwan Matiasen_US
dc.contributor.mitauthorSmith, David Edmunden_US
dc.contributor.mitauthorZuber, Mariaen_US
dc.relation.journalGeophysical Research Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsLemoine, Frank G.; Goossens, Sander; Sabaka, Terence J.; Nicholas, Joseph B.; Mazarico, Erwan; Rowlands, David D.; Loomis, Bryant D.; Chinn, Douglas S.; Neumann, Gregory A.; Smith, David E.; Zuber, Maria T.en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-2652-8017
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record