THE DETERMINATION OF VENUS GRAVITY FIELD WITH VERITAS.

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dc.contributor.authorGiuliani, F.
dc.contributor.authorDurante, D.
dc.contributor.authorIess, L.
dc.contributor.authorMarchi, F. De
dc.contributor.authorCascioli, Gael
dc.contributor.authorMazarico, E.
dc.contributor.authorSmrekar, S.
dc.date.accessioned2026-01-06T20:51:49Z
dc.date.issued2024
dc.description.abstractThe Venus Emissivity, Radio Science, InSAR, Topography and Spectroscopy (VERITAS) NASA Discovery mission will address important scientific questions about Venus’ evolution, structure, and past and on-going geological processes by collecting data from a gravity science experiment, and two instruments: an X-band interferometric SAR (VISAR), and a near-infrared imaging spectrometer (VEM). VERITAS, during the Science Phase 2, relevant for gravity data collection, will orbit Venus for 4 Venusian cycles (2.7 years) on a near - polar, near – circular, low altitude orbit.
dc.description.urihttps://www.scienzeplanetarie.it/files/download/Edizioni-precedenti/Bormio-2024/Posters/140.Giuliani_CNSP2024.pdf
dc.format.extent2 pages
dc.genrejournal articles
dc.genrepreprints
dc.identifierdoi:10.13016/m2eyfp-ckje
dc.identifier.urihttp://hdl.handle.net/11603/41376
dc.language.isoen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rightsPublic Domain
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.titleTHE DETERMINATION OF VENUS GRAVITY FIELD WITH VERITAS.
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0001-9070-7947

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