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The MESSENGER Venus Flybys: Opportunities for Synergy with Venus Express

Solomon, S.C. und McNutt, R.L. und Domingue, D.L. und Gold, R.E. und Svedhem, H. und Titov, D. und Helbert, J. (2006) The MESSENGER Venus Flybys: Opportunities for Synergy with Venus Express. In: Eos Trans. AGU Fall Meeting suppl., 87 (52), . American Geophysical Union Fall Meeting 2006, 2006-12-11 - 2006-12-15, San Francisco (USA).

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The trajectory of the MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) spacecraft, launched by NASA on 3 August 2004 and destined to be the first probe to orbit Mercury, includes two flybys of Venus during the period that the ESA Venus Express mission is operational in Venus orbit. MESSENGER's first Venus flyby occurred on 24 October 2006, at a closest approach distance of 3140 km, but no scientific observations were made because Venus was at superior conjunction and no direct communication with the MESSENGER spacecraft (or with Venus Express) was possible for an extended period. All MESSENGER instruments, however, will be trained on Venus during the spacecraft's second flyby on 6 June 2007, when closest approach will be at 300 km altitude over 12°S, 107°E, in the uplands of Ovda Regio. The Mercury Dual Imaging System will image the night side in near-infrared bands, and color and higher-resolution monochrome mosaics will be made of both the approaching and departing hemispheres. The Ultraviolet and Visible Spectrometer on the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) instrument will make profiles of atmospheric species on the day and night sides as well as observations of the exospheric tail on departure. The Visible and Infrared Spectrograph on MASCS will observe the planet near closest approach to sense cloud chemical properties and near-infrared returns from the lower atmosphere and surface. The laser altimeter will serve as a passive 1064-nm radiometer and will measure the range to one or more cloud decks for several minutes near closest approach. The combined observations of Venus Express and MESSENGER will permit simultaneous and complementary observations of particular value for characterization of the particle and field environment at Venus. MESSENGER's Energetic Particle and Plasma Spectrometer (EPPS) will observe charged particle acceleration at the Venus bow shock and elsewhere. The Magnetometer will provide measurements of the interplanetary magnetic field (IMF), bow shock signatures, and pickup ion waves as a reference for EPPS and Venus Express observations. The encounter will enable two-point measurements of IMF penetration into the Venus ionosphere, primary plasma boundaries, and the near-tail region. During the MESSENGER flyby the instruments on Venus Express will be operated to maximize the synergy between the two spacecraft for this unique opportunity

Dokumentart:Konferenzbeitrag (NICHT SPEZIFIZIERT)
Titel:The MESSENGER Venus Flybys: Opportunities for Synergy with Venus Express
AutorenInstitution oder E-Mail-Adresse der Autoren
Solomon, S.C.Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, N.W., Washington, DC 20015 United States
McNutt, R.L.The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 United States
Domingue, D.L.The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 United States
Gold, R.E.The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 United States
Svedhem, H.European Space Agency/ESTEC, Keplerlaan 1, Noordwijk, 2200 AG Netherlands
Titov, D.Max Planck Institute for Solar System Research, Max-Planck-Str.2, Katlenburg-Lindau, 37191 Germany
Datum:Dezember 2006
Erschienen in:Eos Trans. AGU Fall Meeting suppl.
Name der Reihe:Eos Transactions AGU
Stichwörter:Atmospheres, Interactions with particles and fields, Ionospheres, Surface materials and properties
Veranstaltungstitel:American Geophysical Union Fall Meeting 2006
Veranstaltungsort:San Francisco (USA)
Veranstaltungsart:internationale Konferenz
Veranstaltungsdatum:2006-12-11 - 2006-12-15
Veranstalter :AGU
HGF - Forschungsbereich:Verkehr und Weltraum (alt)
HGF - Programm:Weltraum (alt)
HGF - Programmthema:W EW - Erforschung des Weltraums
DLR - Schwerpunkt:Weltraum
DLR - Forschungsgebiet:W EW - Erforschung des Weltraums
DLR - Teilgebiet (Projekt, Vorhaben):W - Vorhaben Vergleichende Planetologie (alt)
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Planetenphysik
Hinterlegt von: Stefanie Musiol
Hinterlegt am:15 Jan 2007
Letzte Änderung:27 Apr 2009 13:25

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