Helios

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Q664667




Helios-A and Helios-B are a pair of probes that were launched into heliocentric orbit to study solar processes. As a joint venture between German Aerospace Center (DLR) and NASA, the probes were launched from Cape Canaveral Air Force Station, Florida, on December 10, 1974, and January 15, 1976, respectively.

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    Helios spacecraft 2Helios spacecraft 2
    Luminosity of the [[zodiacal light]] along the orbit of Helios 2 as observed by the P16 photometer. The peak at 0.8 AU was caused by [[Comet West]] passing through the field of view.Luminosity of the zodiacal light along the orbit of Helios 2 as observed by the P16 photometer. The peak at 0.8 AU was caused by Comet West passing through the field of view.
    Helios spacecraftHelios spacecraft
    Auszeichnung für drei Physiker vom Institut für Reine und Angewandte Kernphysik der Christian-Albrechts-Universität (CAU) durch die amerikanische Weltraumbehörde NASA (Kiel 67.509)Auszeichnung für drei Physiker vom Institut für Reine und Angewandte Kernphysik der Christian-Albrechts-Universität (CAU) durch die amerikanische Weltraumbehörde NASA (Kiel 67.509)
    Bottom view of the Helios spacecraft showing the three Zodiacal light photometers P15, P30, and P90 as well as the South (S) micrometeoroid sensor.Bottom view of the Helios spacecraft showing the three Zodiacal light photometers P15, P30, and P90 as well as the South (S) micrometeoroid sensor.
    Brightness of the [[zodiacal light]] along the orbit of Helios 1 and 2 as observed by the P16 photometer; blue: inward, red: outward motion. The peak at 0.8 AU was caused by [[Comet West]] passing through the field of view.Brightness of the zodiacal light along the orbit of Helios 1 and 2 as observed by the P16 photometer; blue: inward, red: outward motion. The peak at 0.8 AU was caused by Comet West passing through the field of view.
    Brightness of the zodiacal light along the orbits of Helios 1 and 2 as observed by the P15 photometers; blue: inward, red: outward motion. The peak at 0.8 AU was caused by Comet West passing through the field of view.Brightness of the zodiacal light along the orbits of Helios 1 and 2 as observed by the P15 photometers; blue: inward, red: outward motion. The peak at 0.8 AU was caused by Comet West passing through the field of view.
    Helios - Attitude control electronicsHelios - Attitude control electronics
      TypeSubtypeDateDescriptionNotesSource
      commonsimageHelios spacecraft 2 Commons
      commonsimage[[:File:HeliosP16 radial profile.jpg|Luminosity of the zodiacal light along the orbit of Helios 2 as observed by the P16 photometer. The peak at 0.8 AU was caused by Comet West passing through the field of view.]] Commons
      commonsimageHelios spacecraft Commons
      commonsimageAuszeichnung für drei Physiker vom Institut für Reine und Angewandte Kernphysik der Christian-Albrechts-Universität (CAU) durch die amerikanische Weltraumbehörde NASA (Kiel 67.509) Commons
      commonsimageBottom view of the Helios spacecraft showing the three Zodiacal light photometers P15, P30, and P90 as well as the South (S) micrometeoroid sensor. Commons
      commonsimage[[:File:HeliosZLI.jpg|Brightness of the zodiacal light along the orbit of Helios 1 and 2 as observed by the P16 photometer; blue: inward, red: outward motion. The peak at 0.8 AU was caused by Comet West passing through the field of view.]] Commons
      commonsimageBrightness of the zodiacal light along the orbits of Helios 1 and 2 as observed by the P15 photometers; blue: inward, red: outward motion. The peak at 0.8 AU was caused by Comet West passing through the field of view. Commons
      commonsimageHelios - Attitude control electronics Commons