Dust activity of Comet Halley's nucleusImages obtained by the Halley multicolor camera using the clear filter with a pass band from 300 to 1000 nm were used to study dust activity in the comet nucleus. Comparisons with ground based observations confirm that dust production towards the Sun increases in activity relative to the southern background source while the Giotto spacecraft was approaching. This is in agreement with the assumption that the sunward activity becomes stronger when the source rotates towards the Sun. Estimated dust column density is 90 billion/sqm, with optical thickness less than or = 0.3. Surface reflectivity is less than 1%, indicating a very rough surface with large fractions of shadowed areas.
Document ID
19870016534
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Keller, H. U. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Delamere, W. A. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Huebner, W. F. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Reitsema, H. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Schmidt, H. U. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Schmidt, W. K. H. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Whipple, Fred L. (Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Wilhelm, K. (Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau, Germany)
Date Acquired
September 5, 2013
Publication Date
December 1, 1986
Publication Information
Publication: ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 2: Dust and Nucleus