Evolution of Comet p/ Halley in Early 1986MARCH as Observed from VEGA Pictures

Details Evolution of Comet p/ Halley in Early 1986MARCH as Observed from VEGA Pictures Evolution of Comet p/ Halley in Early 1986MARCH as Observed from VEGA Pictures

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...187..829a&link_type=abstract

Astronomy and Astrophysics, Vol.187, NO. 1+2/NOV, P. 829, 1987

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

From 4 to 10 march 1986, the internal dust coma of comet P/Halley was observed every day with Vega-1 and 2 narrow angle cameras of TVS system. The distribution of dust was monitored within 30,000 km from the nucleus. Strong variations are observed from one day to the other, indicating corresponding variations of the nucleus activity. These variations affect both the overall dust number density and the shape of its distribution around the nucleus. Dust intensities are given in absolute units of brightness.

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