Physics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ncimc..16..769m&link_type=abstract
Nuovo Cimento C, Vol. 16, N. 6, p. 769 - 773
Physics
Comet 1992 Xviii Grigg-Skjellerup, Comets: Infrared Photometry
Scientific paper
After the encounter with the Giotto spacecraft, the comet P/Grigg-Skjellerup was observed with the 2.2 m ESO telescope. Imaging in the V and R bands and infrared photometry with the J and H filters were performed. From the radial enhancement of the images the authors derived that the R frame mainly concerns the dust tail of the comet. Thus they applied the inverse numerical method of dust tail analysis in order to estimate the following cometary-grain parameters: ejection velocity, anisotropy of the emission, size distribution and loss rate. This from the observations back in time to the Giotto encounter. From infrared observation one could calculate the J and H magnitudes and the colour index J-H = 0.4 consistent with previous measurements of the comet.
Bussoletti Ezio
Colangeli Luigi
Fulle Marco
Mennella Vito
Merluzzi Paola
No associations
LandOfFree
Comet P/Grigg-Skjellerup: ground-based observations after the encounter with the Giotto spacecraft. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Comet P/Grigg-Skjellerup: ground-based observations after the encounter with the Giotto spacecraft., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comet P/Grigg-Skjellerup: ground-based observations after the encounter with the Giotto spacecraft. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1301006