Download Cometary Science after Hale-Bopp: Volume 2 Proceedings of by Nicolas Biver, Dominique Bockelée-Morvan, Pierre Colom, PDF

By Nicolas Biver, Dominique Bockelée-Morvan, Pierre Colom, Jacques Crovisier (auth.), H. Boehnhardt, M. Combi, M. R. Kidger, R. Schulz (eds.)

Comet Hale-Bopp defines a milestone occasion for cometary technological know-how: it's the first "really tremendous" comet saw with smooth gear at the floor and from area and thanks to that; it really is thought of the recent reference item in cometary sciences.

At the start of a brand new period in spacecraft exploration of comets and 5 years after Hale-Bopp's perihelion passage those lawsuits of invited and contributed papers for IAU Colloquium 186 "Cometary technology after Hale-Bopp" evaluation the state of the art wisdom on comets, the icy, dusty and so much primordial left-overs of the formation disk of our personal sunlight procedure.

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Extra resources for Cometary Science after Hale-Bopp: Volume 2 Proceedings of IAU Colloquium 186 21–25 January 2002, Tenerife, Spain

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N- 2O 000 lOCI ... ,. , ,.. ' lAlJl .. c - 30· · .. N e ~ II ;, .. -,-·11; "! '''' ,,.. ,,! ------~. : --~·e 000 "" ~-~-~-------~ ! ;:tl o 1 , , .. & iii 1 II- Ii' 10 11 Figure 2. Hale-Bopp nucleus: The partial mass loss due to sublimation Z, (in kg m- 2, vertical axis) versus solar distance r (in AU, horizontal axis). , the strip number n) is given as line label. Upper panel is for rotation axis of nucleus perpendicular to the orbital plane, s = 00. Lower panels are for f = 30 0 , 600 , and 90 0 .

The neck-line structure in comet Hale- Bopp on June 6, 1997. The 5 minute exposure began at 23:03:00 UT. The width of the image shown is approximately 30 arc min. This ESO Schmidt image was obtained by G. Pizarro using Kodak 4415 emulsion and a GG 385 filter for the Liller-Brandt program. a. 15 b. 83 Figure 6. A comparison of the appearance of comet Hale-Bopp in the polar and equatorial regions of the solar wind. Left. 15, 1997. The dust tail (b) is smooth and the plasma tail (a) is relatively undisturbed.

1. 494, 822-827. Lamy, P. , Weaver, H. : 1998, Astron. Astrophys. 335, L25-L29. Marsden, B. G. and Williams, G. : 1997, Catalog o/Cometary Orbits, edn. 12. : 2002, Adv. Space Res. 29, 691-704. 44 BEATA DZIAK-JANKOWSKA ET AL. : 1997, Astrophys. J. 478, 107-110. Weaver H. A. and Lamy, P. : 1999, Earth Moon Planets 79, 17-33. Weaver, H. , Feldman, P. , A'Hearn, M. , Brandt, 1. , and Randall, C. : 1996, IAUC6376. WIDE FIELD IMAGING AND THE VELOCITY STRUCTURE IN THE COMA OF HALE-BOPP WALTER M. HARRIS, JEFFREY P.

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