The Collision of Comet Shoemaker-Levy 9 and Jupiter: IAU by Keith S. Noll, Harold A. Weaver, Paul D. Feldman PDF

By Keith S. Noll, Harold A. Weaver, Paul D. Feldman

ISBN-10: 0511525052

ISBN-13: 9780511525056

ISBN-10: 0521031621

ISBN-13: 9780521031622

ISBN-10: 0521561922

ISBN-13: 9780521561921

The mind-blowing collision of Comet Shoemaker-Levy nine with Jupiter in July 1994 was once a different occasion within the historical past of astronomy. With a year's enhance caution, astronomers and planetary scientists world wide have been capable of coordinate an gazing crusade to trace the development in unheard of element. A yr after the development, a workshop on the area Telescope technology Institute supplied the 1st chance for them to assemble their observations and foster a brand new knowing of the impression. during this publication, the editors current fifteen invited stories from authors chosen as foreign leaders within the learn of the influence and its aftermath. they've got edited and organized the chapters to supply a radical and entire evaluation of our wisdom of the development. whereas our realizing of the effect will evolve with destiny paintings, this e-book offers a high-quality starting place for brand spanking new insights.

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Extra info for The Collision of Comet Shoemaker-Levy 9 and Jupiter: IAU Colloquium 156 (Space Telescope Science Institute Symposium Series)

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25, 1042. KARY, D. , SZ DONES, L. 1995 Capture statistics of short-period comets: Implications for comet Shoemaker-Levy 9. Icarus, (submitted). KRESAK, L. 1979 Dynamical interrelations among comets and asteroids. In Asteroids, (ed. T. Gehrels). pp. 289-309. University of Arizona Press. LAGAGE, P. , ALDEMARD, P. , BELMONTE, J. , REGULO, C , RODRIGUEZ ESPINOSA, J. , SZ GAUTIER, D. 1995 Collision of Shoemaker-Levy 9 fragments A, E, H, L, Ql with Jupiter: Mid-Infrared light curves. Geophys. Res. Lett 22, 1773-1776.

Observers typically captured several fragments in each of their astrometric images, and reduced the positions of all the fragments using the same stars. Our technique took advantage of the fact that errors in the star positions produced the same measurement bias for all fragments in a given observation set. ) The measurement bias can be seen clearly in a plot of the fragment residuals in a given set. The residuals typically cluster around a point offset from the origin by a few tenths of an arc second, P.

16 54 75 82 53 193 120 268 272 281 249 63 107 35 19 273 185 239 35 26 55 180 Impact Obs. s. Orbit Ref. 26 TABLE 2. Summary of orbit solutions. The data interval indicates the dates of the first and last observations used in the solutions, excluding the impact observation. The number of observations similarly excludes the impact observation. The following column indicates whether the impact time was used as an observation in the solution. The final two columns give the weighted rms residual and the orbit reference identifier.

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The Collision of Comet Shoemaker-Levy 9 and Jupiter: IAU Colloquium 156 (Space Telescope Science Institute Symposium Series) by Keith S. Noll, Harold A. Weaver, Paul D. Feldman


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