[meteorite-list] Tunguska Event Part 1 of 2
From: Bernd Pauli HD <bernd.pauli_at_meteoritecentral.com>
Date: Thu Apr 22 09:48:14 2004 Message-ID: <3BDD3F73.8618F4D6_at_lehrer1.rz.uni-karlsruhe.de> almitt wrote: > I'll leave the Tunguska event to someone else. Sky and Telescope, December 1978, pp. 497-498: The Tunguska Event and Encke's Comet Just what was it that collided with the earth on June 30, 1908, in central Siberia? A dazzlingly bright daytime fireball was seen, and over the site of its fall flames and a cloud of smoke appeared. Deafening explosions were heard at distances up to 1,000 km and were recorded on seismographs and barographs. To quote Lubor Kresak of the Slovak Academy of Sciences: "Hundreds of articles written on the unique Tunguska event of June 30, 1908, offer a variety of competitive explanations. Apart from the obvious fictions and speculations lacking [in] scientific objectivity (alien spacecraft, nuclear explosion, antimatter, black hole), every known type of interplanetary body crossing the orbit of the Earth has been suggested as the impacting object. The candidates include a small asteroid - or unusually large meteorite - ranging in composition from meteoric iron (Yavnel', 1957), to pre -type I carbonaceous chondrite (F.L. Whipple, 1967), and a small comet, extinct or active, with a dust tail (F.J.W. Whipple, 1930; Fesenkov, 1961 and 1966)." Writing in the Bulletin of the Astronomical Institutes of Czechoslovakia, Dr. Kresak presents strong grounds for surmising that the Tunguska object was in fact a fragment of Comet Encke, separated from it thousands of years ago. He begins by noting that although the impact energy seems to have been comparable to that expended in forming Arizona's Meteor Crater, no sizable crater was formed in the heavily damaged Tunguska area. This point favors a low- density impacting body. The only direct evidence concerning the orbit of the object before it entered the atmosphere is the position of its apparent radiant in the sky. The radiant was only about 20° from the direction of the earth's orbital motion. Thus the event was either a head-on collision of the earth with an object in retrograde motion (such as a long-period comet) or an object near the aphelion point of a direct orbit (Apollo-type asteroid or daylight meteor stream). Received on Mon 29 Oct 2001 06:37:23 AM PST |
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