Sign on
ADS Classic is now deprecated. It will be completely retired in October 2019. This page will automatically redirect to the new ADS interface at that point.
SAO/NASA ADS Astronomy Abstract Service
· Find Similar Abstracts (with default settings below)
· Full Refereed Journal Article (PDF/Postscript)
· Full Refereed Scanned Article (GIF)
· Citations to the Article (49) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)- ·
· Translate This Page
Title: | The Tunguska object - A fragment of Comet Encke | |
Authors: | Kresak, L'. | |
Affiliation: | AA(Slovenska Akademia Vied, Astronomicky Ustav, Bratislava, Czechoslovakia) | |
Publication: | Astronomical Institutes of Czechoslovakia, Bulletin, vol. 29, no. 3, 1978, p. 129-134. | |
Publication Date: | 00/1978 | |
Category: | Astrophysics | |
Origin: | STI | |
NASA/STI Keywords: | Comets, Meteoroid Showers, Tungusk Meteorite, Chondrites, Earth Orbits, Meteorite Craters, Orbital Elements, Shock Waves, Taurid Meteoroids | |
Bibliographic Code: | 1978BAICz..29..129K |
Abstract
It is pointed out that the solar longitude and equatorial coordinates of
the apparent radiant of the Tunguska object (1908), as given by Zotkin
(1966), are in good agreement with those of Comet Encke and the Beta
Taurid shower, which is one of the two annual appearances of the broad
meteor stream associated with Comet Encke. This suggests that the
Tunguska object may have been a fragment of Comet Encke, and a
trajectory prior to impact is reconstructed, and the encounter velocity
is estimated at 31 plus or minus 2 km/sec. The tremendous explosion,
shock wave, and forest fire without appreciable cratering also provide
support of the cometary nature of the object. The Whipple (1968)
conjecture that the body was an asteroidal pre-type I carbonaceous
chondrite is equally in accord with encounter geometry and nature of
damage, but recent data classify all but one of the Apollo asteroids as
silicaceous or ordinary chondritic objects.
Printing Options
Send high resolution image to Level 2 Postscript Printer
Send low resolution image to Level 2 Postscript Printer
Send low resolution image to Level 1 Postscript Printer
Get high resolution PDF image
Get low resolution PDF
Send 300 dpi image to PCL Printer
Send 150 dpi image to PCL Printer
More Article Retrieval Options
HELP for Article Retrieval
Bibtex entry for this abstract Preferred format for this abstract (see Preferences) |
Find Similar Abstracts:
Use: | | Authors | |
| Title | ||
| Keywords (in text query field) | ||
| Abstract Text | ||
Return: | | Query Results | Return items starting with number |
| Query Form | ||
Database: | | Astronomy | |
| Physics | ||
| arXiv e-prints |
(function(i,s,o,g,r,a,m)function(),i[r].l=1*new Date();a=s.createElement(o),
m=s.getElementsByTagName(o)[0];a.async=1;a.src=g;m.parentNode.insertBefore(a,m)
)(window,document,'script','//www.google-analytics.com/analytics.js','ga');
ga('create', 'UA-37369750-3', 'harvard.edu');
ga('send', 'pageview');