[meteorite-list] Peter Brown's Initial Accessment of Chelaybinsk Event
From: MEM <mstreman53_at_meteoritecentral.com>
Date: Sat, 16 Feb 2013 04:14:15 -0800 (PST) Message-ID: <1361016855.97087.YahooMailNeo_at_web142401.mail.bf1.yahoo.com> Update from Peter Brown (via Richard's FB post) Fri Feb?15,?2013 2:11?pm (PST) . Posted by: "Tomas" scibuffcom? via MPML This report is written by Peter Brown, probably the foremost expert in the world on this type of impact event. "This is what I know as of 17 h UT today... Feb 15, 2013 Fireball Event Summary What follows are *initial* information gleaned for multiple instrumental sources recording various aspects of the Feb 15, 2013 airburst over Chelaybinsk, Russia (55.2N, 61.4E) 1. Time: The time of the main flare/airburst was 03:20:26 UT on Feb 15, 2013; the fireball began ablation about 30 secs before this time. 2. Based on the long duration of the event and videos, it is clear this was a very shallow entry (certainly less than 20 degrees, maybe more shallow). 3. It is *not* related to 2012 DA14 4. Energy: This is perhaps the hardest value to pin down so early in this investigation. From multiple sensors using multiple technologies a best initial estimate of the total energy of the event is about 300 kilotons of TNT equivalent = ~10^15 J). This could easily be in error by a factor of two. I am confident, however that it is in excess of 100 kTons, making it the largest recorded event since the 1908 Tunguska explosion. 5. Speed: The fireball entered the atmosphere at 18 km/s 6. Damage: The airblast clearly caused window breakage and light structural damage in downtown Chelaybinsk. The exact overpressure at which window failure occurs tends to be probabilistic and varies by construction design (ANSI S2.20, 1983). Normally some damage begins to occur around 500 Pa of overpressure, widespread window damage is expected to occur up to around ten-20 times this value. As the fireball had a shallow trajectory, the cylindrical blast wave would have propagated directly to the ground and would be expected to be intense. This could be further compounded by any fragmentation, quasi-spherical blasts. My impression is that the key here is that the terminal part of the fireball (probably between 15-20 km altitude) occurred almost directly over Chelaybinsk; this was perhaps the single greatest contributor to the blast damage (short range to the main part of the terminal detonation). 7. Comparators: The Sikhote-Alin fall (Feb 12, 1947) in the former Soviet Union was the equivalent of about 10 kilotons TNT, BUT as an iron impactor much of this energy was deposited at the ground rather than at altitude. The Oct 8, 2009 Indonesia event is the most recent similar event at about 50 kTons, but over the ocean (paper attached for quick reference). 8. Size: The pre-impacting asteroid was about 15 meters in diameter and had a mass of ~7000 tonnes. I fully expect revision of some of the numbers above, particularly the estimate of the yield which could *easily* change by a factor of two upon more complete analysis and will likely change as the day progresses /end ------------ -------- Dr. Peter Brown Director - Centre for Planetary Science and Exploration Canada Research Chair in Meteor Astronomy Professor Department of Physics and Astronomy University of Western Ontario London, Ontario N6A 3K7 CANADA" Received on Sat 16 Feb 2013 07:14:15 AM PST |
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