[meteorite-list] BREAK! For the love of meteorites, STOP -- COMET 73/P
From: joseph_town_at_att.net <joseph_town_at_meteoritecentral.com>
Date: Sun May 14 17:52:04 2006 Message-ID: <051420062152.17399.4467A67E00039B92000043F721603760210299019BA1089F0A9C0106_at_att.net> Pete Pete, Not to slight all the experts on the met-list, try http://www.meteorobs.org. They are hardcore specialists. Bill -------------- Original message ---------------------- From: "Pete Pete" <rsvp321_at_hotmail.com> > Hi, Sterling and Doug, > > Thanks for your valued input. > > Regarding the 2022 shower, I was wondering how different that spectacle will > be considering it won't be the normal dust-to-pea-sized coma debris, but > more likely some considerable chunks included, due to the current and nicely > timed disintegration. > > Armegaddon!? What side of the planet should we be on then? (-Rhetorical ;]) > > At this rate of break-up, is it possible that there won't be a comet left > for a return trip from around the sun? > > Cheers, > Pete > > > From: "Sterling K. Webb" <sterling_k_webb_at_sbcglobal.net> > To: "Meteorite List" > <meteorite-list_at_meteoritecentral.com>,<joseph_town@att.net>,"Pete Pete" > <rsvp321_at_hotmail.com> > Subject: Re: [meteorite-list] BREAK! For the love of meteorites, STOP -- > COMET 73/P > Date: Sun, 14 May 2006 03:08:50 -0500 > > Hi, Pete, > > Your message came just in time. I was typing a snide remark > about the Hematitic Lump From Mars. (Somebody forward to > this guy Göran Axelsson's picture of the identical "tone rock" > in Sweden at a church, and explain to the guy that he got God's > message all mixed up -- he's supposed to use his rock as the > bell for his church, not sell it on eBay!) > > What bothers me about Comet 73P is this: It can't be a > "new" comet (even though we discovered it in 1930). The orbit > is too stable for the comet to have recently been thrown in > there. It's been around for centuries, probably millennia, in > this same orbit. Yet, it has unraveled so quickly and easily. > > Once it started to come apart, sometime between 1990 > and 1995, it has split, re-split, fractured. If you go back and > read the earliest studies this pass, the authors clearly expected > that whatever splits had occured at the time they wrote to > be the extent of splitting when they passed the Earth. > > Three fragments would be visible, they said. Whoops, make > that six fragments. Uh-oh, make that 9, 12, 30. I'm not making fun > of the researchers, but our experience of split comets is that > this disintegration takes a while. 73P has just gone to hell > overnight. It must be very, very weak, they say. > > OK, BUT... If it's that weak, what has been holding it > together for the last 75 years (and for centuries before > that)? Thermal stress is pegged as the likely culprit for the > breakup, but it's been exposed to the Sun for a long time. > How could it have survived so long if it was this fragile? > > My guess answer is that the fragile material was probably > adhered to something that wasn't fragile, like a small rocky core. > This small dark object would have been completely shielded > from the Sun by the weak porous fluffy ices that surrounded > it and made up the outer body of the comet. > > But once a good chunk of those ices cracks off from a tiny > impact or from thermal stress, it exposes a portion of the dark > rock core to sunlight; the rock warms and more fragments of > icy fluff soon come loose. They're too small to survive and rapidly > break up in a cascade of fragments, as we've seen. A bare dark > rock object is left behind in an orbit similar to the other fragments, > but it's too distant to be detected... yet. > > I'm looking forward to the discovery of a small Earth-crossing > asteroid in 2011, 2016, 2022 with an orbit very like Comet 73P! > It would not be a big one. The pre-breakup 73P nucleus was only > 1000-1200 feet in diameter; a core is unlikely to be more than > a few hundred feet across (30 to 80 meters), I hope, instead of > 400 meters. > > Despite the fact that meteor showers are so showy, no fall > has ever been associated with them. Only one fall was ever > witnessed during a meteor shower and recovered, and it > was an iron, a complete coincidence. The biggest fragments > in a meteor shower are smaller than a pea, moving very fast, > and in for a short bright ride, then Pffft! Small junk never > makes it through the atmosphere. > > Predicting future meteor shower orbits is the most thankless > job in number crunching. Some people like it for that very > reason. Every little piece of cometary material is capable of > puffing little jets of gas; every little jet is a thrust; every thrust > alters the precise orbit somewhat; the thrusts go on for months > with progressive orbital changes, like ion engines. Some jets > are on rotating bodies, so the thrusts are like pinwheel jets, > pushing this way then that way. To quote Charlton Heston > in Planet of the Apes, "It's a madhouse! A madhouse!" > > How spectacular a close comet approach is depends > not only on how close but on how big. The close approach > of a really big fresh long-period comet is probably the most > spectacular thing that is visible in the sky, apart from a > Type II supernova 700 light years away. We haven't had > one really spectacular one for over a century and a half, > but the century before that was blessed with some giant > "apparitions," as they are called, in 1729 and 1744, > and the 19th century had flashier big meteor showers > than the 20th. Maybe we're due for one. > > As for people who worry about close approaches, > here's a table of the 20 closest approaches of comets > that were discovered after 1700 (although some historical > close approaches are included in the list), courtesy of > Harvard http://cfa-www.harvard.edu/iau/lists/ClosestComets.html > One of the brightest recent ones is Hyakutake in > 1996 and it was a really fine sight. Comet 73P is on > the list at Number Ten (in 1930 when it was discovered). > > I added the distance to the Moon for comparison, and > in all this time, nothing has gotten closer than six times the > Moon's distance. > > I say, let's keep it that way. > > Distance Date (TT) Permanent designation > (AU) > 0.0026 Distance to the Moon > 0.0151 1770 July 1.7 D/1770 L1 (Lexell) > 0.0229 1366 Oct. 26.4 55P/1366 U1 (Tempel-Tuttle) > 0.0312 1983 May 11.5 C/1983 H1 (IRAS-Araki-Alcock) > 0.0334 837 Apr. 10.5 1P/837 F1 (Halley) > 0.0366 1805 Dec. 9.9 3D/1805 V1 (Biela) > 0.0390 1743 Feb. 8.9 C/1743 C1 > 0.0394 1927 June 26.8 7P/Pons-Winnecke > 0.0437 1702 Apr. 20.2 C/1702 H1 > 0.0617 1930 May 31.7 73P/1930 J1 (Schwassmann-Wachmann 3) > 0.0628 1983 June 12.8 C/1983 J1 (Sugano-Saigusa-Fujikawa) > 0.0682 1760 Jan. 8.2 C/1760 A1 (Great comet) > 0.0839 1853 Apr. 29.1 C/1853 G1 (Schweizer) > 0.0879 1797 Aug. 16.5 C/1797 P1 (Bouvard-Herschel) > 0.0884 374 Apr. 1.9 1P/374 E1 (Halley) > 0.0898 607 Apr. 19.2 1P/607 H1 (Halley) > 0.0934 1763 Sept.23.7 C/1763 S1 (Messier) > 0.0964 1864 Aug. 8.4 C/1864 N1 (Tempel) > 0.0982 1862 July 4.6 C/1862 N1 (Schmidt) > 0.1018 1996 Mar. 25.3 C/1996 B2 (Hyakutake) > 0.1019 1961 Nov. 15.2 C/1961 T1 (Seki) > Sterling K. Webb > ------------------------------------------------------------------------- > ----- Original Message ----- From: "Pete Pete" <rsvp321_at_hotmail.com> > To: <joseph_town_at_att.net> > Cc: <meteorite-list_at_meteoritecentral.com> > Sent: Saturday, May 13, 2006 11:06 PM > Subject: RE: [meteorite-list] BREAK! For the love of meteorites, STOP > > > > > >Hello, List, > > > >There has been over thirty posts in this thread with barely an > >interruption. Nothing else to talk about? > > > > >I'm hoping Sterling K. Webb will give us his analytical dissection of the > >disintegration of Comet 73P, in his usual interestingly descriptive way! > >>From the top, Sterling! > >And some thoughts about its predicted meteor shower in 2022, if you > >will.(any speculation as to survivors to the surface then?) > >http://www.space.com/scienceastronomy/060510_comet_spitzer.html > >http://www.space.com/scienceastronomy/060510_comet_spitzer.html > > > >Cheers, > >Pete > > > > Received on Sun 14 May 2006 05:52:00 PM PDT |
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