Received: from ATHENA-AS-WELL.MIT.EDU by po7.MIT.EDU (5.61/4.7) id AA14135; Thu, 5 Aug 93 21:53:13 EDT Received: from M66-080-15.MIT.EDU by Athena.MIT.EDU with SMTP id AA02554; Thu, 5 Aug 93 21:53:12 EDT From: jpbonsen@Athena.MIT.EDU Received: by m66-080-15 (5.57/4.7) id AA22467; Thu, 5 Aug 93 21:53:10 -0400 Message-Id: <9308060153.AA22467@m66-080-15> To: rdshydur@Athena.MIT.EDU Subject: comet to hit jupiter! Date: Thu, 05 Aug 93 21:53:08 EDT ------- Forwarded Message Received: from ATHENA-AS-WELL.MIT.EDU by po6.MIT.EDU (5.61/4.7) id AA02114; Thu, 5 Aug 93 21:19:37 EDT Received: from ude.tim.ia.ung.gnu.ai.mit.edu by Athena.MIT.EDU with SMTP id AA01587; Thu, 5 Aug 93 21:19:35 EDT Received: by ude.tim.ia.ung.gnu.ai.mit.edu id AA09729; Thu, 5 Aug 93 21:17:16 EDT Received: from panix.com by ude.tim.ia.ung.gnu.ai.mit.edu via TCP with SMTP id AA09724; Thu, 5 Aug 93 21:17:02 EDT Received: by panix.com id AA02615 (5.65c/IDA-1.4.4 for exi-remail@ung.gnu.ai.mit.edu); Thu, 5 Aug 1993 21:07:12 -0400 To: Exi@panix.com Message-Id: <9308060100.AA02773@mx.nsi.nasa.gov> Date: Thu, 5 Aug 93 18:05:51 PDT From: GRAPS@galileo.arc.nasa.gov Subject: Comet Shoemaker-Levy 9 X-Original-To: vince.k@applelink.apple.com, tcmay@netcom.com, extropians@gnu.ai.mit.edu X-Extropian-Date: Remailed on August 6, 373 P.N.O. [01:06:52 UTC] X-Message-Number: #93-8-141 Reply-To: extropians@gnu.ai.mit.edu Errors-To: Extropians-Request@gnu.ai.mit.edu Hello extropi-oids: It's been quite a while since I posted to this list.. Maybe next time my funding runs out, I shouldn't accept every job that comes along and, perhaps, just work at one???? Anyway... At the Extropian Bay Area lunch today, a discussion popped up about Comet Shoemaker-Levy 9 (aka 1993e). Some of the e-folks had just recently heard about about this comet, while others hadn't heard about it yet. WHERE HAVE YOUR MINDS BEEN??!! Wrapped up in a computer monitor or something? :) :) So, I, your friendly extropian astronomer, am here to educate you about this delightful, explosive (if you like explosions or such- Keith H are you out there?), once-in-a-lifetime celestial event. - --------------------------------------------------------------------- "Jupiter is Offering a Crash Course in Comets" (many excerpts from ref 1) Astronomers will be aiming virtually every telescope in the world towards Jupiter in late-July next year to see what happens when big chunks of a shattered comet punch into the backside of Jupiter at almost 40 miles/sec, exploding with energy equivalent to almost a billion megatons of TNT. For the first time since the invention of the telescope, a comet is hitting a planet. Next year's rare, lucky glimpse of the "before," "during," and "after" should provide an unprecendented opportunity to test theories on, among other things, the nature of comets, the nature of Jupiter, how planetary rings form, how craters form, and the dynamics of high-megaton atmospheric explosions. It's as close to a controlled laboratory experiment on a planetary scale as we're likely to come. The comet (perhaps 12 miles in diameter) almost hit the planet Jupiter on its last pass a year ago, David Levy (one of the discoverers) says. At that time, the planet's powerful gravitational forces ripped it into a swarm of mini-comets enveloped in an enormous cloud of dust and rubble. By the time Earth telescopes spotted it in March, the comet pieces had spread out like a string of pearls (also referred to as a "nuclear train"). Scientists counted 17 major pieces then, but further studies have revealed 21. Uncertainty about whether a collision will occur has all but disappeared in recent weeks, says Donald Yeomans of NASA's JPL. "There is almost no question that major chunks will hit Jupiter." Calculations by Yeomans and colleague Paul Chodas (see my information from them below) indicate a probability of more than 99 percent- a virtual dead certainty in astronomical terms. But Yeomans hedges. "Mother Nature sometimes thumbs her nose at us." In fact scientists emphasize that there are so many unknowns in their calculations that they can only make educated guesses about what's going to happen next July. Unfortunately, we won't be able to directly see the event from Earth. Astronomers calculate that the comet train will strike the far side of Jupiter on July 21-23, 1994, causing repeated flashes over two or three days. Jupiter completes one rotation every 10 hours, so the impact zone will soon spin into view and they/we can inspect the results. The impacts probably will, for a time, "crater" Jupiter's turbulent atmosphere as if it were a a hard surface, causing some of its previously unseen innards to "well up." The shock could linger in the form of a another semi-permanent storm similar to Jupiter's trademark, the Great Red Spot. The impacts could create a series of fireballs emerging from deep within Jupiter's clouds and blowing out the top, the largest perhaps 400 miles across- a mere dot on the vast face of Jupiter- with a flash "as bright as the surface of the sun," and a rain of debris leaving glowing trails all around. Scientists have estimated that the plume caused by the explosion will be 10-100 times brighter than the rest of the surface of Jupiter. If the bulls-eye were on the side facing Earth, Levy says, it would be visible in the daylight without a telescope. Astronomers will indirectly observe the event by measuring reflected light that bounces off Jupiter's nearest moons, Io and Europa. The effects may be visible in backyard telescopes and even binoculars. The visibility of the fireworks depends in part on the size and composition of the incoming objects. Astronomers are hoping to directly observe the event by using several space probes. The partially crippled Galileo will arrive at Jupiter 16 months too late to see the event up-close, but it should be able to observe it from-a-distance. Calculations from Paul Chodas show that Galileo will be able to see the impact on Jupiter's terminator. Gene Shoemaker (the other discoverer) is urging NASA to power up instruments aboard Voyager 2, now cruising beyond the planets. It could record the flash even across such a distance. - --------------------------------------------------------------------- For all of you hard-core techies, who maybe want to see the numbers, I located the following "bulletins". The astronomers that I work with in my building are really excited about this event, and so everyone has graphs of impact simulations and other calculations relating to the event posted everywhere. - --------------------------------------------------------------------- From IAU Circular No 5800 and 5801 (ref 2), "Almost 200 precise positions of this comet have now been reported (mostly from CCD images by S. Nakano and T. Kobayashi in Japan and by E. Meyer, E. Obermair and H. Raab in Austria). These observations are mainly of the the center of the nuclear train, and this point continues to be the most relevant for orbit computations. The presumed encounter with Jupiter that created the train occurred during the first half of July 1992. The comet(s) has a period of roughly 2 years. ... more than half of the nuclear train could collide with Jupiter, over an interval approaching 3 days. Preliminary computations by A. Carusi, Rome University, show that surviving nuclei are likely to remain as satellites of Jupiter or be thrown closer to the sun on short-period heliocentric orbits (depending on which side of Jupiter they pass)." [A mini-solar system in the making!!!!] - --------------------------------------------------------------------- From Don Yeomans and Paul Chodas, JPL, (ref 3) "The following jovicentric impact circumstances for comet 1993e apply: Time of entry = 1994 July 20.4995 Atmospheric entry at Jupiter latitude = -46 degrees Atmospheric entry defined as 69,000 km at this latitude Relative velocity at entry = 60.5 km/s Sun-comet-Jupiter angle at entry = 66 degrees (night side) Orbital eccentricity at entry = 0.99877 Jovicentric periapses = 33,761 km Orbital inclination with respect to Jupiter equator = 84 degrees" - --------------------------------------------------------------------- ref 1) July 19-25, 1993 The Washington Post National Weekly Edition Page 38. ref 2) May 22, 1993 Central Bureau for Astronomical Telegrams, Int'l Astronomical Union Smithsonian Astrophysical Observatory, Cambridge MA 02138 ref 3) June 1, 1993 in NASAMail to D. Morrison, Space Sciences Division, NASA-Ames. - --------------------------------------------------------------------- Amara Graps NASA-Ames Research Center MS 245-5 Moffett Field, CA 94035 graps@gal.arc.nasa.gov ------- End of Forwarded Message