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- Newsgroups: sci.astro
- Path: sparky!uunet!spool.mu.edu!yale.edu!qt.cs.utexas.edu!cs.utexas.edu!sun-barr!ames!news.hawaii.edu!galileo!tholen
- From: tholen@galileo.ifa.hawaii.edu (Dave Tholen)
- Subject: Re: Questions about P/Swift-Tuttle
- Message-ID: <1992Nov7.234122.26598@news.Hawaii.Edu>
- Sender: root@news.Hawaii.Edu (News Service)
- Nntp-Posting-Host: galileo.ifa.hawaii.edu
- Organization: Institute for Astronomy, Hawaii
- Date: Sat, 7 Nov 1992 23:41:22 GMT
- Lines: 24
-
- Mike Schriber writes:
-
- > First of all, in response to a previous post, I belive the /P in
- > P/Swift-Tuttle designates it as a member of Perseid group (I may be
- > very wrong on this though, since the Perseids are a metor shower).
-
- Sorry, but you are very wrong. The P/ mean periodic, though the really
- long period comets (ones with eccentricities just shy of unity) are not
- so labeled.
-
- > My other question is a bit more limited. I have a program called Dance of
- > The Planets by ARC. I've tracked Swift-Tuttle with this program and found
- > the comet to be outbound, near the orbit of Mars on 8/14/2126. Dance of
- > the Planets is suposed to be a first rate orbital simulator (Gavitic forces
- > only) and I'm curious as to why it's so far off.
-
- The non-gravitational forces on comets can be rather substantial. Whether
- this is the dominant contribution to Dance of the Planet's discrepancy
- isn't clear. It can't be that good an orbital simulator, given the size
- of the program. It probably uses the mean orbits for the planets when
- computing perturbations, an approach that is consistent with the program's
- size, but I doubt it performs a full-up N-body numerical integration such
- as JPL's DE200. For one thing, your PC would take forever (and probably
- doesn't have enough memory) to do such a calculation.
-