Issue |
A&A
Volume 448, Number 1, March II 2006
|
|
---|---|---|
Page(s) | 401 - 409 | |
Section | Celestial mechanics and astrometry | |
DOI | https://doi.org/10.1051/0004-6361:20053756 | |
Published online | 17 February 2006 |
Non-gravitational motion of the Jupiter-family comet 81P/Wild 2
I. The dynamical evolution
Space Research Centre of the Polish Academy of Sciences, Bartycka 18A, 00-716, Warsaw, Poland e-mail: mkr@cbk.waw.pl
Received:
4
July
2005
Accepted:
29
September
2005
We investigated the influence of the non-gravitational
effects on the orbital motion of 81P/Wild 2. First, the
non-gravitational accelerations on cometary nucleus throughout all
five revolutions around the sun were analysed using both the
symmetrical and the asymmetrical -function. Next, the
symmetric model was used to examine the past and future dynamical
evolution of Wild 2 within the time interval of ±8 thousand
years. We then introduced a statistical approach. In the most
probable scenario for Wild 2 history, a few thousand years ago,
this comet was an object with its perihelion close to the Jupiter
orbit with an aphelion distance greater than the Neptune orbit: JN
class, JE class, JT class, or even larger. Due to the extremely
close approach to Jupiter in 1974, its future evolution differs
substantially from earlier, so most probably, comet Wild 2 will
survive as a typical Jupiter-family comet during the few thousand
years that follow. After 8000 yr, however, the chance that the
comet Wild 2 will still be a typical JF comet (with
AU)
drops to 29%. Similarities between the orbital histories of
Wild 2 and comets 16P/Brooks 2 and 67P/Churyumov-Gerasimenko are
also discussed.
Key words: comets: individual: comet 81P/Wild 2 / comets: general
© ESO, 2006
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