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Simulations of the Breakup of Comet Shoemaker-Levy 9 Employing a Swarm Model: Initial Conditions
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The breakup of comet Shoemaker-Levy 9 due to its gravitational interaction with Jupiter in July, 1994 is simulated using a swarm model. In this simulation, the comet is modeled as an initially spherical distribution of 16,384 particles. The particles interact with the tidal field of Jupiter and with each other through inter-particle gravitation and collisions. All simulations were performed on the Maspar MP-2 at NASA/GSFC.
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In this animation of the initial simulation conditions, the comet orbit around Jupiter is shown, then the view zooms in to the comet at a distance of 2.1 Jovian radii from Jupiter, where the initial spherical distribution is shown within a box 4 km on a side.
Duration: 52.0 seconds
Available formats:
352x240 (29.97 fps)
MPEG-1
7 MB
160x80
PNG
7 KB
80x40
PNG
2 KB
320x238
JPEG
4 KB
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| Animation Number: | 84 |
| Animator: | Kevin Olson (Lead) |
| Studio: | SVS |
| Completed: | 1995-03-24 |
| Scientists: | Kevin Olson (George Mason University) |
| | Michael Mumma (NASA/GSFC) |
| Series: | Shoemaker-Levy 9 |
| Video: | SVS1995-0004 * |
Keywords:
SVS
>> Comet
SVS
>> Jupiter
DLESE
>> Space science
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Please give credit for this item to
NASA/Goddard Space Flight Center
Scientific Visualization Studio |
*Please note: the SVS does not fulfill requests for copies of the tapes in our library. On some of our animation pages, there is a direct link to a video distribution service from which tapes, handled by the Public Affairs Office (PAO)/Goddard TV, including some of our animations may be ordered. General information on this service can be found here. |
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