STScI-PRC2000-02
[Left]
A NASA Hubble Space Telescope false-color, visible-light picture of
one side of the edge-on dust disk around the star Beta Pictoris. Knots
in the disk (marked A,B,C,D) are interpreted as rings of dust, seen
edge-on.
[Right]
A still frame from a computer simulation, which shows a circumstellar
dust disk highly perturbed by the gravitational pull of a bypassing
star. The gray solid area represents the initial shape and size of
the undisturbed disk. In the simulation, the gravity of the passing
star rearranges the orbit of each particle, setting up an elliptical
ring system that may have survived for the last 100,000 years since
the impact occurred.
Object Name: Beta Pictoris
Image Type: Astronomical/Illustration
Image Credit (Left) : NASA and Paul Kalas (Space Telescope Science Institute)
Simulation courtesy (Right):John Larwood (Queen Mary and Westfield College, London, United Kingdom)
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