Universe  ID: 4317

Exoplanet Disks In Formation

Visualizations by Tom Bridgman Released on June 25, 2015
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This visualization provides a full 360-degree rotating tour of the disk, face-on to edge-on and back.
These visualizations were developed using a simulation run from the SMACK (Superparticle-Method Algorithm for Collisions in Kuiper belts) code.
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This is a still image from the run illustrating an edge-on view of the disk.
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This visualization was generated using half of the disk, tilting down from top view to edge on to better reveal the profile of the disk material.
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This is a thin sliver of disk particles along a line through the disk. This was generated to highlight the particle profile.
 

Related

The Planet Around Beta Pictoris Makes Waves

For More Information

NASA.gov

Visualization Credits

Tom Bridgman (Global Science and Technology, Inc.): Lead Visualizer
Erika Nesvold (UMBC): Scientist
Marc Kuchner (NASA/GSFC): Scientist
Scott Wiessinger (USRA): Producer
Francis Reddy (Syneren Technologies): Writer
Please give credit for this item to:
NASA's Scientific Visualization Studio

Science Paper:
A SMACK Model of Colliding Planetesimals and Dust in the β Pictoris Debris Disk: Thermal Radiation and Scattered Light

Short URL to share this page:
https://svs.gsfc.nasa.gov/4317

This item is part of this series:
Astrophysics Visualizations

Keywords:
SVS >> Simulation
SVS >> Astrophysics
SVS >> Space
NASA Science >> Universe
SVS >> Exoplanet