Naked-Eye Gamma-ray Burst Model for GRB 080319B
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- Visualizations by:
- Cruz deWilde
- View full credits
Gamma-ray bursts that are longer than two seconds are caused by the detonation of a rapidly rotating massive star at the end of its life on the main sequence. Jets of particles and gamma radiation are emitted in opposite directions from the stellar core as the star collapses. In this model, a narrow beam of gamma rays is emitted, followed by a wider beam of gamma rays. The narrow beam for GRB 080319B was aimed almost precisely at the Earth, which made it the brightest gamma-ray burst observed to date by NASA's Swift satellite.
Credits
Please give credit for this item to:
NASA/Swift/Cruz deWilde
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Animator
- Cruz deWilde (Avant Gravity) [Lead]
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Scientist
- Steven Ritz (NASA/GSFC)
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Producer
- Stefanie Misztal (UMBC)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
Fermi (Collected with the LAT sensor)
Fermi Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT)
Dataset can be found at: http://fermi.gsfc.nasa.gov
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details, nor the data sets themselves on our site.