Naked-Eye Gamma-ray Burst Model for GRB 080319B

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.


Cruz deWilde (Avant Gravity): Lead Animator
Stefanie Misztal (UMBC): Producer
Steven Ritz (NASA/GSFC): Scientist
Please give credit for this item to:
NASA/Swift/Cruz deWilde

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Fermi Gamma-ray Space Telescope

Data Used:
Fermi/LAT None
Swift None

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Astrophysics Animations

SVS >> Gamma Ray
SVS >> Gamma Ray Burst
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