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Hubble Gamma Ray Burst
Credit: NASA, ESA, N. Tanvir (University of Leicester), and A. Fruchter, Z. Levay (Space Telescope Science Institute), A. Levan (University of Warwick)
These images taken by NASA’s Hubble Space Telescope reveal a new type of stellar explosion produced by the merger of two compact objects: either two neutron stars or a neutron star and a black hole. The galaxy in the center of the left image produced the gamma-ray burst, whose lingering effects were visible on June 13 but had faded by July 3. [
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Kilonova Gamma-Ray Burst GRB 130603B
Credit: NASA, ESA, N. Tanvir (University of Leicester), A. Levan (University of Warwick), A. Fruchter (STScI), J. Hjorth (University of Copenhagen), R. Hounsell (STScI), K. Wiersema (University of Leicester), and R. Tunnicliffe (University of Warwick)
This wide view of the gamma-ray burst GRB 130603B shows its host galaxy and the surrounding area. The galaxy is 4 billion light-years from Earth. Image released Aug. 3, 2013. [
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Kilonova Gamma-Ray Burst GRB 130603B: Before
Credit: NASA, ESA, N. Tanvir (University of Leicester), A. Levan (University of Warwick), A. Fruchter (STScI), J. Hjorth (University of Copenhagen), R. Hounsell (STScI), K. Wiersema (University of Leicester), and R. Tunnicliffe (University of Warwick)
This view of the host galaxy for the kilonova gamma-ray burst GRB 130603B was captured by the Hubble Space Telescope on June 13, 2013. Image released Aug. 3, 2013. [
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Kilonova Gamma-Ray Burst GRB 130603B: After
Credit: NASA, ESA, N. Tanvir (University of Leicester), A. Levan (University of Warwick), A. Fruchter (STScI), J. Hjorth (University of Copenhagen), R. Hounsell (STScI), K. Wiersema (University of Leicester), and R. Tunnicliffe (University of Warwick)
This image of the host galaxy for the kilonova gamma-ray burst GRB 130603B was captured by the Hubble Space Telescope on July 3, 2013. Image released Aug. 3, 2013. [
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Kilonova Explosion: Sequence of Events
Credit: NASA, ESA, and A. Field (STScI)
This sequence illustrates a model for the formation of a short-duration gamma-ray burst to become a powerful kilonova explosion. Here, two neutron stars circle one another and ultimately collide to kick out highly radioactive material. This material heats up and expands, emitting a burst of light called a kilonova. An accompanying gamma-ray burst lasts just one-tenth of a second, but is 100 billion times brighter than the kilonova flash. Image released Aug. 3, 2013. [
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Kilonova Explosion: Step 1
Credit: NASA, ESA, and A. Feild (STScI)
In this illustration, two ultradense neutron stars circle one another, slowly coming together in the first step toward a cosmic collision that can create a kilonova gamma-ray burst. Image released Aug. 3, 2013. [
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Kilonova Collision Illustration
Credit: NASA, ESA, and A. Feild (STScI)
Two ultradense neutron stars collide to unleash a kilonova gamma-ray burst explosion in this artist's illustration. Image released Aug. 3, 2013. [
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Kilonova Gamma-Ray Burst Explosion
Credit: NASA, ESA, and A. Feild (STScI)
Two ultradense neutron stars explode in a powerful, but just millisecond-brief, gamma-ray burst to spark a kilonova event in this artist's illustration. Image released Aug. 3, 2013. [
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Kilonova Aftermath: Illustration
Credit: gamma-ray burst, gamma ray burst, black hole, neutron star, nasa, hubble space telescope, hubble, astronomy, kilonovas, kilonova explosions
A remnant disk of debris surrounds the merged remains of two ultradense neutron stars in a kilonova gamma-ray burst, which may have collapsed to form a black hole. Image released Aug. 3, 2013. [
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