Hubble image archive

Collision Sequence for a Magnetar-Powered Kilonova Blast Illustration

This illustration shows the sequence for forming a magnetar-powered kilonova, whose peak brightness reaches up to 10,000 times that of a classical nova. 1) Two orbiting neutron stars spiral closer and closer together. 2) They collide and merge, triggering an explosion that unleas...

Date
Jan 1, 2020
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2020-48-4775-image
By

This illustration shows the sequence for forming a magnetar-powered kilonova, whose peak brightness reaches up to 10,000 times that of a classical nova. 1) Two orbiting neutron stars spiral closer and closer together. 2) They collide and merge, triggering an explosion that unleashes more energy in a half-second than the Sun will produce over its entire 10-billion-year lifetime. 3) The merger forms an even more massive neutron star called a magnetar, which has an extraordinarily powerful magnetic field. 4) The magnetar deposits energy into the ejected material, causing it to glow unexpectedly bright at infrared wavelengths.

Credits

NASA, ESA, and D. Player (STScI)

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Source

Image and source material are credited to the official mission archive linked below.

View on NASA.gov

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