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KIC 9832227
PREDICTION OF A RED NOVA OUTBURST IN KIC 9832227
Astronomers predict explosion that will change the night sky in 2022
Molnar's prediction is that a binary star (two stars orbiting each other) he is monitoring will merge and explode in 2022, give or take a year; at which time the star will increase its brightness ten thousand fold, becoming one of the brighter stars in the heavens for a time. The star will be visible as part of the constellation Cygnus, and will add a star to the recognizable Northern Cross star pattern.
Molnar and colleagues will be observing KIC 9832227 in the next year over the full range of wavelengths: using the Very Large Array, the Infrared Telescope Facility, and the XMM-Newton spacecraft to study the star's radio, infrared and X-ray emission, respectively.
Molnar says that this is the beginning of a story that will unfold over the next several years, and people of all levels can participate.
"The orbital timing can be checked by amateur astronomers," said Molnar. "It's amazing the equipment amateur astronomers have these days. They can measure the brightness variations with time of this 12th magnitude star as it eclipses and see for themselves if it is continuing on the schedule we are predicting or not."
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PREDICTION OF A RED NOVA OUTBURST IN KIC 9832227
Astronomers predict explosion that will change the night sky in 2022
Molnar's prediction is that a binary star (two stars orbiting each other) he is monitoring will merge and explode in 2022, give or take a year; at which time the star will increase its brightness ten thousand fold, becoming one of the brighter stars in the heavens for a time. The star will be visible as part of the constellation Cygnus, and will add a star to the recognizable Northern Cross star pattern.
Molnar and colleagues will be observing KIC 9832227 in the next year over the full range of wavelengths: using the Very Large Array, the Infrared Telescope Facility, and the XMM-Newton spacecraft to study the star's radio, infrared and X-ray emission, respectively.
Molnar says that this is the beginning of a story that will unfold over the next several years, and people of all levels can participate.
"The orbital timing can be checked by amateur astronomers," said Molnar. "It's amazing the equipment amateur astronomers have these days. They can measure the brightness variations with time of this 12th magnitude star as it eclipses and see for themselves if it is continuing on the schedule we are predicting or not."
Youtube
S&T