Celestial hemisphere:  Northern  ·  Constellation: Perseus (Per)
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GK Persei, Gary Imm
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GK Persei

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GK Persei, Gary Imm
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GK Persei

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Description

This object is a rarely imaged nova and faint remnant located 1500 light years away in the constellation of Perseus at a declination of +44 degrees. The remnant is 1.5 arc-minutes in diameter in our apparent view, which corresponds to a span of 0.7 light years. The nova is the star GK Persei seen in the center of the remnant. It is an orange sub-giant variable star whose current magnitude is 13.

The nova exploded on Feb. 23, 1901 and was detected a year later. The nova reached a maximum of 0.2 magnitude, one of the brightest novae recorded. Scientists believe that this nova was created when a white dwarf explosion blew away the outer layers of a gas envelope that had accumulated on its surface. This gas envelope had been pulled from its orbiting companion star. The nova still undergoes minor outbursts of about 3 magnitudes every few years.

The nova remnant is not quite symmetrical, which is unusual. It is believed that the interstellar medium is active in this area and is impacting the shape of this remnant.

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GK Persei, Gary Imm