GK Persei
GK Persei (also Nova Persei 1901) was a bright nova first observed on Earth in 1901. It was discovered by Thomas David Anderson, an Edinburgh clergyman, at 02:40 UT on 22 February 1901 when it was at magnitude 2.7. It reached a maximum magnitude of 0.2, the brightest nova of modern times until Nova Aquilae 1918. After fading into obscurity at about magnitude 12 to 13 during the early 20th century, GK Persei began displaying infrequent outbursts of 2 to 3 magnitudes (about 7 to 15 times quiescent brightness). Since about 1980, these outbursts have become quite regular, typically lasting about two months and occurring about every three years. Thus, GK Persei seems to have changed from a classical nova like Nova Aquilae 1918 to something resembling a typical dwarf nova-type cataclysmic variab
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367Auriga (constellation)BV CentauriBeyond the Wall of Sleep (short story)Chandra_X-ray_ObservatoryCharles Dillon PerrineFebruary 1901GK PerIntermediate polarJakob Karl Ernst HalmJoel StebbinsJohn Ellard GoreLight echoList of novae in the Milky Way galaxyNova PerseiNova Persei 1901Nova remnantPerseus (constellation)Stars and planetary systems in fictionSuperluminal motionThomas David AndersonWilliam Herbert Steavenson
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GK Persei
GK Persei (also Nova Persei 1901) was a bright nova first observed on Earth in 1901. It was discovered by Thomas David Anderson, an Edinburgh clergyman, at 02:40 UT on 22 February 1901 when it was at magnitude 2.7. It reached a maximum magnitude of 0.2, the brightest nova of modern times until Nova Aquilae 1918. After fading into obscurity at about magnitude 12 to 13 during the early 20th century, GK Persei began displaying infrequent outbursts of 2 to 3 magnitudes (about 7 to 15 times quiescent brightness). Since about 1980, these outbursts have become quite regular, typically lasting about two months and occurring about every three years. Thus, GK Persei seems to have changed from a classical nova like Nova Aquilae 1918 to something resembling a typical dwarf nova-type cataclysmic variab
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GK Persei (GK Per) è una stell ...... anni luce dal sistema solare.
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GK Persei (GK Per) és un estel ...... mp magnètic de la nana blanca.
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GK Persei (GK Per) es una est ...... magnético de la enana blanca.
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GK Persei (Nova Persei 1901) – ...... pobliżu jego domu w Edynburgu.
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GK Persei (also Nova Persei 19 ...... e) than the Gaia measurements.
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GK Persei (auch Nova Persei 19 ...... eworks nebula bezeichnet wird.
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GK Persei (juga dikenal Nova P ...... 1 ditemukan 21 February oleh .
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GK Persei (ou Nova Persei 1901 ...... couvreur de Nova Aurigae 1892.
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GK Persei (též Nova Persei 190 ...... m Thomasem Davidem Andersonem.
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GK Persei eller Nova Persei 19 ...... net expanderar med 1 200 km/s.
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absmag v
−9.1 - +3.7
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appmag v
class
K1IV
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constell
epoch
p error
parallax
prop mo dec
−17.348
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prop mo ra
−6.878
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radial v
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GK Persei (GK Per) è una stell ...... anni luce dal sistema solare.
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GK Persei (GK Per) és un estel ...... ificativament el seu diàmetre.
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GK Persei (GK Per) es una est ...... gnificativamente su diámetro.
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GK Persei (Nova Persei 1901) – ...... nich latach znacznie mniejsze.
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GK Persei (also Nova Persei 19 ...... f nova-type cataclysmic variab
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GK Persei (auch Nova Persei 19 ...... ps DQ-Herculis zuzuordnen ist.
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GK Persei (juga dikenal Nova P ...... ang variable katalismik tipe .
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GK Persei (ou Nova Persei 1901 ...... couvreur de Nova Aurigae 1892.
@fr
GK Persei (též Nova Persei 190 ...... m Thomasem Davidem Andersonem.
@cs
GK Persei eller Nova Persei 19 ...... net expanderar med 1 200 km/s.
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GK Persei
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GK Persei
@cs
GK Persei
@de
GK Persei
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GK Persei
@es
GK Persei
@fr
GK Persei
@in
GK Persei
@it
GK Persei
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GK Persei
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GK Persei
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