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RR Pictoris, also known as Nova Pictoris 1925, is a cataclysmic variable star system that flared up as a nova that lit up in the constellation Pictor in 1925. It was discovered by South African amateur astronomer R. Watson who lived in Beaufort West. At 05:50 AM on 25 May 1925, Mr. Watson was walking to work and noticed a star that he did not recognize in line with the stars α Crucis and β Carinae. He consulted his copy of Norton's Star Atlas, and realized that the unfamiliar star was a nova. Fortuitously, Mr. Watson was employed as a telegraph operator, and he promptly sent a telegram describing his discovery to the Royal Observatory at Cape Town. This quick reporting of the event allowed southern observatories to obtain spectra of the nova before it had reached maximum brightness.

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rdfs:label
  • RR del Cavallet de Pintor (ca)
  • RR Pictoris (de)
  • RR Pictoris (es)
  • RR Pictoris (fr)
  • RR Pictoris (en)
  • RR Pictoris (pt)
  • RR Pictoris (sv)
  • 绘架座RR (zh)
rdfs:comment
  • RR Pictoris (ou Nova Pictoris 1925) est une nova qui survint en 1925 dans la constellation du Peintre. Elle atteignit une magnitude minimale (correspondant à une luminosité maximale) de 1,2 mag. De nos jours, RR Pictoris a une magnitude de 12,5. Elle est distante d'environ ∼1 670 a.l. (∼512 pc) de la Terre. (fr)
  • RR Pictoris eller Nova Pictoris 1925 var en långsam nova i stjärnbilden Målaren. Novan upptäcktes den 25 maj 1925 av den brittiske telegrafisten och amatörastronomen R. Watson. Den nådde magnitud +1,0 i maximum och avklingade sedan långsamt. Den är nu en stjärna av 12:e magnituden. (sv)
  • 绘架座RR(RR Pictoris)是一颗位于绘架座的新星,1925年爆发。爆发时最亮视星等为1.2,它的亮度的150天下降3等,现在亮度为9等。 (zh)
  • RR del Cavallet de Pintor, també coneguda com Nova del Cavallet de Pintor 1925, és un sistema estel·lar variable cataclísmic que es va encendre com una nova i va il·luminar la constel·lació del Cavallet de Pintor. (ca)
  • RR Pictoris, también conocida como Nova Pictoris 1925, es un sistema estelar variable cataclísmico que se encendió como una nova e iluminó la constelación de Pictor. El astrónomo sudafricano R. Watson la observó por primera vez el 25 de mayo de 1925 cuando tenía una magnitud aparente de 2,3. Continuó brillando hasta la magnitud 1,2 que alcanzó el 9 de junio de 1925. Se atenuó a la magnitud 4 el 4 de julio, pero volvió a iluminarse a 1,9 el 9 de agosto. Seis meses después de su brillo máximo, RR Pictoris desapareció para ser invisible a simple vista, y era de magnitud 12,5 en 1975.​ (es)
  • RR Pictoris, auch Nova Pictoris 1925, war eine langsame Nova vom Typ NB, die im Sternbild Maler aufleuchtete. Sie wurde am 25. Mai 1925 vom südafrikanischen Astronomen R. Watson mit einer Magnitude von 2,3 m entdeckt. Ihre Helligkeit nahm weiter zu, bis sie am 6. Juni 1925 ihr Maximum mit 1,1 ± 0,1 m erreichte. Bis zum 4. Juli ging die Helligkeit weiter auf 4,0 m zurück, stieg jedoch am 9. August wieder auf 1,9 m an. Ein halbes Jahr nach dem Maximum verblasste RR Pictoris so stark, dass sie für das bloße Auge nicht mehr sichtbar war, und ging bis 1975 auf eine Magnitude von 12,5 m zurück. (de)
  • RR Pictoris, also known as Nova Pictoris 1925, is a cataclysmic variable star system that flared up as a nova that lit up in the constellation Pictor in 1925. It was discovered by South African amateur astronomer R. Watson who lived in Beaufort West. At 05:50 AM on 25 May 1925, Mr. Watson was walking to work and noticed a star that he did not recognize in line with the stars α Crucis and β Carinae. He consulted his copy of Norton's Star Atlas, and realized that the unfamiliar star was a nova. Fortuitously, Mr. Watson was employed as a telegraph operator, and he promptly sent a telegram describing his discovery to the Royal Observatory at Cape Town. This quick reporting of the event allowed southern observatories to obtain spectra of the nova before it had reached maximum brightness. (en)
  • RR Pictoris, também conhecida como Nova Pictoris 1925, é uma estrela binária variável cataclísmica que explodiu como uma nova em 1925. Localiza-se na constelação de Pictor a uma distância de aproximadamente 1 700 anos-luz (520 parsecs) da Terra. Foi primeiramente notada pelo astrônomo sul-africano R. Watson em 25 de maio de 1925, quando tinha uma magnitude aparente de 2,3. Seu brilho continuou a aumentar até chegar a uma magnitude de 1,2 em 9 de junho de 1925. A magnitude do sistema diminuiu para 4 em 4 de julho, mas aumentou novamente para 1,9 em 9 de agosto. Seis meses após seu pico de magnitude, RR Pictoris não era mais visível a olho nu, até chegar à sua magnitude aparente atual de 12,5. (pt)
foaf:name
  • RR Pictoris (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/RRPicLocation.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/RRPictorisEarlyLightCurve.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/RRPictorisLightCurve.png
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