Nova Persei 1901
- Nova Persei 1901
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GK Persei
GK Persei (ou Nova Persei 1901) était une nova qui survint en 1901 dans la constellation de Persée. Elle atteignit une luminosité maximale de 0.2 mag.
Elle fut découverte par Thomas David Anderson.
Coordonnées
Liens externes
Portail de l’astronomie
Catégories : Nova | Constellation de Persée
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Contenu soumis à la licence CC-BY-SA. Source : Article Nova Persei 1901 de Wikipédia en français (auteurs)
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Nova Persei — Nova No va (n[=o] v[.a]), n.; pl. L. {Novae} (n[=o] v[=e]), E. {Novas} (n[=o] v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It… … The Collaborative International Dictionary of English
Nova Persei — GK Persei (auch Nova Persei) war eine helle Nova, die 1901 im Sternbild Perseus aufleuchtete und eine Helligkeit von 0,2 mag erreichte. Der Namensteil „GK“ folgt den Regeln zur Benennung veränderlicher Sterne und besagt, dass GK Persei der 193te… … Deutsch Wikipedia
Nova Persei — ▪ astronomy also designated GK Persei bright nova that attained an absolute magnitude of −9.2. Spectroscopic observations of the nova, which appeared in 1901, provided important information about interstellar gas. The shell thrown off by… … Universalium
Nova Aurigae 1892 — T Aurigae T Aurigae (ou Nova Aurigae 1892) était une nova qui devint brillante en 1892, dans la constellation du Cocher. Elle atteignit une luminosité de 3.8 mag qui diminua ensuite durant 100 jours pour se stabiliser à environ 3 mag. De nos… … Wikipédia en Français
Nova — No va (n[=o] v[.a]), n.; pl. L. {Novae} (n[=o] v[=e]), E. {Novas} (n[=o] v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It may… … The Collaborative International Dictionary of English
Nova Andromedae — Nova No va (n[=o] v[.a]), n.; pl. L. {Novae} (n[=o] v[=e]), E. {Novas} (n[=o] v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It… … The Collaborative International Dictionary of English
Nova Aurigae — Nova No va (n[=o] v[.a]), n.; pl. L. {Novae} (n[=o] v[=e]), E. {Novas} (n[=o] v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It… … The Collaborative International Dictionary of English
Nova Coronae Borealis — Nova No va (n[=o] v[.a]), n.; pl. L. {Novae} (n[=o] v[=e]), E. {Novas} (n[=o] v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It… … The Collaborative International Dictionary of English
Nova Cygni — Nova No va (n[=o] v[.a]), n.; pl. L. {Novae} (n[=o] v[=e]), E. {Novas} (n[=o] v[.a]z). [L., fem. sing. of novus new.] (Astron.) A star which suddenly increases in brightness thousands of times, then fades back to near its original intensity. It… … The Collaborative International Dictionary of English
GK Persei — GK Persei: Nova of 1901. Observation data Epoch J2000.0 Equinox J2000.0 Cons … Wikipedia
