About: 17 Sagittarii

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17 Sagittarii is a binary star system in the zodiac constellation of Sagittarius, located 675 light years from the Sun. With a combined apparent visual magnitude of 6.89 it is below the normal limit of visibility to the naked eye. The system is moving closer to the Earth with a heliocentric radial velocity of −14 km/s. J. Allen Hynek (1938) found an initial spectral type of G5 + A5 for the pair. It was first resolved by Harold A. McAlister (1978), who found an angular separation of 0.260″±0.002″ along a position angle of 133.0°±1.2°

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  • 17 Sagittarii is a binary star system in the zodiac constellation of Sagittarius, located 675 light years from the Sun. With a combined apparent visual magnitude of 6.89 it is below the normal limit of visibility to the naked eye. The system is moving closer to the Earth with a heliocentric radial velocity of −14 km/s. J. Allen Hynek (1938) found an initial spectral type of G5 + A5 for the pair. It was first resolved by Harold A. McAlister (1978), who found an angular separation of 0.260″±0.002″ along a position angle of 133.0°±1.2° The magnitude 7.24 primary component is an evolved giant star with a stellar classification of G8/K0 III, indicating it has exhausted the hydrogen at its core and expanded off the main sequence. It is radiating 73 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,700 K. The companion is a hot A-type star of uncertain luminosity class, with a visual magnitude of 8.89. (en)
  • 17 Sagittarii, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna, belägen i den norra delen av stjärnbilden Skytten. Den har en kombinerad skenbar magnitud på 6,89 och kräver åtminstone en handkikare för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 4,8 mas, beräknas den befinna sig på ett avstånd på ca 675 ljusår (ca 207 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -14 km/s. (sv)
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  • 1119031969 (xsd:integer)
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  • 0.680000 (xsd:double)
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  • 6.890000 (xsd:double)
  • (en)
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  • G8/K0 III + A4:: (en)
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  • J2000.0 (en)
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  • 73.210000 (xsd:double)
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  • 0.050500 (xsd:double)
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  • 4.828900 (xsd:double)
dbp:propMoDec
  • −14.342 (en)
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  • 10.978000 (xsd:double)
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  • 4700 (xsd:integer)
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  • 17 Sagittarii, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna, belägen i den norra delen av stjärnbilden Skytten. Den har en kombinerad skenbar magnitud på 6,89 och kräver åtminstone en handkikare för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 4,8 mas, beräknas den befinna sig på ett avstånd på ca 675 ljusår (ca 207 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -14 km/s. (sv)
  • 17 Sagittarii is a binary star system in the zodiac constellation of Sagittarius, located 675 light years from the Sun. With a combined apparent visual magnitude of 6.89 it is below the normal limit of visibility to the naked eye. The system is moving closer to the Earth with a heliocentric radial velocity of −14 km/s. J. Allen Hynek (1938) found an initial spectral type of G5 + A5 for the pair. It was first resolved by Harold A. McAlister (1978), who found an angular separation of 0.260″±0.002″ along a position angle of 133.0°±1.2° (en)
rdfs:label
  • 17 Sagittarii (en)
  • 17 Sagittarii (sv)
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  • 17 Sagittarii (en)
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