V604 Aquilae - definição. O que é V604 Aquilae. Significado, conceito
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O que (quem) é V604 Aquilae - definição


V604 Aquilae         
  • The location of  V604 Aquilae (circled in red)
STAR IN THE CONSTELLATION AQUILA
Nova Aquilae 1905; AAVSO 1856-04; HD 176779; V604; V604 Aql
V604 Aquilae or Nova Aquilae 1905 was a nova, which was first observed in the constellation Aquila in 1905 with a maximum brightness of 7.6 mag.
Omega Aquilae         
WIKIMEDIA DISAMBIGUATION PAGE
Ω Aquilae
The Bayer designation Omega Aquilae (ω Aql / ω Aquilae) is shared by two stars in the constellation Aquila:
Altair         
  • A [[light curve]] for Altair, adapted from Buzasi ''et al.'' (2005)<ref name="Buzasi et al 2005"/>
  • Altair in comparison with the Sun
  • Altair is the brightest star in the constellation Aquila
STAR IN THE CONSTELLATION AQUILA
Alpha Aquilae; Atair; Α Aquilae; Α Aql; Altair (star); SAO 125122; HIP 97649; 53 Aquilae; HD 187642; HR 7557; GJ 768; LHS 3490; ALTAIR; FK5 745; PPM 168779; 53 Aql; LFT 1499; Alpha Aql; GC 27470; ADS 13009 A; LTT 15795; BD+08 4236; BD +08 4236; NLTT 48314; IDS 19459+0836 A; ADS 13009; BD+08 4236B; BD +08 4236B; ADS 13009 B; IDS 19459+0836 B; BD+08 4238; BD +08 4238; ADS 13009 C; IDS 19459+0836 C; BD+08 4236C; BD +08 4236C; CCDM J19508+0852A; CCDM J19508+0852B; CCDM J19508+0852C; CCDM J19508+0852; IDS 19459+0836; ATAIR; BD+08 4236A; BD +08 4236A; 河鼓二; 牛郎星; Altair A; Star Altair; Gliese 768

Altair is the brightest star in the constellation of Aquila and the twelfth-brightest star in the night sky. It has the Bayer designation Alpha Aquilae, which is Latinised from α Aquilae and abbreviated Alpha Aql or α Aql. Altair is an A-type main-sequence star with an apparent visual magnitude of 0.77 and is one of the vertices of the Summer Triangle asterism; the other two vertices are marked by Deneb and Vega. It is located at a distance of 16.7 light-years (5.1 parsecs) from the Sun.: 194  Altair is currently in the G-cloud—a nearby interstellar cloud, an accumulation of gas and dust.

Altair rotates rapidly, with a velocity at the equator of approximately 286 km/s. This is a significant fraction of the star's estimated breakup speed of 400 km/s. A study with the Palomar Testbed Interferometer revealed that Altair is not spherical, but is flattened at the poles due to its high rate of rotation. Other interferometric studies with multiple telescopes, operating in the infrared, have imaged and confirmed this phenomenon.