V354 Cephei | |
---|---|
Observational Data | |
Designation | IRAS 22317+5838 |
Right ascension | 22h 33m 34.6349s[1][2] |
Declination | +58° 52′ 47.1259″[1][2] |
Constellation | Cepheus |
Type of object | Supergiant |
Magnitude | Apparent Mag: +10.42[3] |
Astrometry | |
Distance from Earth | 9,000 ly[3] |
Radial velocity | -59.42 ± 0.28 km/s[1][2] |
Proper motion | RA: -2.816 mas/yr[1][2] Dec: -2.510 mas/yr[1][2] |
Parallax | 0.4581 ± 0.1023 mas[1][2] |
V354 Cephei is a supergiant star in the constellation of Cepheus.[4] It is one of the largest stars known, thought to have a radius over 1,500 times greater than the Sun's. This would mean the star's outer layers extend significantly beyond Saturn if it replaced the Sun.[5] While it has one of the largest radii of any star known, it has a more modest mass estimated at 25 solar masses.[5] Its luminosity is estimated to be 300, times greater than Sol's. A medium sized (4.5 - 6.0 inches) telescope is required to observe the star as although large, it appears faint in the night sky.
V354 Cephei is located 9,000 light years from Earth meaning it shines with an apparent magnitude of +10.42.[3] The star is known to be a variable star with its magnitude varying by around 0.5.[6][7] The star's period is not known, it may be an irregular variable.
Categories: [Astronomy] [Stars]