Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 20h 57m 10.41907s [1] |
Declination | 41° 10′ 01.6991″ [1] |
Apparent magnitude (V) | 3.94 [2] |
Characteristics | |
Spectral type | A0III n [3] |
U−B color index | +0.00 [2] |
B−V color index | +0.02 [2] |
Astrometry | |
Radial velocity (Rv) | −27.60 [4] km/s |
Proper motion (μ) | RA: +9.64 [1] mas/yr Dec.: −22.75 [1] mas/yr |
Parallax (π) | 8.71 ± 0.34 [1] mas |
Distance | 370 ± 10 ly (115 ± 4 pc) |
Absolute magnitude (MV) | −1.36 [5] |
Details | |
ν Cyg A | |
Mass | ±0.08 3.62[6] M☉ |
Radius | 1.90 [7] R☉ |
Luminosity | 412 [6] L☉ |
Temperature | 9,462 [6] K |
Rotational velocity (v sin i) | 217 [6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Nu Cygni, Latinized from ν Cygni, is a binary star [9] system in the constellation Cygnus. Its apparent magnitude is 3.94 [2] and it is approximately 374 light years away based on parallax. [1] The brighter component is a magnitude 4.07 A-type giant star with a stellar classification of A0III n, [3] where the 'n' indicates broad "nebulous" absorption lines due to rapid rotation. This white-hued star has an estimated 3.6 [6] times the mass of the Sun and about 1.9 [7] times the Sun's radius. It is radiating 412 [6] times the Sun's luminosity from its photosphere at an effective temperature of 9,462 K. [6] The magnitude 6.4 companion has an angular separation of 0.24" from the primary. [9]
Latinisation of names, also known as onomastic Latinisation, is the practice of rendering a non-Latin name in a Latin style. It is commonly found with historical proper names, including personal names, and toponyms, and in the standard binomial nomenclature of the life sciences. It goes further than romanisation, which is the transliteration of a word to the Latin alphabet from another script.
A binary star is a star system consisting of two stars orbiting around their common barycenter. Systems of two or more stars are called multiple star systems. These systems, especially when more distant, often appear to the unaided eye as a single point of light, and are then revealed as multiple by other means. Research over the last two centuries suggests that half or more of visible stars are part of multiple star systems.
A constellation is a group of stars that forms an imaginary outline or pattern on the celestial sphere, typically representing an animal, mythological person or creature, a god, or an inanimate object.
Beta Sculptoris, Latinized from β Sculptoris, is a single, blue-white hued star in the southern constellation of Sculptor. It has an apparent visual magnitude of 4.37, which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 18.74 mas as seen from Earth, it is located 174 light years from the Sun.
67 Ophiuchi is a class B5 Ib star in the constellation Ophiuchus. Its apparent magnitude is 3.93 and it is approximately 1200 light years away based on parallax. It is considered to be a member of the open cluster Collinder 359.
23 Vulpeculae is a class K3III star in a triple star system in the constellation Vulpecula. Its apparent magnitude is 4.52 and it is approximately 339 light years away based on parallax. It has two reported companions; Ab has a separation of 0.11", a magnitude of 6.5, and a period of about 25 years, while B has a separation of 0.26" and a magnitude of 6.94.
29 Vulpeculae is a class A0V star in the constellation Vulpecula. Its apparent magnitude is 4.82 and it is approximately 209 light years away based on parallax. Radial velocity measurements from High Accuracy Radial Velocity Planet Searcher with an amplitude of 4 km/s indicate that it is a spectroscopic binary of unknown period.
12 Vulpeculae is a star in the northern constellation of Vulpecula, located approximately 630 light years away based on parallax. It has the variable star designation V395 Vul; 12 Vulpeculae is the Flamsteed designation. This object is visible to the naked eye as a faint, blue-white hued star with a baseline apparent visual magnitude of 4.96. It is moving closer to the Earth with a heliocentric radial velocity of -25 km/s.
Psi Ophiuchi is a class K0II-III star in the constellation Ophiuchus. Its apparent magnitude is 4.50 and it is approximately 199 light years away based on parallax.
30 Leonis Minoris is a class F0V star in the constellation Leo Minor. Its apparent magnitude is 4.72 and it is approximately 233 light years away based on parallax.
20 Monocerotis is a class K0III star in the constellation Monoceros. Its apparent magnitude is 4.92 and it is approximately 203 light years away based on parallax.
Phi Ophiuchi is a class G8+IIIa star in the constellation Ophiuchus. Its apparent magnitude is 4.27 and it is approximately 244 light years away based on parallax.
Iota Ophiuchi is a class B8V star in the constellation Ophiuchus. Its apparent magnitude is 4.39 and it is approximately 245 light years away based on parallax.
HD 40657 is a class K1.5III star in the constellation Orion. Its apparent magnitude is 4.52 and it is approximately 420 light years away based on parallax.
49 Orionis is a class A4V star in the constellation Orion. Its apparent magnitude is 4.80 and it is approximately 145 light years away based on parallax.
32 Pegasi is a class B9III star in the constellation Pegasus. Its apparent magnitude is 4.81 and it is approximately 700 light years away based on parallax.
Rho Pegasi is a class A1V star in the constellation Pegasus. Its apparent magnitude is 4.90 and it is approximately 312 light years away based on parallax. This is a probable astrometric binary system, as determined by changes to the proper motion of the visible component.
Epsilon Phoenicis is a star in the constellation Phoenix. Its apparent magnitude is 3.87. Located around 144 parsecs (470 ly) distant, it is an orange giant of spectral type K0III, a star that has used up its core hydrogen and has expanded.
Mu Phoenicis is a class G8III star in the constellation Phoenix. Its apparent magnitude is 4.59 and it is approximately 246 light years away based on parallax.
QW Puppis is a class F3V star in the constellation Puppis. Its apparent magnitude is 4.49 and it is approximately 69.9 light years away based on parallax.
HD 65810 is a class A2V star in the constellation Puppis. Its apparent magnitude is 4.61 and it is approximately 241 light years away based on parallax.
MX Puppis is a class B1.5IV star in the constellation Puppis. Its apparent magnitude varies irregularly between magnitude 4.6 and 4.9 and it is classified as a Gamma Cassiopeiae variable. It is approximately 930 light years away based on parallax.
20 Puppis is a class G5II star in the constellation Puppis. Its apparent magnitude is 4.99 and it is approximately 870 light years away based on parallax.