27 Vulpeculae

Star in the constellation Vulpecula From Wikipedia, the free encyclopedia

27 Vulpeculae is a single,[10] blue-white star in the northern constellation of Vulpecula. It is a dim star, visible to the naked eye, with an apparent visual magnitude of 5.59.[2] An annual parallax shift of 10.6692±0.0483 mas[1] provides a distance estimate of about 306 light-years. It is moving closer with a heliocentric radial velocity of −22 km/s,[6] and will make perihelion passage at a distance of around 119 ly (36.56 pc) in 3.75 million years.[5]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
27 Vulpeculae
27 Vulpeculae in the constellation Vulpecula
Observation data
Epoch J2000      Equinox J2000
Constellation Vulpecula
Right ascension 20h 37m 04.6724s[1]
Declination +26° 27 43.006[1]
Apparent magnitude (V) 5.590[2]
Characteristics
Evolutionary stage main sequence[1][3]
Spectral type B9 V[4][3]
B−V color index −0.050±0.004[5]
Astrometry
Radial velocity (Rv)−21.8±4.3[6] km/s
Proper motion (μ) RA: 15.349±0.042[1] mas/yr
Dec.: −11.775±0.040[1] mas/yr
Parallax (π)10.6692±0.0483 mas[1]
Distance306 ± 1 ly
(93.7 ± 0.4 pc)
Absolute magnitude (MV)0.65[5]
Details
Mass2.77±0.03[3] M
Radius3.1[7] R
Luminosity75.0+4.8
−4.5
[3] L
Surface gravity (log g)3.781[8] cgs
Temperature10,789+50
−49
[3] K
Metallicity [Fe/H]−0.27±0.04[5] dex
Rotational velocity (v sin i)335[3] km/s
Other designations
27 Vul, BD+25° 4302, FK5 3649, HD 196504, HIP 101716, HR 7880, SAO 88903[9]
Database references
SIMBADdata
Close

This is a B-type main-sequence star with a stellar classification of B9 V.[4] It is spinning rapidly, showing a projected rotational velocity of 335.[3] The star has an estimated 2.77[3] times the mass of the Sun and about 3.1[7] times the Sun's radius. It is radiating 75[3] times the Sun's luminosity from its photosphere at an effective temperature of 10,789 K.[3]

BD Vulpeculae

The location of the reddish colored carbon star BD Vulpeculae (CCCS 2916 / CGCS 4915) is, as seen from Earth, immediately northeast of 27 Vulpeculae. Astronomers and amateur astronomers could use 27 Vulpeculae as guidestar to try to find BD Vulpeculae and to see the color contrast of the bluish white star 27 Vulpeculae and the nearby reddish carbon star.

References

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