3 Vulpeculae
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Vulpecula |
| Right ascension | 19h 22m 50.88540s[1] |
| Declination | +26° 15′ 44.6676″[1] |
| Apparent magnitude (V) | 5.18[2] |
| Characteristics | |
| Spectral type | B6 III[3] |
| B−V color index | −0.119±0.001[2] |
| Variable type | SPB[4][5] |
| Astrometry | |
| Radial velocity (Rv) | −14.1±1.1[2] km/s |
| Proper motion (μ) | RA: +1.081[1] mas/yr Dec.: −10.270[1] mas/yr |
| Parallax (π) | 9.0575 ± 0.1967 mas[1] |
| Distance | 360 ± 8 ly (110 ± 2 pc) |
| Absolute magnitude (MV) | −0.17[2] |
| Orbit[4] | |
| Period (P) | 367.7 |
| Eccentricity (e) | 0.15 |
| Semi-amplitude (K1) (primary) | 6.8 km/s |
| Details | |
| A | |
| Mass | 4.16[4] M☉ |
| Luminosity | 286+64 −52[6] L☉ |
| Surface gravity (log g) | 4.30[4] cgs |
| Temperature | 14,343[4] K |
| Rotational velocity (v sin i) | 15.5[7] km/s |
| B | |
| Mass | 0.6 - 1.1[4] M☉ |
| Age | 25[4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
3 Vulpeculae (abbreviated 3 Vul) is a binary star system in the northern constellation of Vulpecula,[8] located around 360 light years away from the Sun.[1] 3 Vulpeculae is its Flamsteed designation. It has been nicknamed "the Observer's Nightmare" (or its Latin free translation, "Spectatori Error Inextricabilis") by some astronomers[9][4] because it is difficult to study as its orbital period is close to a year and it is pulsating with a period close to a day.[4] It is visible to the naked eye as a faint, blue-white hued star with a baseline apparent visual magnitude of 5.18.[2]
The primary member, designated component A, is a most likely a B-type main-sequence star[6] with a stellar classification of B6 III.[3] It has been identified as a slowly pulsating B-type star,[4] and has the variable star designation V377 Vulpeculae. The star has 4.16[4] times the mass of the Sun and is radiating 286[6] times the Sun's luminosity from its photosphere at an effective temperature of 14,343 K.[4] The secondary has an estimated 0.6–1.1 solar masses.[4]
References
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.
- ^ a b Cucchiaro, A.; Macau-Hercot, D.; Jaschek, M.; Jaschek, C. (1977). "Spectral classification from the ultraviolet line features of S2/68 spectra. II - Late B-type stars". Astronomy and Astrophysics Supplement Series. 30: 71. Bibcode:1977A&AS...30...71C.
- ^ a b c d e f g h i j k l m Dukes, Robert; Kubinec, William; Kubinec, Angela; Adelman, Saul (2003). "A Photometric and Spectroscopic Study of 3 Vulpeculae: An Observer's Nightmare". The Astronomical Journal. 126 (1): 370. Bibcode:2003AJ....126..370D. doi:10.1086/375463.
- ^ Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
- ^ a b c Walczak, P.; et al. (December 2012). "Constraints on stellar parameters of the slowly pulsating B star HD 182255 from complex asteroseismology". Astronomische Nachrichten. 333 (10): 1065. arXiv:1212.4643. Bibcode:2012AN....333.1065W. doi:10.1002/asna.201211824. S2CID 116926922.
- ^ Zverko, J.; Romanyuk, I.; Iliev, I.; Kudryavtsev, D.; Stateva, I.; Semenko, E. (April 2016). "Stars with discrepant v sin i as derived from the Ca II λ3933 Å and Mg II λ4481 Å lines. V. HD 182255 and HD 214923—SPB stars in binary systems". Astrophysical Bulletin. 71 (2): 199–207. Bibcode:2016AstBu..71..199Z. doi:10.1134/S1990341316020073. S2CID 124871780.
- ^ a b "3 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-03-13.
- ^ Kaler, Jim. "3 Vul". Retrieved 2016-08-09.
