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| '''Zeta Delphini''' ('''ζ Delphini''') is a ] in the ] of ]. With an apparent magnitude of about 4.6,<ref name=TYC2/> it is faintly visible to the naked eye. ] measurements of the system made by the ] ] put it at a distance of about 220 ]s, or 67 ]s.<ref name=HIP/> | '''Zeta Delphini''' ('''ζ Delphini''') is a ] in the ] of ]. With an apparent magnitude of about 4.6,<ref name=TYC2/> it is faintly visible to the naked eye. ] measurements of the system made by the ] ] put it at a distance of about 220 ]s, or 67 ]s.<ref name=HIP/> | ||
| Zeta Delphini has a spectral type of A3V, implying it is an ].<ref name=vast/> These types of stars are bluish-white colored, and have ]s between 7100 and 11500 ]:<ref>{{cite journal|title=The physical properties of normal A stars|author=Adelman, Saul J.|journal=Proceedings of the International Astronomical Union|volume=2004|pages=1|date=2004|bibcode=2004IAUS..224....1A|doi=10.1017/S1743921304004314}}</ref> Zeta Delphini has a temperature of 8336 K.<ref name=vast/> Its age is estimated to be around 500 million light years, considerably younger than the Sun.<ref name=vast/> | Zeta Delphini has a spectral type of A3V, implying it is an ].<ref name=vast/> These types of stars are bluish-white colored, and have ]s between 7100 and 11500 ]:<ref>{{cite journal|title=The physical properties of normal A stars|author=Adelman, Saul J.|journal=Proceedings of the International Astronomical Union|volume=2004|pages=1|date=2004|bibcode=2004IAUS..224....1A|doi=10.1017/S1743921304004314|doi-access=free}}</ref> Zeta Delphini has a temperature of 8336 K.<ref name=vast/> Its age is estimated to be around 500 million light years, considerably younger than the Sun.<ref name=vast/> | ||
| In 2014, the discovery of a ] around Zeta Delphini was announced. Zeta Delphini B is a brown dwarf with a ] of L5 (but may be from L3 to L7), and has a mass of about 55 ]s. At over 13 ]s away, this brown dwarf is separated at least 910 ] from Zeta Delphini.<ref name=vast/> | In 2014, the discovery of a ] around Zeta Delphini was announced. Zeta Delphini B is a brown dwarf with a ] of L5 (but may be from L3 to L7), and has a mass of about 55 ]s. At over 13 ]s away, this brown dwarf is separated at least 910 ] from Zeta Delphini.<ref name=vast/> | ||
Revision as of 16:47, 13 April 2020
Star in the constellation Delphinus
Location of ζ Delphini (circled) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Delphinus |
| Right ascension | 20 35 18.53563 |
| Declination | +14° 40′ 27.1675″ |
| Apparent magnitude (V) | +4.647 |
| Characteristics | |
| Spectral type | A3Va / L5 |
| U−B color index | +0.14 |
| B−V color index | +0.105 |
| Astrometry | |
| Radial velocity (Rv) | −25 ± 2 km/s |
| Proper motion (μ) | RA: 45.52 mas/yr Dec.: 11.74 mas/yr |
| Parallax (π) | 14.82 ± 0.23 mas |
| Distance | 220 ± 3 ly (67 ± 1 pc) |
| Absolute bolometric magnitude (Mbol) | 0.523 / 14.59 |
| Details | |
| ζ Del A | |
| Mass | 2.5 ± 0.2 M☉ |
| Luminosity | 48.63 ± 1.66 L☉ |
| Surface gravity (log g) | 3.72 cgs |
| Temperature | 8336 K |
| Metallicity | −0.05 dex |
| Age | 525 ± 125 Myr |
| ζ Del B | |
| Mass | 55 ± 10 MJup |
| Luminosity | 0.00012 ± 0.00001 L☉ |
| Surface gravity (log g) | 5.0+0.5 −1.0 cgs |
| Temperature | 1550+250 −100 K |
| Age | 525 ± 125 Myr |
| Other designations | |
| 4 Delphini, BD+14°4353, HD 196180, HIP 101589, HR 7871, SAO 106274 | |
| Database references | |
| SIMBAD | ζ Del |
| ζ Del B | |
Zeta Delphini (ζ Delphini) is a star in the constellation of Delphinus. With an apparent magnitude of about 4.6, it is faintly visible to the naked eye. Parallax measurements of the system made by the Hipparcos spacecraft put it at a distance of about 220 light-years, or 67 parsecs.
Zeta Delphini has a spectral type of A3V, implying it is an A-type main-sequence star. These types of stars are bluish-white colored, and have effective temperatures between 7100 and 11500 K: Zeta Delphini has a temperature of 8336 K. Its age is estimated to be around 500 million light years, considerably younger than the Sun.
In 2014, the discovery of a brown dwarf around Zeta Delphini was announced. Zeta Delphini B is a brown dwarf with a spectral type of L5 (but may be from L3 to L7), and has a mass of about 55 Jupiters. At over 13 arcseconds away, this brown dwarf is separated at least 910 AU from Zeta Delphini.
References
- ^ van Leeuwen, F.; et al. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ^ Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27 – L30. Bibcode:2000A&A...355L..27H.
- ^ De Rosa, R. J.; Patience, J.; Ward-Duong, K.; Vigan, A.; Marois, C.; Song, I.; MacIntosh, B.; Graham, J. R.; Doyon, R.; Bessell, M. S.; Lai, O.; McCarthy, D. W.; Kulesa, C. (2014). "The VAST Survey - IV. A wide brown dwarf companion to the A3V star ζ Delphini". Monthly Notices of the Royal Astronomical Society. 445 (4): 3694. arXiv:1410.0005. Bibcode:2014MNRAS.445.3694D. doi:10.1093/mnras/stu2018.
{{cite journal}}: CS1 maint: unflagged free DOI (link) - ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
- Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode:1953GCRV..C......0W.
- "zet+Del". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 5 March 2017.
- Adelman, Saul J. (2004). "The physical properties of normal A stars". Proceedings of the International Astronomical Union. 2004: 1. Bibcode:2004IAUS..224....1A. doi:10.1017/S1743921304004314.
External links
Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy & Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691.
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