HD 199223: Difference between revisions
Content deleted Content added
Lithopsian (talk | contribs) location chart |
Lithopsian (talk | contribs) ce |
||
| Line 88: | Line 88: | ||
{{Starbox end}} |
{{Starbox end}} |
||
'''HD 199223''' ('''HR 8010''') is a double star in the equatorial [[constellation]] [[Delphinus]]. However, the system was originally in [[Equuleus]] prior to the creation official [[International Astronomical Union|IAU]] constellation borders.<ref name = Davenhall1997/> The components have [[apparent magnitude]]s of 6.34 and 7.49 and distances of 354 and 359 [[light year]]s respectively. |
'''HD 199223''' ('''HR 8010''') is a double star in the equatorial [[constellation]] [[Delphinus]]. However, the system was originally in [[Equuleus]] prior to the creation of official [[International Astronomical Union|IAU]] constellation borders.<ref name = Davenhall1997/> The components have a separation of {{val|2|ul=arcsecond}} at a [[position angle]] of {{val|282|ul=°}} as of 2016.<ref name = Mason2001/> They have [[apparent magnitude]]s of 6.34 and 7.49 and distances of 354 and 359 [[light year]]s respectively. The system is drifting closer with a [[radial velocity]] of {{val|-33|ul=km/s}}. |
||
The brighter component has a [[stellar classification]] of G8 III/IV,<ref name = Harlan1974/> indicating that it is a [[G-type star]] with the blended [[luminosity]] class of a [[giant star]] and a [[subgiant]]. It has 125% the [[mass of the Sun]]<ref name = Anders2019/> and an enlarged |
The brighter component has a [[stellar classification]] of G8 III/IV,<ref name = Harlan1974/> indicating that it is a [[G-type star]] with the blended [[luminosity]] class of a [[giant star]] and a [[subgiant]]. It has 125% of the [[mass of the Sun]]<ref name = Anders2019/> and an enlarged radius of {{val|8.26|ul=solar radius}}.<ref name = DR2A/> It shines at 37.1 times the [[luminosity of the Sun]]<ref name = DR2A/> from its [[photosphere]] at an [[effective temperature]] of {{val|4956|ul=K|fmt=commas}},<ref name = DR2A/> giving it a yellow glow. HD 199223A's [[iron]] abundance is 135% that of the [[Sun]]<ref name = Randich1999/> and it spins modestly with a [[projected rotational velocity]] less than {{val|1|ul=km/s}}.<ref name = deMed1999/> |
||
As for the dimmer one, it is classified as an F/G star,<ref name = Houk1999/> |
As for the dimmer one, it is classified as an F/G star,<ref name = Houk1999/> and is calculated to be an [[F-type star|F-type]] subgiant. It has 146% of the mass of the Sun<ref name = Anders2019/> and 2.1 times its radius.<ref name = DR2B/> It radiates with a luminosity of {{val|8.82|ul=solar luminosity}}<ref name = DR2B/> from its photosphere at an effective temperature of {{val|6,865|fmt=commas|u=K}},<ref name = DR2B/> giving it a yellow white glow. |
||
The components have a separation of {{val|2|ul=arcsecond}} at a [[position angle]] of {{val|282|ul=°}} as of 2016.<ref name = Mason2001/> |
|||
==References== |
==References== |
||
Revision as of 12:15, 5 June 2022
  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Delphinus |
| A | |
| Right ascension | 20h 55m 40.6778s[1] |
| Declination | +04° 31′ 57.7994″[1] |
| Apparent magnitude (V) | 6.34±0.01[2] |
| B | |
| Right ascension | 20h 55m 40.5439s[3] |
| Declination | +04° 31′ 58.2271″[3] |
| Apparent magnitude (V) | 7.49±0.01[2] |
| Characteristics | |
| A | |
| Spectral type | G8 III/IV[4] |
| U−B color index | +0.49[5] |
| B−V color index | +0.82[5] |
| B | |
| Spectral type | F/G[6] |
| Astrometry | |
| Radial velocity (Rv) | −32.6±0.4[7] km/s |
| Absolute magnitude (MV) | +0.33[8] |
| A | |
| Proper motion (μ) | RA: +60.413[1] mas/yr Dec.: +10.949[1] mas/yr |
| Parallax (π) | 9.2067 ± 0.0354 mas[1] |
| Distance | 354 ± 1 ly (108.6 ± 0.4 pc) |
| B | |
| Proper motion (μ) | RA: +60.315[3] mas/yr Dec.: +9.758[3] mas/yr |
| Parallax (π) | 9.0757 ± 0.0758 mas[3] |
| Distance | 359 ± 3 ly (110.2 ± 0.9 pc) |
| Details | |
| A | |
| Mass | 1.25[9] M☉ |
| Radius | 8.26+0.65 −0.22[10] R☉ |
| Luminosity | 37.1±0.4[10] L☉ |
| Surface gravity (log g) | 2.60±0.25[11] cgs |
| Temperature | 4,956+68 −185[10] K |
| Metallicity [Fe/H] | 0.13±0.09[11] dex |
| Rotational velocity (v sin i) | <1[12] km/s |
| B | |
| Mass | 1.46[9] M☉ |
| Radius | 2.10+0.16 −0.27[13] R☉ |
| Luminosity | 8.82±0.23[13] L☉ |
| Surface gravity (log g) | 3.85[9] cgs |
| Temperature | 6,865+494 −251[13] K |
| Metallicity [Fe/H] | −0.2[9] dex |
| Other designations | |
| A: HD 199223A, WDS J20557+0432A | |
| B: HD 199223B, WDS J20557+0432B | |
| Database references | |
| SIMBAD | The system |
| A | |
| B | |
HD 199223 (HR 8010) is a double star in the equatorial constellation Delphinus. However, the system was originally in Equuleus prior to the creation of official IAU constellation borders.[14] The components have a separation of 2″ at a position angle of 282° as of 2016.[15] They have apparent magnitudes of 6.34 and 7.49 and distances of 354 and 359 light years respectively. The system is drifting closer with a radial velocity of −33 km/s.
The brighter component has a stellar classification of G8 III/IV,[4] indicating that it is a G-type star with the blended luminosity class of a giant star and a subgiant. It has 125% of the mass of the Sun[9] and an enlarged radius of 8.26 R☉.[10] It shines at 37.1 times the luminosity of the Sun[10] from its photosphere at an effective temperature of 4,956 K,[10] giving it a yellow glow. HD 199223A's iron abundance is 135% that of the Sun[11] and it spins modestly with a projected rotational velocity less than 1 km/s.[12]
As for the dimmer one, it is classified as an F/G star,[6] and is calculated to be an F-type subgiant. It has 146% of the mass of the Sun[9] and 2.1 times its radius.[13] It radiates with a luminosity of 8.82 L☉[13] from its photosphere at an effective temperature of 6,865 K,[13] giving it a yellow white glow.
References
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. (March 2002). "The Tycho double star catalogue". Astronomy & Astrophysics. 384 (1): 180–189. Bibcode:2002A&A...384..180F. doi:10.1051/0004-6361:20011822. ISSN 0004-6361.
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b Harlan, E. A. (June 1974). "MK classifications for F-and G-type stars. 3". The Astronomical Journal. 79: 682. Bibcode:1974AJ.....79..682H. doi:10.1086/111597. ISSN 0004-6256.
- ^ a b Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
- ^ a b Houk, N.; Swift, C. (1999). Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5. p. 0. Bibcode:1999MSS...C05....0H.
- ^ Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. ISSN 1063-7737. S2CID 119231169.
- ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. ISSN 1063-7737.
- ^ a b c d e f Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. ISSN 0004-6361.
- ^ 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 Randich, S.; Gratton, R.; Pallavicini, R.; Pasquini, L.; Carretta, E. (August 1999). "Lithium in population I subgiants". Astronomy and Astrophysics. 348: 487–500. Bibcode:1999A&A...348..487R. ISSN 0004-6361.
- ^ a b de Medeiros, J. R.; Mayor, M. (November 1999). "A catalog of rotational and radial velocities for evolved stars". Astronomy and Astrophysics Supplement Series. 139 (3): 433–460. Bibcode:1999A&AS..139..433D. doi:10.1051/aas:1999401. ISSN 0365-0138.
- ^ 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.
- ^ Davenhall, A. C.; Leggett, S. K. (May 1997). "VizieR Online Data Catalog: Constellation Boundary Data (Davenhall+ 1989)". VizieR Online Data Catalog: VI/49. Bibcode:1997yCat.6049....0D.
- ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi:10.1086/323920. ISSN 0004-6256.
