| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 10h 35m 24.7604s [1] |
| Declination | −76° 18′ 32.3366″ [1] |
| Apparent magnitude (V) | 6.29±0.01 [2] |
| Characteristics | |
| Spectral type | K2 III [3] |
| U−B color index | +1.27 [4] |
| B−V color index | +1.20 [4] |
| Astrometry | |
| Radial velocity (Rv) | 17.8±2.3 [5] km/s |
| Proper motion (μ) |
RA: −16.952
mas/
yr
[1] Dec.: +6.489 mas/ yr [1] |
| Parallax (π) | 5.4324 ± 0.1144 mas [1] |
| Distance | 600 ± 10
ly (184 ± 4 pc) |
| Absolute magnitude (MV) | −0.03 |
| Details | |
| Mass | 1.22 [6] M☉ |
| Radius | 14.39 [7] R☉ |
| Luminosity | 81.3+9.9 −8.8 [8] L☉ |
| Surface gravity (log g) | 1.76 [6] cgs |
| Temperature | 4,460±90 [8] K |
| Metallicity [Fe/H] | +0.06 [9] dex |
| Rotational velocity (v sin i) | <1 [10] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 92209 (HR 4170) is a probable spectroscopic binary [10] in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.29, [2] placing it near the max naked eye visibility. Parallax measurements place the system at a distance of 600 light years [1] and is currently receding with a heliocentric radial velocity of almost 18 km/s. [5]
The visible component has a stellar classification of K2 III, [3] indicating that it is a red giant. As a consequence, it has expanded to 14.39 times the radius of the Sun. [7] Nevertheless, it has 122% the mass of the Sun [6] and shines with a luminosity of 81.3 L☉, [8] yielding an effective temperature of 4,460 K [8] from its enlarged photosphere, which in turn gives an orange hue. HD 92209 has a metallicity 115% that of the Sun [9] and spins leisurely with a projected rotational velocity lower than 1 km/s. [10]
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 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H. ISSN 0004-6361.
- ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode: 1975mcts.book.....H.
- ^ 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 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.
- ^ a b c 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 Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv: 2109.10912. Bibcode: 2022A&A...657A...7K. doi: 10.1051/0004-6361/202142146. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b c d Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics. 633: A34. arXiv: 1910.12732. Bibcode: 2020A&A...633A..34C. doi: 10.1051/0004-6361/201936360. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Eggen, O. J. (February 1994). "Evolved GK stars near the Sun. 2: The young disk population". The Astronomical Journal. 107: 594. Bibcode: 1994AJ....107..594E. doi: 10.1086/116879. ISSN 0004-6256.
- ^ a b c De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. ISSN 0004-6361.
- ^ "HD 92209". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 13, 2022.
- ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode: 1879RNAO....1.....G.
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 10h 35m 24.7604s [1] |
| Declination | −76° 18′ 32.3366″ [1] |
| Apparent magnitude (V) | 6.29±0.01 [2] |
| Characteristics | |
| Spectral type | K2 III [3] |
| U−B color index | +1.27 [4] |
| B−V color index | +1.20 [4] |
| Astrometry | |
| Radial velocity (Rv) | 17.8±2.3 [5] km/s |
| Proper motion (μ) |
RA: −16.952
mas/
yr
[1] Dec.: +6.489 mas/ yr [1] |
| Parallax (π) | 5.4324 ± 0.1144 mas [1] |
| Distance | 600 ± 10
ly (184 ± 4 pc) |
| Absolute magnitude (MV) | −0.03 |
| Details | |
| Mass | 1.22 [6] M☉ |
| Radius | 14.39 [7] R☉ |
| Luminosity | 81.3+9.9 −8.8 [8] L☉ |
| Surface gravity (log g) | 1.76 [6] cgs |
| Temperature | 4,460±90 [8] K |
| Metallicity [Fe/H] | +0.06 [9] dex |
| Rotational velocity (v sin i) | <1 [10] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 92209 (HR 4170) is a probable spectroscopic binary [10] in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.29, [2] placing it near the max naked eye visibility. Parallax measurements place the system at a distance of 600 light years [1] and is currently receding with a heliocentric radial velocity of almost 18 km/s. [5]
The visible component has a stellar classification of K2 III, [3] indicating that it is a red giant. As a consequence, it has expanded to 14.39 times the radius of the Sun. [7] Nevertheless, it has 122% the mass of the Sun [6] and shines with a luminosity of 81.3 L☉, [8] yielding an effective temperature of 4,460 K [8] from its enlarged photosphere, which in turn gives an orange hue. HD 92209 has a metallicity 115% that of the Sun [9] and spins leisurely with a projected rotational velocity lower than 1 km/s. [10]
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 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode: 2000A&A...355L..27H. ISSN 0004-6361.
- ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode: 1975mcts.book.....H.
- ^ 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 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.
- ^ a b c 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 Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics. 657: A7. arXiv: 2109.10912. Bibcode: 2022A&A...657A...7K. doi: 10.1051/0004-6361/202142146. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b c d Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics. 633: A34. arXiv: 1910.12732. Bibcode: 2020A&A...633A..34C. doi: 10.1051/0004-6361/201936360. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Eggen, O. J. (February 1994). "Evolved GK stars near the Sun. 2: The young disk population". The Astronomical Journal. 107: 594. Bibcode: 1994AJ....107..594E. doi: 10.1086/116879. ISSN 0004-6256.
- ^ a b c De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. ISSN 0004-6361.
- ^ "HD 92209". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 13, 2022.
- ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode: 1879RNAO....1.....G.