  | |
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 10h 52m 28.63166s [1] |
| Declination | −79° 33′ 33.9765″ [1] |
| Apparent magnitude (V) | 6.34±0.01 [2] |
| Characteristics | |
| Spectral type | K2 II/III [3] |
| U−B color index | +1.57 [4] |
| B−V color index | +1.46 [4] |
| Astrometry | |
| Radial velocity (Rv) | 3.4±0.5 [5] km/s |
| Proper motion (μ) |
RA: −11.341
mas/
yr
[1] Dec.: +1.655 mas/ yr [1] |
| Parallax (π) | 1.8682 ± 0.021 mas [1] |
| Distance | 1,750 ± 20
ly (535 ± 6 pc) |
| Absolute magnitude (MV) | −2.10 [6] |
| Details | |
| Mass | 6.3±0.7 [7] M☉ |
| Radius | 77.8±3.9 [8] R☉ |
| Luminosity | 1,847+46 −49 [1] L☉ |
| Surface gravity (log g) | 1.47±0.04 [1] cgs |
| Temperature | 4,446±122 [9] K |
| Metallicity [Fe/H] | −0.01 [1] dex |
| Rotational velocity (v sin i) | 2.4±1.3 [10] km/s |
| Age | 63±20 [7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 94717, also known as HR 4268, is a solitary orange hued star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.34, [2] placing it near the limit for naked eye visibility. The object is located relatively far at a distance of 1,750 light years based on Gaia DR3 parallax measurements, [1] but it is receding with a heliocentric radial velocity of 3.4 km/s. [5] At its current distance, HD 94717's brightness is diminished by 0.62 magnitudes due to interstellar dust. [13]
HD 94717 has a stellar classification of K2 II/III, [3] indicating that it is an evolved red giant with the blended luminosity class of a giant star and a bright giant. It is estimated to be 63 million years old, [7] enough time for it to cool and expand to 78 times the Sun's radius. [8] It has 6.3 times the mass of the Sun [7] and radiates 1,847 times the luminosity of the Sun [1] from its photosphere at an effective temperature of 4,446 K. [9] HD 94717 has a solar metallicity [1] and spins modestly with a projected rotational velocity of 2.4 km/s. [10]
- ^ a b c d e f g h i j Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211. Bibcode: 2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 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°. 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. eISSN 1562-6873. ISSN 1063-7737. S2CID 119231169.
- ^ Corbally, C. J.; Garrison, R. F. (1984). "Which Map of Absolute Magnitudes: Keenan or Schmidt-Kaler?". The Mk Process and Stellar Classification: 277. Bibcode: 1984mpsc.conf..277C.
- ^ a b c d Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (October 12, 2010). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". Monthly Notices of the Royal Astronomical Society. 410 (1). Oxford University Press (OUP): 190–200. arXiv: 1007.4883. Bibcode: 2011MNRAS.410..190T. doi: 10.1111/j.1365-2966.2010.17434.x. ISSN 0035-8711.
- ^ a b Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004). "The angular sizes of dwarf stars and subgiants". Astronomy & Astrophysics. 426 (1): 297–307. arXiv: astro-ph/0404180. Bibcode: 2004A&A...426..297K. doi: 10.1051/0004-6361:20035930. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. eISSN 1538-3881. hdl: 1721.1/124721. S2CID 166227927.
- ^ a b 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". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. eISSN 1432-0746. ISSN 0004-6361.
- ^ 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.
- ^ "HD 94717". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 December 2022.
- ^ Guarinos, J. (February 1995). "VizieR Online Data Catalog: Interstellar matter in the Galactic Disk (Guarinos J., 1992)". VizieR Online Data Catalog: 301V/86. Bibcode: 1995yCat.5086....0G.
| |
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 10h 52m 28.63166s [1] |
| Declination | −79° 33′ 33.9765″ [1] |
| Apparent magnitude (V) | 6.34±0.01 [2] |
| Characteristics | |
| Spectral type | K2 II/III [3] |
| U−B color index | +1.57 [4] |
| B−V color index | +1.46 [4] |
| Astrometry | |
| Radial velocity (Rv) | 3.4±0.5 [5] km/s |
| Proper motion (μ) |
RA: −11.341
mas/
yr
[1] Dec.: +1.655 mas/ yr [1] |
| Parallax (π) | 1.8682 ± 0.021 mas [1] |
| Distance | 1,750 ± 20
ly (535 ± 6 pc) |
| Absolute magnitude (MV) | −2.10 [6] |
| Details | |
| Mass | 6.3±0.7 [7] M☉ |
| Radius | 77.8±3.9 [8] R☉ |
| Luminosity | 1,847+46 −49 [1] L☉ |
| Surface gravity (log g) | 1.47±0.04 [1] cgs |
| Temperature | 4,446±122 [9] K |
| Metallicity [Fe/H] | −0.01 [1] dex |
| Rotational velocity (v sin i) | 2.4±1.3 [10] km/s |
| Age | 63±20 [7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 94717, also known as HR 4268, is a solitary orange hued star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.34, [2] placing it near the limit for naked eye visibility. The object is located relatively far at a distance of 1,750 light years based on Gaia DR3 parallax measurements, [1] but it is receding with a heliocentric radial velocity of 3.4 km/s. [5] At its current distance, HD 94717's brightness is diminished by 0.62 magnitudes due to interstellar dust. [13]
HD 94717 has a stellar classification of K2 II/III, [3] indicating that it is an evolved red giant with the blended luminosity class of a giant star and a bright giant. It is estimated to be 63 million years old, [7] enough time for it to cool and expand to 78 times the Sun's radius. [8] It has 6.3 times the mass of the Sun [7] and radiates 1,847 times the luminosity of the Sun [1] from its photosphere at an effective temperature of 4,446 K. [9] HD 94717 has a solar metallicity [1] and spins modestly with a projected rotational velocity of 2.4 km/s. [10]
- ^ a b c d e f g h i j Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211. Bibcode: 2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 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°. 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. eISSN 1562-6873. ISSN 1063-7737. S2CID 119231169.
- ^ Corbally, C. J.; Garrison, R. F. (1984). "Which Map of Absolute Magnitudes: Keenan or Schmidt-Kaler?". The Mk Process and Stellar Classification: 277. Bibcode: 1984mpsc.conf..277C.
- ^ a b c d Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (October 12, 2010). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". Monthly Notices of the Royal Astronomical Society. 410 (1). Oxford University Press (OUP): 190–200. arXiv: 1007.4883. Bibcode: 2011MNRAS.410..190T. doi: 10.1111/j.1365-2966.2010.17434.x. ISSN 0035-8711.
- ^ a b Kervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004). "The angular sizes of dwarf stars and subgiants". Astronomy & Astrophysics. 426 (1): 297–307. arXiv: astro-ph/0404180. Bibcode: 2004A&A...426..297K. doi: 10.1051/0004-6361:20035930. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694. Bibcode: 2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467. eISSN 1538-3881. hdl: 1721.1/124721. S2CID 166227927.
- ^ a b 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". Astronomy & Astrophysics. 561: A126. arXiv: 1312.3474. Bibcode: 2014A&A...561A.126D. doi: 10.1051/0004-6361/201220762. eISSN 1432-0746. ISSN 0004-6361.
- ^ 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.
- ^ "HD 94717". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 December 2022.
- ^ Guarinos, J. (February 1995). "VizieR Online Data Catalog: Interstellar matter in the Galactic Disk (Guarinos J., 1992)". VizieR Online Data Catalog: 301V/86. Bibcode: 1995yCat.5086....0G.