Astronomy:HD 64307
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Short description: Star in the constellation of Camelopardalis
| Observation data Epoch J2000.0 Equinox (celestial coordinates) | |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 08h 00m 11.7385s[1] |
| Declination | +73° 55′ 04.5036″[1] |
| Apparent magnitude (V) | 5.35±0.01[2] |
| Characteristics | |
| Evolutionary stage | red giant branch[3] |
| Spectral type | K3 III[4] |
| U−B color index | +1.64[5] |
| B−V color index | +1.43[5] |
| Astrometry | |
| Radial velocity (Rv) | 33.54±0.19[6] km/s |
| Proper motion (μ) | RA: −8.194[1] mas/yr Dec.: −37.514[1] mas/yr |
| Parallax (π) | 4.7407 ± 0.0741[1] mas |
| Distance | 690 ± 10 ly (211 ± 3 pc) |
| Absolute magnitude (MV) | −1.77[7] |
| Details | |
| Mass | 1.19[8] M☉ |
| Radius | 49.9[9] R☉ |
| Luminosity (bolometric) | 892[10] L☉ |
| Surface gravity (log g) | 1.18[8] cgs |
| Temperature | 4,264±122[11] K |
| Metallicity [Fe/H] | −0.1[12] dex |
| Rotational velocity (v sin i) | <2[13] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 64307, also known as HR 3075, is a solitary,[14] orange hued star located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.35,[2] allowing it to be faintly seen with the naked eye. Based on parallax measurements from the Gaia spacecraft, The object is estimated to be 690 light years[1] distant. It appears to be receding from the Sun, having a heliocentric radial velocity of 34 km/s.[6]
HD 64307 is an evolved star with a stellar classification of K3 III.[4] Gaia DR3 stellar evolution models place it on the red giant branch.[3] It has a mass comparable to the Sun[8] but due to its evolved state, it has an enlarged radius of 49.9 R☉. It shines with a bolometric luminosity of 892 solar luminosity from its photosphere at an effective temperature of 4,264 K.[11] HD 64307 has an iron abundance 80% that of the Sun, and is also lithium enriched.[12] Like most giant stars, the object spins slowly, having a projected rotational velocity lower than 2 km/s.[13]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G. Gaia EDR3 record for this source at VizieR.
- ↑ 2.0 2.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H.
- ↑ 3.0 3.1 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 4.0 4.1 Roman, Nancy G. (July 1952). "The Spectra of the Bright Stars of Types F5-K5.". The Astrophysical Journal 116: 122. doi:10.1086/145598. ISSN 0004-637X. Bibcode: 1952ApJ...116..122R.
- ↑ 5.0 5.1 Rybka, E. (1969). "The corrected magnitudes and colours of 278 stars msg ok near SA 1-139 in the UBV system.". Acta Astronomica 19: 229. ISSN 0001-5237. Bibcode: 1969AcA....19..229R.
- ↑ 6.0 6.1 Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (January 2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data: Revisiting the concept of superclusters". Astronomy & Astrophysics 430 (1): 165–186. doi:10.1051/0004-6361:20041272. ISSN 0004-6361. Bibcode: 2005A&A...430..165F.
- ↑ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation" (in en). Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode: 2012AstL...38..331A.
- ↑ 8.0 8.1 8.2 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. doi:10.1051/0004-6361/201935765. ISSN 0004-6361. Bibcode: 2019A&A...628A..94A.
- ↑ Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3". Astronomy & Astrophysics 657: A7. doi:10.1051/0004-6361/202142146. ISSN 0004-6361. Bibcode: 2022A&A...657A...7K.
- ↑ McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (21 November 2012). "Fundamental parameters and infrared excesses of Hipparcos stars: Parameters and IR excesses from Hipparcos". Monthly Notices of the Royal Astronomical Society 427 (1): 343–357. doi:10.1111/j.1365-2966.2012.21873.x. ISSN 0035-8711. Bibcode: 2012MNRAS.427..343M.
- ↑ 11.0 11.1 Stassun, Keivan G. et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S.
- ↑ 12.0 12.1 Brown, Jeffery A.; Sneden, Christopher; Lambert, David L.; Dutchover, Edward Jr. (October 1989). "A search for lithium-rich giant stars". The Astrophysical Journal Supplement Series 71: 293. doi:10.1086/191375. ISSN 0067-0049. Bibcode: 1989ApJS...71..293B.
- ↑ 13.0 13.1 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. doi:10.1051/aas:1999401. ISSN 0365-0138. Bibcode: 1999A&AS..139..433D.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society 389 (2): 869–879. doi:10.1111/j.1365-2966.2008.13596.x. Bibcode: 2008MNRAS.389..869E.
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