| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Leo Minor |
| Right ascension | 10h 39m 07.63244s [1] |
| Declination | +37° 54′ 36.0035″ [1] |
| Apparent magnitude (V) | 5.84 [2] |
| Characteristics | |
| Spectral type | G0 IV [3] |
| B−V color index | 0.595±0.003 [2] |
| Astrometry | |
| Radial velocity (Rv) | +30.9±0.3 [4] km/s |
| Proper motion (μ) |
RA: −220.50
[1]
mas/
yr Dec.: −45.31 [1] mas/ yr |
| Parallax (π) | 19.11 ± 0.37 mas [1] |
| Distance | 171 ± 3
ly (52 ± 1 pc) |
| Absolute magnitude (MV) | 2.26 [5] |
| Orbit [5] | |
| Period (P) | 7.7991499±0.0000037 d |
| Eccentricity (e) | 0.023±0.034 |
| Periastron epoch (T) | 20,165.164±1.470 HJD |
|
Argument of periastron (ω) (secondary) | 285.56±68.51° |
|
Semi-amplitude (K1) (primary) | 24.10±0.73 km/s |
| Details | |
| 38 LMi A | |
| Mass | 1.68 [6] M☉ |
| Luminosity | 11.32 [2] L☉ |
| Surface gravity (log g) | 3.73 [6] cgs |
| Temperature | 6,106 [7] K |
| Metallicity [Fe/H] | +0.32 [7] dex |
| Rotational velocity (v sin i) | 14.5±1.0 [5] km/s |
| Age | 2.03±0.14 [7] Gyr |
| 38 LMi B | |
| Mass | ≥ 0.31 [8] M☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
38 Leonis Minoris is a binary star [3] system in the northern constellation of Leo Minor. It shines with a combined light of apparent magnitude 5.84, [2] which indicates it a dimly visible to the naked eye under good viewing conditions. An annual parallax shift of 19.11 [1] mas provides a distance estimate of around 171 light years. It has a relatively high proper motion, traversing the celestial sphere at a rate of 0.226 arcseconds per year, [10] and is moving away from the Sun with a radial velocity of +31 km/s. [4]
This is a single-lined spectroscopic binary [3] with an orbital period of 7.8 days and a low eccentricity of 0.023 – nearly circular. [5] The visible component has a stellar classification of G0 IV, [3] matching a G-type subgiant star that is exhausting the hydrogen at its core and evolving into a giant. It is about two [7] billion years old with 1.68 [6] times the mass of the Sun and is spinning with a projected rotational velocity of 14.5 km/s. [5] The star has a higher than solar abundance of iron in its spectrum. [7] It is radiating 11 [2] times the Sun's luminosity from its photosphere at an effective temperature of 6,106 K. [7]
- ^ a b c d e f van Leeuwen, F. (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, S2CID 18759600.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c d Abt, Helmut A. (2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement, 180 (1): 117–18, Bibcode: 2009ApJS..180..117A, doi: 10.1088/0067-0049/180/1/117, S2CID 122811461.
- ^ a b de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv: 1208.3048, Bibcode: 2012A&A...546A..61D, doi: 10.1051/0004-6361/201219219, S2CID 59451347, A61.
- ^ a b c d e Willmarth, Daryl W.; et al. (August 2016), "Spectroscopic Orbits for 15 Late-type Stars" (PDF), The Astronomical Journal, 152 (2): 13, Bibcode: 2016AJ....152...46W, doi: 10.3847/0004-6256/152/2/46, S2CID 53648490, 46.
- ^ a b c Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy and Astrophysics, 530: A138, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID 56118016.
- ^ a b c d e f Pace, G. (March 2013), "Chromospheric activity as age indicator. An L-shaped chromospheric-activity versus age diagram", Astronomy & Astrophysics, 551: 4, arXiv: 1301.5651, Bibcode: 2013A&A...551L...8P, doi: 10.1051/0004-6361/201220364, S2CID 56420519, L8.
- ^ Tokovinin, A.; et al. (May 2006), "Tertiary companions to close spectroscopic binaries", Astronomy and Astrophysics, 450 (2): 681–69, arXiv: astro-ph/0601518, Bibcode: 2006A&A...450..681T, doi: 10.1051/0004-6361:20054427, S2CID 8899546.
- ^ "38 LMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-02-20.
- ^ Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal, 129 (3): 1483–1522, arXiv: astro-ph/0412070, Bibcode: 2005AJ....129.1483L, doi: 10.1086/427854, S2CID 2603568.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Leo Minor |
| Right ascension | 10h 39m 07.63244s [1] |
| Declination | +37° 54′ 36.0035″ [1] |
| Apparent magnitude (V) | 5.84 [2] |
| Characteristics | |
| Spectral type | G0 IV [3] |
| B−V color index | 0.595±0.003 [2] |
| Astrometry | |
| Radial velocity (Rv) | +30.9±0.3 [4] km/s |
| Proper motion (μ) |
RA: −220.50
[1]
mas/
yr Dec.: −45.31 [1] mas/ yr |
| Parallax (π) | 19.11 ± 0.37 mas [1] |
| Distance | 171 ± 3
ly (52 ± 1 pc) |
| Absolute magnitude (MV) | 2.26 [5] |
| Orbit [5] | |
| Period (P) | 7.7991499±0.0000037 d |
| Eccentricity (e) | 0.023±0.034 |
| Periastron epoch (T) | 20,165.164±1.470 HJD |
|
Argument of periastron (ω) (secondary) | 285.56±68.51° |
|
Semi-amplitude (K1) (primary) | 24.10±0.73 km/s |
| Details | |
| 38 LMi A | |
| Mass | 1.68 [6] M☉ |
| Luminosity | 11.32 [2] L☉ |
| Surface gravity (log g) | 3.73 [6] cgs |
| Temperature | 6,106 [7] K |
| Metallicity [Fe/H] | +0.32 [7] dex |
| Rotational velocity (v sin i) | 14.5±1.0 [5] km/s |
| Age | 2.03±0.14 [7] Gyr |
| 38 LMi B | |
| Mass | ≥ 0.31 [8] M☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
38 Leonis Minoris is a binary star [3] system in the northern constellation of Leo Minor. It shines with a combined light of apparent magnitude 5.84, [2] which indicates it a dimly visible to the naked eye under good viewing conditions. An annual parallax shift of 19.11 [1] mas provides a distance estimate of around 171 light years. It has a relatively high proper motion, traversing the celestial sphere at a rate of 0.226 arcseconds per year, [10] and is moving away from the Sun with a radial velocity of +31 km/s. [4]
This is a single-lined spectroscopic binary [3] with an orbital period of 7.8 days and a low eccentricity of 0.023 – nearly circular. [5] The visible component has a stellar classification of G0 IV, [3] matching a G-type subgiant star that is exhausting the hydrogen at its core and evolving into a giant. It is about two [7] billion years old with 1.68 [6] times the mass of the Sun and is spinning with a projected rotational velocity of 14.5 km/s. [5] The star has a higher than solar abundance of iron in its spectrum. [7] It is radiating 11 [2] times the Sun's luminosity from its photosphere at an effective temperature of 6,106 K. [7]
- ^ a b c d e f van Leeuwen, F. (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, S2CID 18759600.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c d Abt, Helmut A. (2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement, 180 (1): 117–18, Bibcode: 2009ApJS..180..117A, doi: 10.1088/0067-0049/180/1/117, S2CID 122811461.
- ^ a b de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv: 1208.3048, Bibcode: 2012A&A...546A..61D, doi: 10.1051/0004-6361/201219219, S2CID 59451347, A61.
- ^ a b c d e Willmarth, Daryl W.; et al. (August 2016), "Spectroscopic Orbits for 15 Late-type Stars" (PDF), The Astronomical Journal, 152 (2): 13, Bibcode: 2016AJ....152...46W, doi: 10.3847/0004-6256/152/2/46, S2CID 53648490, 46.
- ^ a b c Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy and Astrophysics, 530: A138, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID 56118016.
- ^ a b c d e f Pace, G. (March 2013), "Chromospheric activity as age indicator. An L-shaped chromospheric-activity versus age diagram", Astronomy & Astrophysics, 551: 4, arXiv: 1301.5651, Bibcode: 2013A&A...551L...8P, doi: 10.1051/0004-6361/201220364, S2CID 56420519, L8.
- ^ Tokovinin, A.; et al. (May 2006), "Tertiary companions to close spectroscopic binaries", Astronomy and Astrophysics, 450 (2): 681–69, arXiv: astro-ph/0601518, Bibcode: 2006A&A...450..681T, doi: 10.1051/0004-6361:20054427, S2CID 8899546.
- ^ "38 LMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-02-20.
- ^ Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal, 129 (3): 1483–1522, arXiv: astro-ph/0412070, Bibcode: 2005AJ....129.1483L, doi: 10.1086/427854, S2CID 2603568.