| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Phoenix |
| Right ascension | 00h 45m 45.5930s [1] |
| Declination | –47° 33′ 07.1438″ [1] |
| Apparent magnitude (V) | 5.80 [2] |
| Characteristics | |
| Spectral type | G3V [3] |
| B−V color index | +0.64 [2] |
| Astrometry | |
| Radial velocity (Rv) | –11.4 [4] km/s |
| Proper motion (μ) |
RA: 183.99
[1]
mas/
yr Dec.: 78.81 [1] mas/ yr |
| Parallax (π) | 65.97 ± 0.39 mas [1] |
| Distance | 49.4 ± 0.3
ly (15.16 ± 0.09 pc) |
| Details | |
| Mass | 1.22 ± 0.04 [5] M☉ |
| Surface gravity (log g) | 4.85 [5] cgs |
| Temperature | 5,955 [5] K |
| Metallicity [Fe/H] | 0.01 [5] dex |
| Rotation | 12 days [6] |
| Rotational velocity (v sin i) | 3.5 [3] km/s |
| Age | 1.2 [6] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 4391 is a triple star system [8] in the constellation Phoenix that is located at a distance of 48.7 light years from the Sun. The primary has a stellar classification of G3V, which is a G-type main sequence star. The physical properties of this star are similar to the Sun, making it a solar analog. However, it is believed to have 22% greater mass than the Sun and is only 1.2 billion years old. [5] The spectrum for this star displays an abnormally low level of beryllium, which may be the result of some form of mixing process. [6]
No planet has been detected in orbit around this star, [5] nor does it emit a statistically significant excess of infrared radiation that might indicate a debris disk. [9] However, it has two companions that share a common proper motion through space with HD 4391, effectively making it a triple star system. The first, a red dwarf of type M4, lies at an angular separation of 17″ from the primary. The second is a type M5 star at a separation of 49″. [8]
- ^ a b c d e van Leeuwen, F. (November 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 Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode: 1966CoLPL...4...99J.
- ^ a b Torres, C. A. O.; et al. (December 2006). "Search for associations containing young stars (SACY). I. Sample and searching method". Astronomy and Astrophysics. 460 (3): 695–708. arXiv: astro-ph/0609258. Bibcode: 2006A&A...460..695T. doi: 10.1051/0004-6361:20065602. S2CID 16080025.
- ^ Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Alan Henry Batten; John Frederick Heard (eds.). Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto: Academic Press, London. p. 57. Bibcode: 1967IAUS...30...57E.
- ^ a b c d e f Santos, N. C.; et al. (July 2001). "The metal-rich nature of stars with planets". Astronomy and Astrophysics. 373 (3): 1019–1031. arXiv: astro-ph/0105216. Bibcode: 2001A&A...373.1019S. doi: 10.1051/0004-6361:20010648. S2CID 119347084.
- ^ a b c Santos, N. C.; et al. (October 2004). "Beryllium anomalies in solar-type field stars". Astronomy and Astrophysics. 425 (3): 1013–1027. arXiv: astro-ph/0408109. Bibcode: 2004A&A...425.1013S. doi: 10.1051/0004-6361:20040510. S2CID 17279966.
- ^ "HD 4391 -- Pre-main sequence Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-07-13.
- ^ a b Raghavan, Deepak; et al. (September 2010). "A Survey of Stellar Families: Multiplicity of Solar-type Stars". The Astrophysical Journal Supplement. 190 (1): 1–42. arXiv: 1007.0414. Bibcode: 2010ApJS..190....1R. doi: 10.1088/0067-0049/190/1/1. S2CID 368553.
- ^ Beichman, C. A.; et al. (December 2006). "New Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets". The Astrophysical Journal. 652 (2): 1674–1693. arXiv: astro-ph/0611682. Bibcode: 2006ApJ...652.1674B. doi: 10.1086/508449. S2CID 14207148.
| Stars |
| ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||
| Galaxies |
| ||||||||||
| |||||||||||
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Phoenix |
| Right ascension | 00h 45m 45.5930s [1] |
| Declination | –47° 33′ 07.1438″ [1] |
| Apparent magnitude (V) | 5.80 [2] |
| Characteristics | |
| Spectral type | G3V [3] |
| B−V color index | +0.64 [2] |
| Astrometry | |
| Radial velocity (Rv) | –11.4 [4] km/s |
| Proper motion (μ) |
RA: 183.99
[1]
mas/
yr Dec.: 78.81 [1] mas/ yr |
| Parallax (π) | 65.97 ± 0.39 mas [1] |
| Distance | 49.4 ± 0.3
ly (15.16 ± 0.09 pc) |
| Details | |
| Mass | 1.22 ± 0.04 [5] M☉ |
| Surface gravity (log g) | 4.85 [5] cgs |
| Temperature | 5,955 [5] K |
| Metallicity [Fe/H] | 0.01 [5] dex |
| Rotation | 12 days [6] |
| Rotational velocity (v sin i) | 3.5 [3] km/s |
| Age | 1.2 [6] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 4391 is a triple star system [8] in the constellation Phoenix that is located at a distance of 48.7 light years from the Sun. The primary has a stellar classification of G3V, which is a G-type main sequence star. The physical properties of this star are similar to the Sun, making it a solar analog. However, it is believed to have 22% greater mass than the Sun and is only 1.2 billion years old. [5] The spectrum for this star displays an abnormally low level of beryllium, which may be the result of some form of mixing process. [6]
No planet has been detected in orbit around this star, [5] nor does it emit a statistically significant excess of infrared radiation that might indicate a debris disk. [9] However, it has two companions that share a common proper motion through space with HD 4391, effectively making it a triple star system. The first, a red dwarf of type M4, lies at an angular separation of 17″ from the primary. The second is a type M5 star at a separation of 49″. [8]
- ^ a b c d e van Leeuwen, F. (November 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 Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode: 1966CoLPL...4...99J.
- ^ a b Torres, C. A. O.; et al. (December 2006). "Search for associations containing young stars (SACY). I. Sample and searching method". Astronomy and Astrophysics. 460 (3): 695–708. arXiv: astro-ph/0609258. Bibcode: 2006A&A...460..695T. doi: 10.1051/0004-6361:20065602. S2CID 16080025.
- ^ Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Alan Henry Batten; John Frederick Heard (eds.). Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto: Academic Press, London. p. 57. Bibcode: 1967IAUS...30...57E.
- ^ a b c d e f Santos, N. C.; et al. (July 2001). "The metal-rich nature of stars with planets". Astronomy and Astrophysics. 373 (3): 1019–1031. arXiv: astro-ph/0105216. Bibcode: 2001A&A...373.1019S. doi: 10.1051/0004-6361:20010648. S2CID 119347084.
- ^ a b c Santos, N. C.; et al. (October 2004). "Beryllium anomalies in solar-type field stars". Astronomy and Astrophysics. 425 (3): 1013–1027. arXiv: astro-ph/0408109. Bibcode: 2004A&A...425.1013S. doi: 10.1051/0004-6361:20040510. S2CID 17279966.
- ^ "HD 4391 -- Pre-main sequence Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-07-13.
- ^ a b Raghavan, Deepak; et al. (September 2010). "A Survey of Stellar Families: Multiplicity of Solar-type Stars". The Astrophysical Journal Supplement. 190 (1): 1–42. arXiv: 1007.0414. Bibcode: 2010ApJS..190....1R. doi: 10.1088/0067-0049/190/1/1. S2CID 368553.
- ^ Beichman, C. A.; et al. (December 2006). "New Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets". The Astrophysical Journal. 652 (2): 1674–1693. arXiv: astro-ph/0611682. Bibcode: 2006ApJ...652.1674B. doi: 10.1086/508449. S2CID 14207148.
| Stars |
| ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||
| Galaxies |
| ||||||||||
| |||||||||||