HR 8323
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
Constellation |
Grus |
Right ascension |
21h 48m 15.7514s[1] |
Declination |
−47° 18′ 13.014″[1] |
Apparent magnitude (V) | 5.58[1] |
Characteristics |
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Spectral type | G2V[1] |
U−B color index | +0.08[2] |
B−V color index | +0.60[2] |
Astrometry |
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Radial velocity (Rv) | −7.6 ± 0.2[1] km/s |
Proper motion (μ) | RA: 165.64[1] mas/yr Dec.: −295.00[1] mas/yr |
Parallax (π) | 63.95 ± 0.78[1] mas |
Distance | 51.0 ± 0.6 ly (15.6 ± 0.2 pc) |
Absolute magnitude (MV) | 4.61[3] |
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Details |
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Mass | 0.97 (0.92 to 1.04)[4] M☉ |
Radius | 1.0[5] R☉ |
Temperature | 5900[4] K |
Metallicity [Fe/H] | −0.15[4] dex |
Rotational velocity (v sin i) | 2[4] km/s |
Age | 3.8 (1.3 to 7.4)[4] Gyr |
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Other designations |
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CCDM J21483-4718A, CD−47 13928, CPD−47 9758, FK5 1573, GC 30516, Gliese 838, GJ 838, HD 207129, HIP 107649, IDS 21418-4746 A, LTT 8704, NLTT 52100, PPM 327579, SAO 230846, WDS J21483-4718A. [1] |
Database references |
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SIMBAD | data |
HR 8323 is a G-type pre-main-sequence star in the constellation of Grus.[1] It has an apparent visual magnitude of approximately 5.58.[1] This is a Sun-like star with the same stellar classification G2V and a similar mass. It is roughly the same age as the Sun, but has a lower abundance of elements other than hydrogen and helium; what astronomers term the star's metallicity.[4]
A debris disk has been imaged around this star in visible light using the ACS instrument on the Hubble Space Telescope; it has also been imaged in the infrared (70 μm) using the MIPS instrument on the Spitzer Space Telescope. Based on the ACS image, the disk appears to have a radius of about 163 astronomical units and to be about 30 AU wide, and to be inclined at 60° to the plane of the sky.[6]
Another star, CCDM J21483-4718B (also designated CD−47 13929 or WDS J21483-4718B), of apparent visual magnitude 8.7, has been observed 55 arcseconds away from this star,[7] but based on comparison of proper motions, it is believed to be an optical double and not physically related to its companion.[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 1.10 HD 207129 -- Pre-main sequence Star, database entry, SIMBAD. Accessed on line February 9, 2011.
- ↑ 2.0 2.1 HR 8323, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line February 9, 2011.
- ↑ From apparent magnitude and parallax.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 HD 207129, database entry, The Geneva-Copenhagen Survey of Solar neighbourhood, J. Holmberg et al., 2007, CDS ID V/117A. Accessed on line February 9, 2011.
- ↑ HD 207129, database entry, Catalog of Apparent Diameters and Absolute Radii of Stars (CADARS), 3rd edition, L. E. Pasinetti-Fracassini, L. Pastori, S. Covino, and A. Pozzi, CDS ID II/224. Accessed on line February 9, 2011.
- ↑ HST and Spitzer Observations of the HD 207129 Debris Ring, John E. Krist et al., The Astronomical Journal 140, #4 (October 2010), pp. 1051-1061, doi:10.1088/0004-6256/140/4/1051, Bibcode: 2010AJ....140.1051K.
- ↑ CCDM J21483-4718, database entry, CCDM (Catalog of Components of Double & Multiple stars), J. Dommanget and O. Nys, second edition, 2002, VizieR database I/274.
- ↑ Notes, WDS 21483-4718, The Washington Double Star Catalog, B. D. Mason et al., version 2011-02-06, VizieR database B/wds.
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| Bayer | |
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| Variable |
- U
- W
- RS
- RZ
- BC
- BP
- BZ
- CE
- DL
- DQ
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| HR |
- 8236
- 8241
- 8299
- 8323
- 8366
- 8379
- 8440
- 8477
- 8484
- 8501
- 8635
- 8639
- 8657
- 8658
- 8659
- 8685
- 8713
- 8749
- 8760
- 8771
- 8791
- 8793
- 8814
- 8835
- 8846
- 8847
- 8877
- 8896
- 8898
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| HD | |
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| Gliese | |
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| Other | |
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← Star systems within 50–55 light-years → |
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| | |
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- Castor (51.6 ± 1.0 ly; 6 stars)
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- 51 Pegasi (50.1 ± 0.6 ly; 1 star, 1 planet: b «Bellerophon»)
- GJ 3233 (50.2+6.0
−4.9 ly; 1 star)
- Gliese 758 (50.5 ± 0.5 ly; 1 star, 1 brown dwarf: B)
- HD 38858 (50.8 ± 0.9 ly; 1 star, 1 planet: b)
- HR 8323 (51.0 ± 0.6 ly; 1 star)
- 104 Tauri (51.8 ± 0.8 ly; 2 stars)
- Gliese 777 (51.8 ± 0.5 ly; 3 stars, 2 planets: c
- b)
- GJ 3781 (52.3 ± 1.2 ly; 2 stars)
- HR 3138 (52.8 ± 0.4 ly; 3 stars)
- 9 Puppis (53.4 ± 0.8 ly; 2 stars)
- Psi⁵ Aurigae (53.9 ± 0.6 ly; 1 star)
- HD 53705/53706/53680 (53.9 ± 0.9 ly; 4 stars)
- HR 5273 (54.1 ± 0.7 ly; 2 stars)
- HR 2225 (54.5 ± 0.7 ly; 1 star)
- 39 Tauri (54.6 ± 0.8 ly; 2 stars)
- Gliese 295 (54.8 ± 0.7 ly; 1 star)
- HR 2721 (55.0 ± 0.6 ly; 1 star)
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- HR 159 (50.2 ± 0.8 ly; 2 stars)
- Gliese 156 (50.3 ± 0.9 ly; 1 star)
- Gliese 862 (50.4 ± 0.8 ly; 1 star)
- Gliese 227 (50.4 ± 0.7 ly; 1 star)
- HD 135599 (50.8 ± 0.8 ly; 1 star)
- Gliese 778 (50.8 ± 0.7 ly; 1 star)
- GJ 1175 (50.9 ± 0.6 ly; 1 star)
- Gliese 782 (51.1 ± 1.2 ly; 1 star)
- Gliese 397 (51.1 ± 1.0 ly; 1 star)
- HD 113538 (51.2 ± 1.1 ly; 1 star, 2 planets: b
- c)
- HD 139763 (51.3 ± 1.1 ly; 1 star)
- Gliese 157 (51.4 ± 1.7 ly; 3 stars)
- Gliese 619 (51.9 ± 0.7 ly; 1 star)
- Gliese 112.1 (51.9 ± 1.3 ly; 1 star)
- Gliese 156.2 (52.1 ± 0.7 ly; 1 star)
- Gliese 462 (52.2 ± 1.1 ly; 1 star)
- Gliese 3 (52.2 ± 0.7 ly; 1 star)
- Gliese 32 (52.3 ± 1.4 ly; 2 stars)
- Gliese 472 (52.8 ± 0.5 ly; 1 star)
- Gliese 824 (52.8 ± 0.9 ly; 1 star)
- Gliese 152 (52.9 ± 0.6 ly; 1 star)
- Gliese 143 (53.4 ± 1.3 ly; 1 star)
- GJ 1177 (53.4 ± 2.7 ly; 2 stars)
- Gliese 826.1 (53.4 ± 1.2 ly; 1 star)
- Gliese 247 (53.5 ± 1.2 ly; 1 star)
- BY Draconis (53.6 ± 0.6 ly; 1 star)
- Gliese 531 (53.6 ± 0.8 ly; 1 star)
- Gliese 322 (53.8 ± 1.3 ly; 1 star)
- Gliese 553 (53.9 ± 1.4 ly; 1 star)
- HD 128311 (54.0 ± 0.9 ly; 1 star, 2 planets: b
- c)
- Gliese 795 (54.5 ± 2.0 ly; 2 stars)
- A 2329 (54.6 ± 1.1 ly; 2 stars)
- GJ 1181 (54.8 ± 2.5 ly; 2 stars)
- Gliese 786 (54.8 ± 0.7 ly; 1 star)
- HD 7924 (54.9 ± 0.5 ly; 1 star, 1 planet: b)
- Gliese 895.4 (55.0 ± 0.6 ly; 1 star)
- Gliese 200 (55.0 ± 1.6 ly; 2 stars)
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- GJ 3685/3686 (50.7+11.8
−8.0 ly; 2 stars)
- GJ 1062 (52.3 ± 2.9 ly; 1 star)
- HD 179930 (52.5 ± 1.7 ly; 2 stars)
- GJ 1264 (52.6 ± 2.1 ly; 1 star)
- Gliese 676 (53.7 ± 1.5 ly; 2 stars, 4 planets: Ad
- Ae
- Ab
- Ac)
- GJ 1049 (53.9 ± 1.2 ly; 1 star)
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T |
- WISE 0614+3912 (~50.2 ly; 1 brown dwarf)
- WISE 1617+1807 (~50.2 ly; 1 brown dwarf)
- WISE 1627+3255 (~50.2 ly; 1 brown dwarf)
- WISE 0542-1628 (~50.6 ly; 1 brown dwarf)
- WISE 1124-0421 (~50.6 ly; 1 brown dwarf)
- WISE 2015+6646 (~50.6 ly; 1 brown dwarf)
- WISE 1519+7009 (~50.9 ly; 1 brown dwarf)
- WISE 0325-3854 (~51.2 ly; 1 brown dwarf)
- WISE 2342+0856 (~51.2 ly; 1 brown dwarf)
- WISE 0614+0951 (~51.5 ly; 1 brown dwarf)
- WISE 0750+2725 (~51.5 ly; 1 brown dwarf)
- WISE 0906+4735 (~51.5 ly; 1 brown dwarf)
- WISE 1906+4508 (~51.5 ly; 1 brown dwarf)
- WISE 1457+5815 (~52.2 ly; 1 brown dwarf)
- WISE 2319-1844 (~52.2 ly; 1 brown dwarf)
- WISE 1622-0959 (52.2 ± 6.5 ly; 1 brown dwarf)
- WISE 1042-3842 (~53.2 ly; 1 brown dwarf)
- WISE 2237-0614 (~53.5 ly; 1 brown dwarf)
- WISE 0241-3653 (~53.8 ly; 1 brown dwarf)
- WISE 0656+4205 (~54.1 ly; 1 brown dwarf)
- WISE 2348-1028 (~54.1 ly; 1 brown dwarf)
- WISE 1804+3117 (54.4+12.2
−8.4 ly; 1 brown dwarf)
- WISE 0148+7202 (54.4+19.8
−11.4 ly; 1 brown dwarf)
- WISE 0333-5856 (~54.8 ly; 1 brown dwarf)
- WISE 2357+1227 (~54.8 ly; 1 brown dwarf)
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In left column are stellar classes of primary members of star systems. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems without known trigonometric parallax. |
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