| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Crux |
| Right ascension | 12h 06m 52.89900s [1] |
| Declination | −64° 36′ 49.4244″ [1] |
| Apparent magnitude (V) | 4.14 [2] |
| Characteristics | |
| Spectral type | F2 V [3] |
| U−B color index | +0.00 [2] |
| B−V color index | +0.35 [2] |
| Astrometry | |
| Radial velocity (Rv) | +9.0 [4] km/s |
| Proper motion (μ) |
RA: +33.88
[1]
mas/
yr Dec.: −37.02 [1] mas/ yr |
| Parallax (π) | 50.62 ± 0.12 mas [1] |
| Distance | 64.4 ± 0.2
ly (19.76 ± 0.05 pc) |
| Absolute magnitude (MV) | 2.67 [5] |
| Details | |
| Radius | 1.3 [6] R☉ |
| Luminosity | 7 [7] L☉ |
| Surface gravity (log g) | 4.01 [3] cgs |
| Temperature | 6,964 [5] K |
| Metallicity [Fe/H] | −0.04 [3] dex |
| Rotational velocity (v sin i) | 46.1±2.3 [5] km/s |
| Age | 2.53 [8] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Eta Crucis (η Crucis) is a solitary [10] star in the southern constellation of Crux. It can be seen with the naked eye, having an apparent visual magnitude of 4.14m. [2] Based upon parallax measurements, [1] η Crucis is located 64 light-years from the Sun. The system made its closest approach about 1.6 million years ago when it achieved perihelion at a distance of roughly 26 light years. [11]
This is an F-type main sequence star with a stellar classification of F2 V. [3] It has 130% [6] of the Sun's radius and shines with 7 [7] times the luminosity of the Sun from an outer atmosphere with an effective temperature of 6,964 K. [5] Observations of the system using the Spitzer Space Telescope show a statistically significant infrared excess of emission at a wavelength of 70 μm. This suggests the presence of a circumstellar disk. The temperature of this material is below 70 K. [8]
Eta Crucis has a pair of visual companions. Component B is a magnitude 11.80 star located at an angular separation of 48.30 ″ along a position angle of 300°, as of 2010. Component C has a magnitude of 12.16 and lies at an angular separation of 35.50″ along a position angle of 194°, as of 2000. [12]
- ^ 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- ^ a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode: 1986EgUBV........0M.
- ^ a b c d Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv: astro-ph/0603770, Bibcode: 2006AJ....132..161G, doi: 10.1086/504637, S2CID 119476992.
- ^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Carnegie Institute of Washington, D.C., Bibcode: 1953GCRV..C......0W.
- ^ a b c d Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv: 1204.2459, Bibcode: 2012A&A...542A.116A, doi: 10.1051/0004-6361/201118724, S2CID 53666672.
- ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 521–524, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ a b 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.
-
^
"eta Cru".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2016-10-06.
{{ cite web}}: CS1 maint: postscript ( link) - ^ 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, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ Bailer-Jones, C. A. L. (March 2015), "Close encounters of the stellar kind", Astronomy & Astrophysics, 575: 13, arXiv: 1412.3648, Bibcode: 2015A&A...575A..35B, doi: 10.1051/0004-6361/201425221, S2CID 59039482, A35.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920.
- Kaler, James B., "Eta Crucis", Stars, University of Illinois, retrieved 2016-10-08.
| Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
|---|---|
| Constellation | Crux |
| Right ascension | 12h 06m 52.89900s [1] |
| Declination | −64° 36′ 49.4244″ [1] |
| Apparent magnitude (V) | 4.14 [2] |
| Characteristics | |
| Spectral type | F2 V [3] |
| U−B color index | +0.00 [2] |
| B−V color index | +0.35 [2] |
| Astrometry | |
| Radial velocity (Rv) | +9.0 [4] km/s |
| Proper motion (μ) |
RA: +33.88
[1]
mas/
yr Dec.: −37.02 [1] mas/ yr |
| Parallax (π) | 50.62 ± 0.12 mas [1] |
| Distance | 64.4 ± 0.2
ly (19.76 ± 0.05 pc) |
| Absolute magnitude (MV) | 2.67 [5] |
| Details | |
| Radius | 1.3 [6] R☉ |
| Luminosity | 7 [7] L☉ |
| Surface gravity (log g) | 4.01 [3] cgs |
| Temperature | 6,964 [5] K |
| Metallicity [Fe/H] | −0.04 [3] dex |
| Rotational velocity (v sin i) | 46.1±2.3 [5] km/s |
| Age | 2.53 [8] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Eta Crucis (η Crucis) is a solitary [10] star in the southern constellation of Crux. It can be seen with the naked eye, having an apparent visual magnitude of 4.14m. [2] Based upon parallax measurements, [1] η Crucis is located 64 light-years from the Sun. The system made its closest approach about 1.6 million years ago when it achieved perihelion at a distance of roughly 26 light years. [11]
This is an F-type main sequence star with a stellar classification of F2 V. [3] It has 130% [6] of the Sun's radius and shines with 7 [7] times the luminosity of the Sun from an outer atmosphere with an effective temperature of 6,964 K. [5] Observations of the system using the Spitzer Space Telescope show a statistically significant infrared excess of emission at a wavelength of 70 μm. This suggests the presence of a circumstellar disk. The temperature of this material is below 70 K. [8]
Eta Crucis has a pair of visual companions. Component B is a magnitude 11.80 star located at an angular separation of 48.30 ″ along a position angle of 300°, as of 2010. Component C has a magnitude of 12.16 and lies at an angular separation of 35.50″ along a position angle of 194°, as of 2000. [12]
- ^ 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 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode: 1986EgUBV........0M.
- ^ a b c d Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal, 132 (1): 161–170, arXiv: astro-ph/0603770, Bibcode: 2006AJ....132..161G, doi: 10.1086/504637, S2CID 119476992.
- ^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Carnegie Institute of Washington, D.C., Bibcode: 1953GCRV..C......0W.
- ^ a b c d Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv: 1204.2459, Bibcode: 2012A&A...542A.116A, doi: 10.1051/0004-6361/201118724, S2CID 53666672.
- ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 521–524, arXiv: astro-ph/0012289, Bibcode: 2001A&A...367..521P, doi: 10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ a b 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.
-
^
"eta Cru".
SIMBAD.
Centre de données astronomiques de Strasbourg. Retrieved 2016-10-06.
{{ cite web}}: CS1 maint: postscript ( link) - ^ 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, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ Bailer-Jones, C. A. L. (March 2015), "Close encounters of the stellar kind", Astronomy & Astrophysics, 575: 13, arXiv: 1412.3648, Bibcode: 2015A&A...575A..35B, doi: 10.1051/0004-6361/201425221, S2CID 59039482, A35.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920.
- Kaler, James B., "Eta Crucis", Stars, University of Illinois, retrieved 2016-10-08.