The Bayer-designated stars in Cassiopeia. Iota Cassiopeiae is circled. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Cassiopeia |
ι Cas A | |
Right ascension | 02 29 03.960 |
Declination | +67° 24′ 08.70″ |
Apparent magnitude (V) | 4.61 (4.65 / 8.48) |
ι Cas B | |
Right ascension | 02 29 03.567 |
Declination | +67° 24′ 07.01″ |
Apparent magnitude (V) | 6.87 |
ι Cas C | |
Right ascension | 02 29 05.086 |
Declination | +67° 24′ 05.53″ |
Apparent magnitude (V) | 9.05 (9.14 / 11.84) |
Characteristics | |
U−B color index | +0.03 |
B−V color index | +0.12 |
ι Cas A | |
Spectral type | A3p / G6 |
Variable type | α CVn |
ι Cas B | |
Spectral type | F5 |
ι Cas C | |
Spectral type | K4 / M2 |
U−B color index | +0.18 |
B−V color index | +0.72 |
Astrometry | |
Radial velocity (Rv) | 1.2 ± 2 km/s |
Proper motion (μ) | RA: -26.61 mas/yr Dec.: 38.21 mas/yr |
Parallax (π) | 22.22 ± 0.08 mas |
Distance | 146.8 ± 0.5 ly (45.0 ± 0.2 pc) |
Absolute magnitude (MV) | 1.62 ± 0.07 (Aa) 5.60 ± 0.17 (Ab) |
Orbit | |
Primary | ι Cas Aa |
Companion | ι Cas Ab |
Period (P) | 48.72 ± 0.45 yr |
Semi-major axis (a) | 0.423 ± 0.004″ |
Eccentricity (e) | 0.637 ± 0.004 |
Inclination (i) | 148.2 ± 1.3° |
Longitude of the node (Ω) | 176.6 ± 1.8° |
Periastron epoch (T) | B 1993.21 ± 0.05 |
Argument of periastron (ω) (secondary) | 328.2 ± 1.9° |
Orbit | |
Primary | ι Cas A |
Companion | ι Cas B |
Period (P) | 2400 yr |
Semi-major axis (a) | 6.50″ |
Eccentricity (e) | 0.40 |
Inclination (i) | 102.9 ± 0.3° |
Longitude of the node (Ω) | 188.0 ± 0.9° |
Periastron epoch (T) | B 940 ± 47 |
Argument of periastron (ω) (secondary) | 113.3 ± 3.4° |
Details | |
ι Cas Aa | |
Mass | 1.98 M☉ |
Radius | 2.3 ± 0.4 R☉ |
Luminosity | 24 L☉ |
Temperature | 8360 ± 275 K |
Rotation | 1.74033 d |
Rotational velocity (v sin i) | 48 km/s |
Age | 100 Myr |
ι Cas Ab | |
Mass | 0.98 M☉ |
ι Cas B | |
Mass | 1.28 M☉ |
Temperature | 6540 K |
ι Cas Ca | |
Temperature | 4520 ± 20 K |
ι Cas Cb | |
Temperature | 3590 ± 45 K |
Other designations | |
BD+66° 213, HD 15089, HIP 11569, HR 707, SAO 12298 | |
ι Cas A: TYC 4058-1504-1 | |
ι Cas B: TYC 4058-1504-2 | |
ι Cas C: TYC 4058-1505-1 | |
Database references | |
ι Cas AB | |
ι Cas A | |
ι Cas B | |
ι Cas C |
Iota Cassiopeiae (ι Cas, ι Cassiopeiae) is a star system in the constellation Cassiopeia. The system has a combined apparent magnitude of 4.53, making it visible to the naked eye. Based on its parallax, it is located about 133 light-years (41 parsecs) from Earth.
Components
Iota Cassiopeiae is known to be a quintuple star system. The brightest star system, ι Cassiopeiae A, contains a white-colored A-type main-sequence star with a mean apparent magnitude of +4.61. The primary is itself a tighter binary star system. The two stars were resolved by adaptive optics. These are designated Aa and Ab (although confusingly they may also be labeled as A and Aa, respectively). The primary is classified as an Alpha Canum Venaticorum-type variable star and the brightness of the system varies from magnitude +4.45 to +4.53 with a period of 1.74 days, because of its magnetic field. The variability in brightness was first detected by Karl D. Rakos in 1962, although its spectrum was known to be variable from earlier observations. The fainter companion is a G-type star with a mass of 0.98 M☉. The orbital period of the system is about 49 years.
ι Cassiopeiae B is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.87. It orbits around ι Cassiopeiae A approximately every 2,400 years with a semi-major axis of around 6.5 arcseconds, but the orbit is not very well constrained. This object may be causing Kozai–Lidov cycles in the inner orbital pair.
ι Cassiopeiae C is itself another binary, designated Ca and Cb, or just C and c. It comprises two stars, a K-type star and an M-type star. It is currently at an angular distance of about 7 arcseconds from the AB pair. Since the semimajor axis of the AB orbit is about 6.5 arcseconds, the true semimajor axis of C's orbit around them is thought to be significantly larger than 7 arcseconds.
References
- ^ Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27 – L30. Bibcode:2000A&A...355L..27H.
- ^ Drummond, Jack; Milster, Scott; Ryan, Patrick; Roberts, Jr., Lewis C. (2003). "ι Cassiopeiae: Orbit, Masses, and Photometry from Adaptive Optics Imaging in the I and H Bands". The Astrophysical Journal. 585 (2): 1007. Bibcode:2003ApJ...585.1007D. doi:10.1086/346224.
- ^ Christou, Julian C.; Drummond, Jack D. (2006). "Measurements of Binary Stars, Including Two New Discoveries, with the Lick Observatory Adaptive Optics System". The Astronomical Journal. 131 (6): 3100. Bibcode:2006AJ....131.3100C. doi:10.1086/503255.
- ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
- ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
- Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode:1953GCRV..C......0W.
- ^ van Leeuwen, F.; et al. (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.
- ^ Tokovinin, A. (2021). "Inner and Outer Orbits in 13 Resolved Hierarchical Stellar Systems". The Astronomical Journal. 161 (3): 144. arXiv:2101.02976. Bibcode:2021AJ....161..144T. doi:10.3847/1538-3881/abda42. S2CID 231419112.
- ^ De Rosa, R. J.; Patience, J.; Vigan, A.; Wilson, P. A.; Schneider, A.; McConnell, N. J.; Wiktorowicz, S. J.; Marois, C.; Song, I.; MacIntosh, B.; Graham, J. R.; Bessell, M. S.; Doyon, R.; Lai, O. (2012). "The Volume-limited A-Star (VAST) survey - II. Orbital motion monitoring of A-type star multiples". Monthly Notices of the Royal Astronomical Society. 422 (4): 2765. arXiv:1112.3666. Bibcode:2012MNRAS.422.2765D. doi:10.1111/j.1365-2966.2011.20397.x. S2CID 102487103.
- ^ Aurière, M.; Wade, G. A.; Silvester, J.; Lignières, F.; Bagnulo, S.; Bale, K.; Dintrans, B.; Donati, J. F.; Folsom, C. P.; Gruberbauer, M.; Hui Bon Hoa, A.; Jeffers, S.; Johnson, N.; Landstreet, J. D.; Lèbre, A.; Lueftinger, T.; Marsden, S.; Mouillet, D.; Naseri, S.; Paletou, F.; Petit, P.; Power, J.; Rincon, F.; Strasser, S.; Toqué, N. (2007). "Weak magnetic fields in Ap/Bp stars". Astronomy and Astrophysics. 475 (3): 1053. arXiv:0710.1554. Bibcode:2007A&A...475.1053A. doi:10.1051/0004-6361:20078189. S2CID 54850596.
- "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
- Rakos, Karl D. (1962). "Photoelectric investigation of magnetic and spectrum variable stars". Bulletin / Lowell Observatory. 5 (12): 227–256. Bibcode:1962LowOB...5..227R. Retrieved 10 October 2024.
- Tokovinin, A. A. (1997). "MSC - a catalogue of physical multiple stars". Astronomy and Astrophysics Supplement Series. 124: 75–84. Bibcode:1997A&AS..124...75T. doi:10.1051/aas:1997181. (HR 707 Archived 2021-02-05 at the Wayback Machine)
Constellation of Cassiopeia | |||||||||||||
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Category |
- Alpha2 Canum Venaticorum variables
- Bayer objects
- Cassiopeia (constellation)
- Multiple star systems
- Spectroscopic binaries
- A-type main-sequence stars
- F-type main-sequence stars
- G-type main-sequence stars
- Bright Star Catalogue objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Durchmusterung objects
- Ap stars