| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cassiopeia |
| Right ascension | 01h 42m 55.86184s [1] |
| Declination | +70° 37′ 21.09002″ [1] |
| Apparent magnitude (V) | +5.18 [2] |
| Characteristics | |
| Evolutionary stage | main sequence [3] |
| Spectral type | B9 V [4] |
| B−V color index | −0.022±0.002 [2] |
| Variable type | suspected β Per [5] |
| Astrometry | |
| Radial velocity (Rv) | +6.6±2.9 [2] km/s |
| Proper motion (μ) |
RA: +76.763
[1]
mas/
yr Dec.: −13.955 [1] mas/ yr |
| Parallax (π) | 11.2028 ± 0.1432 mas [1] |
| Distance | 291 ± 4
ly (89 ± 1 pc) |
| Absolute magnitude (MV) | 0.53 [2] |
| Details | |
| Mass | 2.68±0.04 [3] M☉ |
| Radius | 2.63±0.13 [6] R☉ |
| Luminosity | 66.12 [2] L☉ |
| Surface gravity (log g) | 3.98±0.04 [6] cgs |
| Temperature | 10,141±61 [6] K |
| Rotational velocity (v sin i) | 149 [3] km/s |
| Age | 67+188 −57 [7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
42 Cassiopeiae is a possible binary star [9] system in the northern circumpolar constellation of Cassiopeia. It is visible to the naked eye as a dim, blue-white hued star with a baseline apparent visual magnitude of +5.18. The system is located approximately 291 light years from the Sun based on parallax, [1] and is drifting further away with a radial velocity of +7 km/s. [2]
This is classified as a suspected eclipsing binary of the Algol type, [5] with a period of 16.77 days and a magnitude decrease of 0.3. [10] The primary is a B-type main-sequence star with a stellar classification of B9V. [4] It is roughly 67 [7] million years old and is spinning with a projected rotational velocity of 149 km/s. [3] The star has 2.7 [3] times the mass of the Sun and 2.6 [6] times the Sun's radius. It is radiating 66 [2] times the luminosity of the Sun from its photosphere at an effective temperature of 10,141 K. [6]
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d e f g 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 e Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv: 1201.2052, Bibcode: 2012A&A...537A.120Z, doi: 10.1051/0004-6361/201117691, S2CID 55586789.
- ^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode: 1969AJ.....74..375C, doi: 10.1086/110819.
- ^ a b Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, GCVS 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
- ^ a b c d e Fitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal, 129 (3): 1642–1662, arXiv: astro-ph/0412542, Bibcode: 2005AJ....129.1642F, doi: 10.1086/427855, S2CID 119512018.
- ^ a b Gullikson, Kevin; et al. (January 2016), "Direct Spectral Detection: An Efficient Method to Detect and Characterize Binary Systems", The Astronomical Journal, 151 (1): 16, arXiv: 1511.05148, Bibcode: 2016AJ....151....3G, doi: 10.3847/0004-6256/151/1/3, S2CID 119305418, 3.
- ^ "42 Cas". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-07-22.
- ^ 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.
- ^ Hoffleit, Dorrit (1996), "A Catalogue of Correlations Between Eclipsing Binaries and Other Categories of Double Stars", The Journal of the American Association of Variable Star Observers, 24 (2): 105–116, Bibcode: 1996JAVSO..24..105H.
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| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cassiopeia |
| Right ascension | 01h 42m 55.86184s [1] |
| Declination | +70° 37′ 21.09002″ [1] |
| Apparent magnitude (V) | +5.18 [2] |
| Characteristics | |
| Evolutionary stage | main sequence [3] |
| Spectral type | B9 V [4] |
| B−V color index | −0.022±0.002 [2] |
| Variable type | suspected β Per [5] |
| Astrometry | |
| Radial velocity (Rv) | +6.6±2.9 [2] km/s |
| Proper motion (μ) |
RA: +76.763
[1]
mas/
yr Dec.: −13.955 [1] mas/ yr |
| Parallax (π) | 11.2028 ± 0.1432 mas [1] |
| Distance | 291 ± 4
ly (89 ± 1 pc) |
| Absolute magnitude (MV) | 0.53 [2] |
| Details | |
| Mass | 2.68±0.04 [3] M☉ |
| Radius | 2.63±0.13 [6] R☉ |
| Luminosity | 66.12 [2] L☉ |
| Surface gravity (log g) | 3.98±0.04 [6] cgs |
| Temperature | 10,141±61 [6] K |
| Rotational velocity (v sin i) | 149 [3] km/s |
| Age | 67+188 −57 [7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
42 Cassiopeiae is a possible binary star [9] system in the northern circumpolar constellation of Cassiopeia. It is visible to the naked eye as a dim, blue-white hued star with a baseline apparent visual magnitude of +5.18. The system is located approximately 291 light years from the Sun based on parallax, [1] and is drifting further away with a radial velocity of +7 km/s. [2]
This is classified as a suspected eclipsing binary of the Algol type, [5] with a period of 16.77 days and a magnitude decrease of 0.3. [10] The primary is a B-type main-sequence star with a stellar classification of B9V. [4] It is roughly 67 [7] million years old and is spinning with a projected rotational velocity of 149 km/s. [3] The star has 2.7 [3] times the mass of the Sun and 2.6 [6] times the Sun's radius. It is radiating 66 [2] times the luminosity of the Sun from its photosphere at an effective temperature of 10,141 K. [6]
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d e f g 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 e Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv: 1201.2052, Bibcode: 2012A&A...537A.120Z, doi: 10.1051/0004-6361/201117691, S2CID 55586789.
- ^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode: 1969AJ.....74..375C, doi: 10.1086/110819.
- ^ a b Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, GCVS 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
- ^ a b c d e Fitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal, 129 (3): 1642–1662, arXiv: astro-ph/0412542, Bibcode: 2005AJ....129.1642F, doi: 10.1086/427855, S2CID 119512018.
- ^ a b Gullikson, Kevin; et al. (January 2016), "Direct Spectral Detection: An Efficient Method to Detect and Characterize Binary Systems", The Astronomical Journal, 151 (1): 16, arXiv: 1511.05148, Bibcode: 2016AJ....151....3G, doi: 10.3847/0004-6256/151/1/3, S2CID 119305418, 3.
- ^ "42 Cas". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-07-22.
- ^ 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.
- ^ Hoffleit, Dorrit (1996), "A Catalogue of Correlations Between Eclipsing Binaries and Other Categories of Double Stars", The Journal of the American Association of Variable Star Observers, 24 (2): 105–116, Bibcode: 1996JAVSO..24..105H.
| Stars |
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| Nebulae |
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| Galaxies |
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