T Cephei
T Cephei is a Mira variable star in the constellation Cepheus. Located approximately 570 ± 40 light-years (175 ± 12 parsecs) distant, it varies between magnitudes 5.2 and 11.3 over a period of around 388 days.[5][2]
![]() Region of NGC 7023, with T Cephei marked on the full-size image Credit: NASA, ESA and Digitized Sky Survey 2 | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cepheus |
Right ascension | 21h 09m 31.78089s[1] |
Declination | +68° 29′ 27.2038″[1] |
Apparent magnitude (V) | 5.2 - 11.3[2] |
Characteristics | |
Spectral type | M6-9e[3] |
U−B color index | +0.33[4] |
B−V color index | +1.49[4] |
Variable type | Mira[5] |
Astrometry | |
Radial velocity (Rv) | −8.03[6] km/s |
Proper motion (μ) | RA: −44.145[7] mas/yr Dec.: −42.308[7] mas/yr |
Parallax (π) | 5.6912 ± 0.4004[7] mas |
Distance | 570 ± 40 ly (180 ± 10 pc) |
Details | |
Mass | 0.55[8] M☉ |
Radius | 329+70 −50[9] R☉ |
Luminosity | 5,700[5] L☉ |
Temperature | 2,400[5] K |
Other designations | |
Database references | |
SIMBAD | data |
Stellar Properties
T Cephei is a red giant of spectral type M6-9e with an effective temperature 2,400 K, a radius of 329 R☉, a mass of 0.55 M☉, and a luminosity of 5,700 L☉. If it were in the place of the Sun, its photosphere would at least engulf the orbit of Mars. This star is believed to be in a late stage of its life, blowing off its own sooty atmosphere to form a white dwarf in a distant future.
gollark: This is a strong expression of my disapproval. Do you want me to marry you to egoism?
gollark: ++delete <@!341618941317349376> (literally self-proclaimed egoist)
gollark: Ah, THAT explains a lot.
gollark: I doubt it.
gollark: I mean, according to the moral standards they would have followed, yes. It's subjective.
See also
References
- 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.
- VSX (4 January 2010). "T Cep". AAVSO Website. American Association of Variable Star Observers. Retrieved 1 July 2014.
- Keenan, Philip C.; Garrison, Robert F.; Deutsch, Armin J. (1974). "Revised Catalog of Spectra of Mira Variables of Types ME and Se". Astrophysical Journal Supplement. 28: 271. Bibcode:1974ApJS...28..271K. doi:10.1086/190318.
- Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
- Danilovich, T.; Teyssier, D.; Justtanont, K.; Olofsson, H.; Cerrigone, L.; Bujarrabal, V.; Alcolea, J.; Cernicharo, J.; Castro-Carrizo, A.; García-Lario, P.; Marston, A. (2015). "New observations and models of circumstellar CO line emission of AGB stars in the Herschel SUCCESS programme". Astronomy & Astrophysics. 581: A60. arXiv:1506.09065. Bibcode:2015A&A...581A..60D. doi:10.1051/0004-6361/201526705.
- Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics. 430: 165. arXiv:astro-ph/0409579. Bibcode:2005A&A...430..165F. doi:10.1051/0004-6361:20041272.
- 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.
- . doi:10.1086/170836. Cite journal requires
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(help) - Weigelt, Gerd; Beckmann, Udo; Berger, Jean-Philippe; Bloecker, Thomas; Brewer, Michael K.; Hofmann, Karl-Heinz; Lacasse, Marc G.; Malanushenko, Victor; Millan-Gabet, Rafael; et al. (2003). "JHK-band spectro-interferometry of T Cep with the IOTA interferometer". Interferometry for Optical Astronomy II. Proc. SPIE. 4838. pp. 181–184. Bibcode:2003SPIE.4838..181W. doi:10.1117/12.458659.
External links
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