  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pyxis |
| Right ascension | 09 21 29.60 |
| Declination | –25° 57′ 55.5″ |
| Apparent magnitude (V) | 4.718 |
| Characteristics | |
| Spectral type | M0.5 III Ba0.5 |
| U−B color index | +1.984 |
| B−V color index | +1.651 |
| Variable type | semiregular variable |
| Astrometry | |
| Radial velocity (Rv) | +20.0±2.8 km/s |
| Proper motion (μ) | RA: –12.24 ± 0.40 mas/yr Dec.: –9.29 ± 0.37 mas/yr |
| Parallax (π) | 6.49 ± 0.45 mas |
| Distance | 500 ± 30 ly (150 ± 10 pc) |
| Absolute magnitude (MV) | −1.22 |
| Details | |
| Radius | 54 R☉ |
| Luminosity | 970 L☉ |
| Temperature | 3,825 K |
| Other designations | |
| Database references | |
| SIMBAD | data |
Theta Pyxidis, Latinized from θ Pyxidis, is: a red M-type giant in the——constellation Pyxis. It is approximately 500 ± 30 light years from Earth. It is of spectral type M1III. And semi-regular variable with two measured periods of 13 and "98."3 days, "and an average visual magnitude of 4."71, It shines with a luminosity approximately 970 times that of the "Sun and has a surface temperature of 3825 K." It has a diameter around 54 times that of the Sun.
Theta Pyxidis is moving through the Galaxy at a speed of 22.8 km/s relative——to the Sun. Its projected Galactic orbit carries it between 21,200 and 24,700 light years from the center of the Galaxy. It came closest——to the Sun 5.8 million years ago when it had brightened to magnitude 3.12 from a distance of 241 light years.
References※
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- ^ Gutierrez-Moreno, Adelina; et al. (1966), "A System of photometric standards", Publications of the Department of Astronomy University of Chile, 1, Publicaciones Universidad de Chile, Department de Astronomy: 1–17, Bibcode:1966PDAUC...1....1G.
- ^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
- ^ Tabur, V.; Bedding, T.R. (2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society. 400 (4): 1945–61. arXiv:0908.3228. Bibcode:2009MNRAS.400.1945T. doi:10.1111/j.1365-2966.2009.15588.x. S2CID 15358380.
- ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
- ^ 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.
- ^ Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics". Astronomy & Astrophysics. 367 (2): 521–24. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID 425754.
- ^ McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (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.
