TZ Arietis is the variable star designation for a red dwarf star in the northern constellation of Aries. With an apparent visual magnitude of 12.298[2] is too faint to be seen by the naked eye, although it lies relatively close to our Sun at a distance of about 14.7 light-years (4.5 parsecs).[5] It is a flare star, which means it can suddenly increase in brightness for short periods of time.
See also [edit]
References [edit]
- ^ a b c d Zacharias, N. et al. (2003), "The Second U.S. Naval Observatory CCD Astrograph Catalog (UCAC2)", CDS/ADC Collection of Electronic Catalogues volume=1289, Bibcode:2003yCat.1289....0Z.
- ^ a b Landolt, Arlo U. (July 1992), "UBVRI photometric standard stars in the magnitude range 11.5-16.0 around the celestial equator", Astronomical Journal 104 (1): 340–371, 436–491, Bibcode:1992AJ....104..340L, doi:10.1086/116242.
- ^ Riaz, Basmah; Gizis, John E.; Harvin, James (August 2006), "Identification of New M Dwarfs in the Solar Neighborhood", The Astronomical Journal 132 (2): 866–872, arXiv:astro-ph/0606617, Bibcode:2006AJ....132..866R, doi:10.1086/505632.
- ^ a b Nicolet, B. (1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System", Astronomy and Astrophysics Supplement Series 34: 1–49, Bibcode:1978A&AS...34....1N.
- ^ a b Harrington, R. S.; Dahn, C. C. (April 1980), "Summary of U.S. Naval Observatory parallaxes", Astronomical Journal 85: 454–465, Bibcode:1980AJ.....85..454H, doi:10.1086/112696.
- ^ a b McLean, M.; Berger, E.; Reiners, A. (February 2012), "The Radio Activity-Rotation Relation of Ultracool Dwarfs", The Astrophysical Journal 746 (1): 23, arXiv:1108.0415, Bibcode:2012ApJ...746...23M, doi:10.1088/0004-637X/746/1/23.
- ^ "TZ Ari -- Flare Star", SIMBAD Astronomical Database (Centre de Données astronomiques de Strasbourg), retrieved 2012-08-18.
External links [edit]
|
|
|
|
|
|
|
|
|
|
|
|
|
|
- Sirius (8.60 ± 0.04 ly; 2 stars)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
- Altair (16.73 ± 0.05 ly; 1 star)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
- Vega (25.04 ± 0.07 ly; 1 star)
- Fomalhaut (25.13 ± 0.09 ly; 1 star, 1 planet: b)
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
In left column are stellar classes of primary members of star systems. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems without known trigonometric parallax.
|
|