TZ Cassiopeiae
Observation data J2000
| |
---|---|
Constellation | Cassiopeia |
Right ascension | 23h 52m 56.23689s[1] |
Declination | 61° 00′ 08.3915″[1] |
Apparent magnitude (V) | 9.18[2] (+8.86 - +10.5[3]) |
Characteristics | |
Spectral type | M3 Iab[4] |
U−B color index | +2.43[2] |
B−V color index | +2.57[2] |
Variable type | Lc[3] |
Absolute magnitude (MV) | −5.98[6] |
Details | |
dex | |
AAVSO 2348+60 | |
Database references | |
SIMBAD | data |
TZ Cassiopeiae (TZ Cas, HIP 117763, SAO 20912) is a
TZ Cassiopeiae was reported as being variable by Williamina Fleming and published posthumously in 1911.[11] It is a slow irregular variable star with a possible period of 3,100 days.[12] It is over 90,000 times the luminosity of the Sun, and it is 767 times larger than the Sun. It is a member of the Cas OB5 stellar association, together with the nearby red supergiant PZ Cassiopeiae.[13]
The initial mass of TZ Cassiopeiae has been estimated from its position relative to theoretical stellar evolutionary tracks to be around 15 M☉.[14]
TZ Cas is losing mass through a powerful stellar wind at two millionths of a solar mass each year.[15] It is unclear whether this is sufficient to cause the star to lose its atmosphere and become a blue supergiant before the core exhausts its fuel and collapses as a supernova. Either as a red or blue supergiant, or a Wolf–Rayet star, it will inevitably end its life violently in a supernova explosion when the core collapse occurs.[16]
References
- ^ .
- ^ Bibcode:2002yCat.2237....0D.
- ^ Bibcode:2011JAVSO..39....1P.
- S2CID 123149047.
- S2CID 17804304.
- S2CID 15109583.
- ^ ISSN 0004-6361.
- S2CID 166227927.
- ^ S2CID 221340538.
- ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
- Bibcode:1911HarCi.167....1F.
- S2CID 5203133.
- doi:10.1086/190559.
- S2CID 17789027.
- S2CID 119276502.
- S2CID 38736311.