42 Cassiopeiae

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Template:Short description

42 Cassiopeiae
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) +5.18[1]
Characteristics
Evolutionary stage main sequence[3]
Spectral type B9 V[4]
B−V Template:Engvar Script error: No such module "val".[1]
Variable type suspected β Per[5]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[1] km/s
Proper motion (μ) RA: +76.295[2] mas/yr
Dec.: −14.091[2] mas/yr
Parallax (π)11.1166±0.0661 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.53[1]
Details
MassScript error: No such module "val".[3] Template:Solar mass
RadiusScript error: No such module "val".[6] Template:Solar radius
Luminosity66.12[1] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[6] cgs
TemperatureScript error: No such module "val".[6] K
Rotational velocity (v sin i)149[3] km/s
AgeScript error: No such module "val".[7] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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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 293 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +7 km/s.

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[1] times the luminosity of the Sun from its photosphere at an effective temperature of 10,141 K.[6]

References

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  2. a b c d e Template:Cite Gaia DR3
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Template:Stars of Cassiopeia