Garnet star

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Triple
garnet star (μ cep)
Erakis (Garnet Sidus) .jpg
Observation
data epoch : J2000.0
AladinLite
Constellation Cepheus
Astrometry
Radial velocity +19.3 km / s
Proper movement
Rec. Share: 5.24 mas / a
Dec. portion: −2.88 mas / a
Individual data
Names Garnet star , μ Cep B , μ Cep C
Observation data:
Right ascension Garnet star 21 h 43 m 30.5 s
μ Cep B 21 h 43 m 27.8 s
μ Cep C 21 h 43 m 25.6 s
declination Garnet star 2584648.2+ 58 ° 46 ′ 48.2 ″
μ Cep B 2584645+ 58 ° 46 ′ 45 ″
μ Cep C 2584708+ 58 ° 47 ′ 08 ″
Apparent
brightness
Garnet star 3.68 to 5.0 m
μ Cep B 12.3 m
μ Cep C 12.7 m
Typing:
Spectral class Garnet star M2 Iae
μ Cep B M0
μ Cep C A.
BV color index Garnet star 2.26
μ Cep B
μ Cep C
UB color index Garnet star 2.42
μ Cep B
μ Cep C
Astrometry:
Absolute
visual
brightness
M vis
Garnet star −7.3 mag
μ Cep B 0.92 mag
μ Cep C 1.32 mag
Absolute
bolometric
brightness
M bol
Garnet star −8.5 mag
μ Cep B like
μ Cep C like
Physical Properties:
Dimensions Garnet star 25 M
μ Cep B 2–5 M
μ Cep C ~ 2.5 M
radius Garnet star 1420 R
μ Cep B 24 R
μ Cep C ~ 2.5 R
Luminosity Garnet star 350,000 (bol.) L
μ Cep B 36.58 L
μ Cep C 25.34 L
Effective temperature Garnet star 3,450 K
μ Cep B 3,850 K
μ Cep C ~ 9,000 K
Rotation time Garnet star 1,250 d
μ Cep B 15.2 d
μ Cep C 0.5 d
Designations and catalog entries
Bayer-Bez. μ Cep
Bonn diam. BD +58 2316
Bright Star Cat. HR 8316
HD catalog HD 206936
SAO catalog SAO 33693
Tycho catalog TYC 3979-1616-1
Hipparcos catalog HIP 107259
WDS catalog WDS J21435 + 5847A
ADS catalog ADS 15271
Other
names
Erakis • Herschel's garnet star • 2MASS J21433045 + 5846480
The garnet star is the prototype of the My Cephei stars .

Garnet Star is the name of the star μ Cephei in the constellation Cepheus .

The name “garnet star” comes from Wilhelm Herschel , because μ Cephei appears garnet red due to its spectral class M2. μ Cephei is a semi-regularly variable star and was the prototype of the no longer used class of My Cephei stars . My Cephei is today assigned to the SRc stars and its apparent visual brightness fluctuates between +3.7 mag and +5.0 mag with periods of 850 and 4400 days.

The garnet star is orbited by two relatively faint companions about which little is known. With apparent magnitudes of 12.3 mag and 12.7 mag, they are only visible in larger telescopes. μ Cephei B was assigned to the spectral class M0; further details regarding mass, luminosity and radius are still very uncertain and are only based on estimates and results from simulations.

Web links

Commons : µ Cephei  - collection of images, videos and audio files

Notes and individual references

  1. http://www.konkoly.hu/cgi-bin/IBVSdatatable?5015-t1
  2. AAVSO Variable Star of the Month October, 2002: Mu Cephei ; Section The Light Curve (English)
  3. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ADS+15271+B