CS Camelopardalis

CS Camelopardalis (CS Cam; HD 21291) is a binary star in reflection nebula VdB 14, in the constellation Camelopardalis.

CS Camelopardalis
Location of CS Camelopardalis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis
A
Right ascension 03h 29m 04.13196s
Declination +59° 56 25.1970
Apparent magnitude (V) 4.22 (4.19 - 4.23)
B
Right ascension 03h 29m 04.22561s
Declination +59° 56 25.9860
Apparent magnitude (V) 7.75
Characteristics
A
Spectral type B9 Ia
U−B color index −0.23
B−V color index +0.41
Variable type α Cyg
B
Spectral type B2III
Astrometry
A
Radial velocity (Rv)−5.10 km/s
Proper motion (μ) RA: −2.751 mas/yr
Dec.: −1.066 mas/yr
Parallax (π)1.0527 ± 0.1311 mas
Distanceapprox. 3,100 ly
(approx. 900 pc)
Absolute magnitude (MV)−7.10
B
Proper motion (μ) RA: −1.702 mas/yr
Dec.: −0.646 mas/yr
Parallax (π)0.9642 ± 0.0601 mas
Distance3,400 ± 200 ly
(1,040 ± 60 pc)
Details
Mass19 M
Radius85.7 R
Luminosity75,900 L
Surface gravity (log g)1.65 cgs
Temperature10,800 K
Rotational velocity (v sin i)30 km/s
Age16.5 Myr
Other designations
ADS 2544, BD+59°660, CCDM 03291+5956, GC 4113, HD 21291, HIP 16228, HR 1035, SAO 24054, WDS J03291+5956
Database references
SIMBADdata
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

It forms a group of stars known as the Camelopardalis R1 association, part of the Cam OB1 association. The near-identical supergiant CE Camelopardalis is located half a degree to the south.

As a binary star, CS Cam is designated as Struve 385 (STF 385, Σ385).

The primary component, CS Camelopardalis A, is a blue-white B-type supergiant with a mean apparent magnitude of 4.21m. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude 4.19m to 4.23m. Its companion, CS Camelopardalis B, is a magnitude 8.7m blue giant star located 2.4 arcseconds from the primary.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.