53 Camelopardalis

53 Camelopardalis

A light curve for AX Camelopardalis, plotted from TESS data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Camelopardalis
Right ascension 08h 01m 42.43137s[2]
Declination +60° 19′ 27.8016″[2]
Apparent magnitude (V) 6.02[3] (6.3 + 7.5)[4]
Characteristics
Evolutionary stage main sequence
Spectral type A3VpSrSiCrEu[5]
B−V color index 0.158±0.005[3]
Variable type α2 CVn[6]
Astrometry
Radial velocity (Rv)−2.2[3] km/s
Proper motion (μ) RA: −21.367[2] mas/yr
Dec.: −26.386[2] mas/yr
Parallax (π)11.2327 ± 0.1547 mas[2]
Distance290 ± 4 ly
(89 ± 1 pc)
Absolute magnitude (MV)1.05[3]
Orbit[7]
Period (P)2,422.04±2.42 d
Eccentricity (e)0.718±0.012
Periastron epoch (T)2,427,723.6±14.3 JD
Argument of periastron (ω)
(secondary)		5.22±1.64°
Semi-amplitude (K1)
(primary)		12.08±0.45 km/s
Details[7]
53 Cam A
Mass2.074±0.012 M☉
Radius2.36±0.10 R☉
Luminosity24.9±1.15 L☉
Surface gravity (log g)3.70±0.10 cgs
Temperature8,400±150 K
Rotation8.02681±0.00004 d
Rotational velocity (v sin i)12.5±0.5 km/s
Age615+56
−51 Myr
Other designations
53 Cam, AX Cam, BD+60°1105, FK5 302, GC 10822, HD 65339, HIP 39261, HR 3109, SAO 14402, CCDM 08017+6019, WDS J08017+6019[8]
Database references
SIMBADdata

53 Camelopardalis is a binary star system in the northern circumpolar constellation of Camelopardalis,[8] located 290 light years away from the Sun as determined by parallax measurements.[2] It has the variable star designation AX Camelopardalis; 53 Camelopardalis is the Flamsteed designation.[8] This object is dimly visible to the naked eye as a white hued star with a baseline apparent visual magnitude of +6.02.[3] It is a single-lined spectroscopic binary[9] system with an orbital period of 6.63 years and a high eccentricity of 0.718.[7] The "a sin i" value of the primary is 280 Gm (1.9 AU), where a is the semimajor axis and i is the orbital inclination.[7]

The visible component is a well-studied magnetic Ap star[7] with a stellar classification of A3VpSrSiCrEu[5] and a visual magnitude of 6.3.[4] The magnetic field topology of 53 Camelopardalis is complex, and is accompanied by abundance variations across the surface of elements like silicon, calcium, titanium, iron, and neodymium.[7] It is classified as an Alpha2 Canum Venaticorum type variable star and the combined brightness of the system varies from magnitude +6.00 down to +6.05 with a rotationally-modulated period of 8.0278 days.[6]

The primary has 2.1 times the mass of the Sun and 2.4 times the Sun's radius. It is spinning with a projected rotational velocity of 12.5 km/s and a rotation period of 8.0268 days. The inclination angle of the pole is estimated to be 57°±5°. The star is about 615 million years old and is radiating 25 times the luminosity of the Sun from its photosphere at an effective temperature of 8,400 K.[7]

  1. ^ Cite error: The named reference MAST was invoked but never defined (see the help page).
  2. ^ a b c d e f Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  3. ^ a b c d e Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference Malkov2012 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference abt1995 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference Samus2017 was invoked but never defined (see the help page).
  7. ^ a b c d e f g Cite error: The named reference Carrier2002 was invoked but never defined (see the help page).
  8. ^ a b c Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Kochukhov2004 was invoked but never defined (see the help page).