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Kruger 60 information


Krüger 60 A/B

A blue band light curve for a flare on DO Cephei, adapted from Dal (2020)[1]
Observation data
Epoch J2000      Equinox
Constellation Cepheus
Krüger 60 A
Right ascension 22h 27m 59.55755s[2]
Declination +57° 41′ 42.0806″[2]
Apparent magnitude (V) 9.59[citation needed]
Krüger 60 B
Right ascension 22h 27m 59.79560s[3]
Declination +57° 41′ 49.7468″[3]
Apparent magnitude (V) 11.40[citation needed]
Characteristics
Spectral type M3V/M4V[4]
U−B color index 1.27/1.3[citation needed]
B−V color index 1.65/1.8[citation needed]
Variable type None/Flare star
Astrometry
Krüger 60 A
Radial velocity (Rv)–33.1[citation needed] km/s
Proper motion (μ) RA: −725.227±0.537[2] mas/yr
Dec.: −223.461±0.348[2] mas/yr
Parallax (π)249.3926 ± 0.1653 mas[2]
Distance13.078 ± 0.009 ly
(4.010 ± 0.003 pc)
Absolute magnitude (MV)11.76
Krüger 60 B
Radial velocity (Rv)–31.9[citation needed] km/s
Proper motion (μ) RA: −934.098±1.319[3] mas/yr
Dec.: −686.244±1.410[3] mas/yr
Parallax (π)249.9668 ± 0.7414 mas[3]
Distance13.05 ± 0.04 ly
(4.00 ± 0.01 pc)
Absolute magnitude (MV)13.46
Details
Krüger 60 A
Mass0.271[5] M
Radius0.35[6] R
Luminosity0.010[citation needed] L
Temperature3,180[citation needed] K
Metallicity–0.04[7]
Krüger 60 B
Mass0.176[5] M
Radius0.24[6] R
Luminosity0.0034[citation needed] L
Temperature2,890[citation needed] K
Orbit[8]
PrimaryKrüger 60 A
CompanionKrüger 60 B
Period (P)44.67 yr
Semi-major axis (a)2.383″
Eccentricity (e)0.410
Inclination (i)167.2°
Longitude of the node (Ω)154.5°
Periastron epoch (T)1970.22
Argument of periastron (ω)
(primary)
211.0°
Other designations
BD+56° 2783, GJ 860 A/B, HD 239960, HIP 110893, ADS 15972, G 232-075, LHS 3814/3815[9]
Database references
SIMBADThe system
A
B
Krüger 60 is located in the constellation Cepheus.
Krüger 60 is located in the constellation Cepheus.
Krüger 60
Location of Krüger 60 in the constellation Cepheus

Krüger 60 (DO Cephei) is a binary star system located 13.1 light-years (4.0 parsecs) from the Sun. These red dwarf stars orbit each other every 44.6 years.

  1. ^ Cite error: The named reference Dal was invoked but never defined (see the help page).
  2. ^ a b c d e Cite error: The named reference GaiaDR2a was invoked but never defined (see the help page).
  3. ^ a b c d e Cite error: The named reference GaiaDR2b was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference apj108 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference aaa364 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference aaa367 was invoked but never defined (see the help page).
  7. ^ Bonfils, Xavier; Delfosse, Xavier; Udry, Stéphane; Santos, Nuno C.; Forveille, Thierry; Ségransan, Damien (2005). "Metallicity of M dwarfs. I. A photometric calibration and the impact on the mass-luminosity relation at the bottom of the main sequence". Astronomy and Astrophysics. 442 (2): 635–642. arXiv:astro-ph/0503260. Bibcode:2005A&A...442..635B. doi:10.1051/0004-6361:20053046. S2CID 13900901. Only listed for component A.
  8. ^ Cite error: The named reference aas65 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).

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