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GRW +70 8247 is a white dwarf star located 42 light-years from Earth[1] in the constellation Draco. With a magnitude of about 13 it is visible only through a large telescope.

Quick Facts Constellation, Right ascension ...
GRW +70 8247
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Draco
Right ascension 19h 00m 10.2534s[1]
Declination +70° 39 51.418[1]
Apparent magnitude (V) 13.19[2]
Characteristics
Spectral type DAP4.5[3]
U−B color index -0.85[4]
B−V color index +0.05[4]
Astrometry
Proper motion (μ) RA: +85.774[1] mas/yr
Dec.: +505.050[1] mas/yr
Parallax (π)77.6525 ± 0.0317 mas[1]
Distance42.00 ± 0.02 ly
(12.878 ± 0.005 pc)
Details[5]
Mass1.029 M
Radius5,960[a] km
Luminosity0.013182 L
Surface gravity (log g)8.67 cgs
Temperature12540±143 K
Age(as white dwarf) 1.138 Gyr
Other designations
GJ 742, AC +70 8247, G 260-15, LFT 1446, LHS 3424, LTT 15585, Grw+70 8247, WD 1900+705[2][6]
Database references
SIMBADdata
ARICNSdata
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Properties

Although photographed in the 19th century as part of the Carte du Ciel project, the star was not determined to be a white dwarf until G. P. Kuiper observed it in 1934.[7] This makes it the fifth or sixth white dwarf discovered.[b] At first, its spectrum was thought to be almost featureless,[7] but later observation showed it to have unusual broad, shallow absorption bands.[11][12] In 1970, when light that it emitted was observed to be circularly polarized, it became the first white dwarf known to have a magnetic field.[13][14] In the 1980s, it was realized that the unusual absorption bands could be explained as hydrogen absorption lines shifted by the Zeeman effect.[6][15][16]

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Notes

  1. Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772 K:
    .
  2. The star EGGR 37 was suspected to be a white dwarf by April 1934,[8] but this was not confirmed until 1938.[9][10]
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References

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