G 99-47

G 99-47 (V1201 Orionis) is a nearby degenerate star (white dwarf) of spectral class DAP8 (DAP8.9, or DAP8.7), the single known component of the system, located in the constellation Orion. G 99-47 is probably the tenth closest white dwarf, followed by Gliese 293, Gliese 518 and Gliese 915.

G 99-47

A visual band light curve for V1201 Orionis, adapted from Brinkworth et al. (2013)
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 56m 25.47s
Declination +05° 21 48.6
Apparent magnitude (V) 14.105
Characteristics
Spectral type DAP8.9
Apparent magnitude (B) 14.69
Apparent magnitude (V) 14.10
Apparent magnitude (R) 14.0
Apparent magnitude (I) 13.6
Apparent magnitude (J) 12.930 ± 0.022
Apparent magnitude (H) 12.720 ± 0.025
Apparent magnitude (K) 12.653 ± 0.024
Astrometry
Proper motion (μ) RA: -444.685 mas/yr
Dec.: -925.140 mas/yr
Parallax (π)123.1989 ± 0.0170 mas
Distance26.474 ± 0.004 ly
(8.117 ± 0.001 pc)
Absolute magnitude (MV)14.59
Details
Mass0.71 ± 0.03 M
Radius0.011 R
Surface gravity (log g)8.20 ± 0.05 cgs
Temperature5790 ± 110 K
Age3.97 Gyr
Other designations
WD 0553+053, V1201 Ori, LHS 212, LTT 17891, NLTT 15834, G 099-047, GJ 1087, G 102-40, G 106-15, EGGR 290, 2MASS J05562547+0521486, USNO-B1.0 0953-00073703, Gaia DR2 3320184202856027776
Database references
SIMBADdata

The mass of G 99-47 is 0.71±0.03 Solar masses; its surface gravity is 108.20 ± 0.05 (1.58 · 108) cm·s−2, or approximately 162 000 of Earth's, corresponding to a radius 7711 km, or 121% of Earth's. Its temperature is 5790 ± 110 K, almost like the Sun's; its cooling age, i. e. age as degenerate star (not including lifetime as main sequence star and as giant star) is 3.97 Gyr. Due almost equal to the Sun's temperature, GJ 1087 should appear almost the same white color as the Sun. The white dwarf has a strong magnetic field, with measured vertical component near surface equal to 560 T.

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