Contents

G 240-72

Star in the constellation Draco

G 240-72

Observation data Epoch J2000[1]      Equinox J2000[1]
Constellation	Draco
Right ascension	17h48m 08.17s[1]
Declination	+70° 52′ 35.3″[1]
Apparent magnitude (V)	14.15[2]
Characteristics
Spectral type	DQP9.0[2]
Apparent magnitude (B)	14.55[1]
Apparent magnitude (V)	14.15[1]
Apparent magnitude (R)	13.5[1]
Apparent magnitude (I)	13.1[1]
Apparent magnitude (J)	12.709 ± 0.021[1]
Apparent magnitude (H)	12.528 ± 0.023[1]
Apparent magnitude (K)	12.507 ± 0.023[1]
Astrometry
Proper motion (μ)	RA: -1261[3] mas/yr Dec.: 1112[3] mas/yr
Parallax (π)	160.9952 ± 0.0119 mas[4]
Distance	20.259 ± 0.001 ly (6.2114 ± 0.0005 pc)
Absolute magnitude (MV)	15.23[2][5][note 1]
Details
Mass	0.81 ± 0.01[2] M☉
Radius	0.00984[2][note 2] R☉
Luminosity	0.000085[6] L☉
Surface gravity (log g)	8.36 ± 0.02[2] cgs
Temperature	5590 ± 90[2] K
Rotation	>100 years[7]
Age	5.69[note 3][3] Gyr
Other designations
WD 1748+708,[2][3] LHS 455,[2] LP 44-113,[1] NLTT 45565,[1] GJ 1221,[5] EGGR 372,[1] 2MASS J17480817+7052353[1]
Database references
SIMBAD	data
G 240-72 Location of G 240-72 in the constellation Draco

G 240-72 (orWD 1748+708, or LHS 455, or GJ 1221) is a nearby degenerate star (white dwarf) of spectral class DQP9.0,^[2] located in constellation Draco.

Distance[edit]

G 240-72 is the seventh closest white dwarf (after Sirius B, Procyon B, van Maanen's star, Gliese 440, 40 Eridani B and Stein 2051 B). Its trigonometric parallax is 0.1647 ± 0.0024 arcsec,^[5] corresponding to a distance 6.07 ± 0.09 pc, or 19.80^+0.29
_−0.28 ly.

Properties[edit]

G 240-72 has mass 0.81 Solar masses^[2] and surface gravity10^8.36 (2.29 · 10⁸) cm·s⁻²,^[2] or approximately 234 000 of Earth's, corresponding to a radius 6850 km, or 107% of Earth's.

This white dwarf has relatively low temperature 5590 K^[2] (slightly cooler than the Sun), and old cooling age, i. e. age as degenerate star (not counting duration of previous existence as main sequence star and as giant star) 5.69 Gyr.^[3] It has a white appearance, due to its similar temperature to the Sun. It has a pure helium atmosphere and rotates very slowly, with period of possibly over 100 years.^[7]

References[edit]

Notes[edit]

External links[edit]

• The 100 Nearest Star Systems (RECONS)

This article about a white dwarf is a stub. You can help Wikipedia by expanding it.