Astronomy:GD 40

From HandWiki
Short description: Star in the constellation Cetus
GD 40
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cetus[1]
Right ascension  03h 02m 53.10375s[2]
Declination −01° 08′ 33.7987″[2]
Apparent magnitude (V) 15.56[3]
Characteristics
Evolutionary stage white dwarf[3]
Spectral type DB[3]
Astrometry
Parallax (π)15.3618 ± 0.0456[2] mas
Distance212.3 ± 0.6 ly
(65.1 ± 0.2 pc)
Absolute magnitude (MV)11.30[3]
Details[3]
Mass0.54 M
Radius0.014±0.003[lower-alpha 1] R
Luminosity0.0068 L
Surface gravity (log g)7.91±0.18 cgs
Age200 Myr
Other designations
GD 40, EGGR 384, US 3562, WD 0300-013
Database references
SIMBADdata

GD 40 is a white dwarf in the constellation Cetus. It is located about 212 light-years (65 parsecs) away from the Sun.[2] The star's spectrum has been found to show traces of external of metal contamination due to disruption of an extrasolar dwarf planet or an asteroid.[4] The disrupted object should have had at least the same mass of the asteroid 4 Vesta.

See also

  • ZZ Piscium
  • GD 61, white dwarf with an observed asteroid

Notes

  1. Derived from known mass and gravity of star; radius is consistent with known luminosity and temperature within 0.4%.

References

  1. Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode1987PASP...99..695R  Constellation record for this object at VizieR.
  2. 2.0 2.1 2.2 2.3 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  3. 3.0 3.1 3.2 3.3 3.4 Limoges, M.-M.; Bergeron, P. (2010). "A Spectroscopic Analysis of White Dwarfs in the Kiso Survey". The Astrophysical Journal 714 (2): 1037–1051. doi:10.1088/0004-637X/714/2/1037. Bibcode2010ApJ...714.1037L. 
  4. Klein (2010). "Chemical Abundances in the Externally Polluted White Dwarf GD 40: Evidence of a Rocky Extrasolar Minor Planet". The Astrophysical Journal 709 (2): 950–962. doi:10.1088/0004-637X/709/2/950. Bibcode2010ApJ...709..950K.