HD 197027

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HD 197027
HIP 102152.jpg
HIP 102152
Credit: ESO/Digitized Sky Survey 2
Observation data
Epoch J2000      Equinox J2000
Constellation Capricornus
Right ascension 20h 41m 45.632s[1]
Declination −27° 12′ 57.414″[1]
Apparent magnitude (V) 9.18
Characteristics
Spectral type G3V[1]
B−V color index +0.65[1]
Astrometry
Radial velocity (Rv)-44.3[1] km/s
Proper motion (μ) RA: +172.91[1] mas/yr
Dec.: -15.41[1] mas/yr
Parallax (π)12.84 ± 0.97[1] mas
Distance250 ± 20 ly
(78 ± 6 pc)
Absolute magnitude (MV)4.72
Details
Mass0.97[2] M☉
Surface gravity (log g)4.40±0.02[3] cgs
Temperature5718±5[3] K
Metallicity [Fe/H]−0.020±0.005[3] dex
Rotational velocity (v sin i)1.78±0.12[3] km/s
Age6.92±0.69[3] Gyr
Other designations
CD−27° 14976, HIP 102152, SAO 189585.[1]
Database references
SIMBADdata

HD 197027 (HIP 102152) is a star in the constellation Capricornus that is located about 250 light years from the Sun.

The measured properties of this star are very similar to those of the Sun, making it a candidate older solar twin.[4] The abundances of 21 elements overall are more similar to the Sun than any other known solar twin. Additionally, the effective temperature, surface gravity, and microturbulence are nearly identical to the Sun's. However, it is significantly older than the Sun, being approximately 2.2 billion years older than the Sun, at 6.9 billion years old. The fact that the abundances are so similar to the Sun's suggests that it is a potential candidate for hosting terrestrial type planets.

Age[]

The age of HD 197027, here annotated as HIP 102152, shown relative to the Sun, the younger solar twin 18 Scorpii and the formation of the Milky Way

References[]

  1. ^ a b c d e f g h i "HD 197027". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-09-07.
  2. ^ Talawanda R. Monroe; et al. (Aug 2013). "High Precision Abundances of the Old Solar Twin HIP 102152: Insights on Li Depletion from the Oldest Sun". Astrophysical Journal Letters. 774 (2): L32. arXiv:1308.5744. Bibcode:2013ApJ...774L..32M. doi:10.1088/2041-8205/774/2/l32. S2CID 56111132.
  3. ^ a b c d e dos Santos, Leonardo A.; et al. (August 2016), "The Solar Twin Planet Search. IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars", Astronomy & Astrophysics, 592: 8, arXiv:1606.06214, Bibcode:2016A&A...592A.156D, doi:10.1051/0004-6361/201628558, S2CID 53533614, A156.
  4. ^ ESO, The life cycle of a Sun-like star (annotated), from European Southern Observatory, 28 August 2013

External links[]


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