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HD 143436
Observation data
Epoch J2000       Equinox J2000
Constellation Serpens
Right ascension 16h 00m 18.83726s [1]
Declination +00° 08′ 13.2306″ [1]
Apparent magnitude (V) 8.03 [2]
Characteristics
Spectral type G3V [3]
B−V color index 0.644 [4]
Astrometry
Radial velocity (Rv)−24.7±0.7 [4] km/s
Proper motion (μ) RA: −136.615 [1]  mas/ yr
Dec.: −108.779 [1]  mas/ yr
Parallax (π)22.3164 ± 0.0456  mas [1]
Distance146.2 ± 0.3  ly
(44.81 ± 0.09  pc)
Absolute magnitude (MV)4.87±0.10 [4]
Details [4]
Mass1.01±0.02  M
Radius1.01+0.01
−0.04
[1]  R
Luminosity1.047±0.003 [1]  L
Surface gravity (log g)4.28±0.12  cgs
Temperature5,768±43  K
Metallicity [Fe/H]0.008  dex
Rotational velocity (v sin i)< 2.6 km/s
Age3.8±2.9  Gyr
Other designations
BD+00°3441, HIP 78399, SAO 121307, PPM 162138, LTT 14757, NLTT 41715 [5]
Database references
SIMBAD data

HD 143436 also known as HIP 78399, is a G-type star in the constellation Serpens. The temperature, rotation, mass, and abundance of elements in this star are close to properties of the Sun, and for this reason it is a solar twin candidate. The only notable difference is an approximately six times higher abundance of lithium compared to the Sun and most likely a younger age of 3.8 Gyr. The space velocity components of this star are (U, V, W) = (−19.2, −38.6, −7.0) km/s. [4]

References

  1. ^ a b c d e f g Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode: 2000A&A...355L..27H. doi: 10.1888/0333750888/2862.
  3. ^ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey. 05. Bibcode: 1999MSS...C05....0H.
  4. ^ a b c d e King, Jeremy R.; et al. (November 2005). "Keck HIRES Spectroscopy of Four Candidate Solar Twins". The Astronomical Journal. 130 (5): 2318–2325. arXiv: astro-ph/0508004. Bibcode: 2005AJ....130.2318K. doi: 10.1086/452640. S2CID  6535115.
  5. ^ "HD 143436". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-05.