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62 Aries

62 Aries ( lat. 62 Arietis ), or Tianhe ( Chinese 天 阿 ), is a solitary star in the constellation Aries . It is located at a distance of 884 light years (271 parsecs) from the Sun. Initially, parallax was estimated at 3.35 ± 1.16 mas [1] , then it was specified 3.69 ± 0.49 mas [3] .

62 Aries
Star
Observational data
( Age J2000.0 )
Right ascension
Declination
Distance884 St. of the year
Visible magnitude ( V )+5.52 [1]
ConstellationAries
Astrometry
Radial velocity ( R v )6.2 [1] km / s
Own movement (μ)RA: 4.42 [1]
Dec: -9.88 [1]
Parallax (π)3.69 ± 0.49 mas
Absolute magnitude (V)-1.65
Specifications
Spectral classG5IIID [1]
physical characteristics
Temperature
Luminosity391 L ☉
Other designations
Fl 62 ari
BD +27 500 , HD 20825 , HIC 15696 , HIP 15696 , HR 1012 , IRAS 03191 + 2725 , PPM 92435 , SAO 75892 , 2MASS J03221188 + 2736271, AG +27 333, GC 4017, GCRV 1859, SKY # 5064, UBV M 9468, YPAC 317, YZ 27 1662
Database Information
SIMBADdata
Sources: [1]

The star is a yellow giant of the spectral class G5 III [4] . Thanks to a visible magnitude of 5.52, it is visible to the naked eye [5] .

Content

Title

In Chinese astrology, 62 Aries is called 天 阿 (Tiānhé, Tianhe) which means “Heavenly River”, because this star is located separately in the asterism of the Heavenly River, which takes place in the Chinese constellation Hairy Head [6] .

See also

  • Aries constellation stars list

Notes

  1. ↑ 1 2 3 4 5 6 7 SIMBAD (English) . - 62 Aries in the SIMBAD database . Date of treatment April 14, 2010.
  2. ↑ 1 2 S. Hekker Precise radial velocities of giant stars // Astron. Astrophys. - EDP ​​Sciences , 2007. - Vol. 475, Iss. 3. - P. 1003–1009. - ISSN 0004-6361 ; 0365-0138 ; 1432-0746 ; 1286-4846 - doi: 10.1051 / 0004-6361: 20078233
    <a href=" https://wikidata.org/wiki/Track:Q114404 "> </a> <a href=" https://wikidata.org/wiki/Track:Q60784972 "> </a> <a href = " https://wikidata.org/wiki/Track:Q752075 "> </a> <a href=" https://wikidata.org/wiki/Track:Q54255401 "> </a>
  3. ↑ Validation of the new Hipparcos reduction
  4. ↑ A catalog of multiplicity among bright stellar systems
  5. ↑ Rybka E. The corrected magnitudes and colors of 278 stars near SA 1-139 in the UBV system (Eng.) // Acta Astronomica: journal. - 1969. - Vol. 19 . - P. 229 . - .
  6. ↑ 陳久 金.中國 星座 神話. - 台灣 書房 出版 有限公司, 2005. - P. 470. - ISBN 9789867332257 .

Links

  • HR 1012
  • Aladin previewer


Source - https://ru.wikipedia.org/w/index.php?title=62_Ovna&oldid=100073330


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