HD 162826

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HD 162826
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 17h 51m 14.02204s[1]
Declination +40° 04′ 20.8772″[1]
Apparent magnitude (V) 6.55[1]
Spectral type F8V[1]
Proper motion (μ) RA: -16.86[1] mas/yr
Dec.: 11.01[1] mas/yr
Parallax (π)29.76 ± 0.36[1] mas
Distance110 ± 1 ly
(33.6 ± 0.4 pc)
Absolute magnitude (MV)3.92
Mass1.15 M
Radius1.11 R
Surface gravity (log g)4.41 ± 0.03 cgs
Temperature6210 ± 13 K
Metallicity [Fe/H]0.03 ± 0.01 dex
Age4.5 Gyr
Other designations
2MASS J17511402+4004208, GSC 03093-01946, TYC 3093-1946-1, BD+40 3225, HD 162826, HIP 87382, HR 6669, SAO 47009, ROT 2503
Database references

HD 162826 (HR 6669)[1] is a star in the constellation Hercules. It is about 110 light-years (34 parsecs) away from Earth.[2][3] With an apparent magnitude of 6.46,[1] the star can be found with binoculars or a low-power telescope by reference to nearby Vega in the constellation Lyra.[4] It is 15% more massive than the Sun and is 3% more abundant in metals, making it likely to harbor terrestrial planets. It is very similar to the Sun; the Sun is a G2V star with a temperature of 5778 K and 4.6 billion years old while HD 162826 is a F8V star with a temperature of 6210 K, 4.5 billion years old, and is just 15% more massive than the Sun and 3% more abundant in metals.[5][6]

The star is considered to be a stellar sibling of the Sun and is the first and only such sibling to be discovered.[7] Solar siblings are those stars that formed from the same gas cloud and in the same star cluster; the term was introduced in 2009.[8][9] It has no known planets, but due to its metallicity, it is likely to harbor terrestrial planets; the star's spectra had been under observation previously.[10]


In May 2014 astronomers at the University of Texas at Austin announced that HD 162826 is "almost certainly" one of what may be thousands of "siblings" of the Sun, emerging from the same stellar nursery some 4.5 billion years ago. This conclusion was reached by determining it has the same chemical composition as the Sun, including rare elements such as barium and yttrium, and by determining its orbit and projecting backward its revolutions about the galactic center.[2][3][11] The discovery of a first solar sibling by searching for specific rare elements may make it easier to identify other siblings in the future.[12] However, HD 162826 is probably the nearest solar sibling of this type, because others would have been identified first if they had been closer to the Sun. It had not been expected that even one sibling would be found at this relatively short distance; the study that identified this star worked on a dataset of only 100,000 stars, in preparation for data about billions of stars expected from the Gaia Space Telescope in five to ten years.[13]

The cluster in which HD 162826 and the Sun formed is believed to have been an open cluster, permitting the stars to scatter widely over time. The stars in this cluster were not too closely packed during their formation to disrupt planetary disk development, but were not so far apart as to prevent the seeding of Earth with radioactive elements produced by a nearby supernova.[14]

Possible planets and life[edit]

HD 162826 has no known planets. The current state of knowledge excludes hot Jupiters and suggests that a more distant "Jupiter" is unlikely,[15] but terrestrial planets are possible.[16] A rocky terrestrial planet situated in a Mars-like orbit at about 1.525 AU's could potentially be habitable. However, more studies on this star are needed in order to verify these habitability factors.

Lead researcher Ivan Ramirez explained the significance of finding solar siblings: "We want to know where we were born. If we can figure out in what part of the galaxy the Sun formed, we can constrain conditions on the early solar system. That could help us understand why we are here." He also said there was a "small, but not zero" chance that planets with life might orbit solar sibling stars, because during the frequent collisions during planetary formation material might have travelled from one system to another. He said the siblings might be "key candidates" in the search for extraterrestrial life.[17] A scenario for transfer of life by this means might require life or a precursor molecule to be shielded from radiation for millions of years, dormant within an outgoing chunk of planetary debris one meter or more in diameter that is produced by a meteorite impact, until this new meteorite impacts on a different planet. Such an unlikely event might have transferred life from another planet to Earth or vice versa, termed panspermia.[18]

See also[edit]


  1. ^ a b c d e f g h i "HD 162826". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved May 9, 2014.
  2. ^ a b Garber, Megan (May 8, 2014). "Our Sun Has a Sister". The Atlantic. Retrieved May 9, 2014.
  3. ^ a b Klotz, Irene (May 9, 2014). "Our Sun's Long Lost Stellar 'Sister' Found". Discovery News.
  4. ^ Saltarin, Alexander (May 10, 2014). "Meet HD 162826, the sister star of our Sun". Tech Times. Retrieved November 11, 2014.
  5. ^ "Astronomers Find Sun's Long Lost Brother". University of Texas at Austin. May 8, 2014. Retrieved May 9, 2014.
  6. ^ "Astronomers Discover Sun's 'Sibling'". Voice of America. May 9, 2014.
  7. ^ "Astronomers find Sun's 'long-lost brother,' pave way for family reunion". Science Daily. May 10, 2014. Retrieved May 13, 2014.
  8. ^ Zwart, S. Portegies (November 2009). "The long-lost siblings of the Sun". Scientific American. Retrieved November 11, 2014. (Subscription required (help)).
  9. ^ Zwart, S. Portegies (April 2009). "The Lost Siblings of the Sun". The Astrophysical Journal Letters. 696 (1): L13–L16. arXiv:0903.0237. Bibcode:2009ApJ...696L..13P. doi:10.1088/0004-637X/696/1/L13.
  10. ^ González, G.; et al. (December 8, 2009). "Parent stars of extrasolar planets – X. Lithium abundances and v sin i revisited". MNRAS. 403 (3): 1368–1380. arXiv:0912.1621. Bibcode:2010MNRAS.403.1368G. doi:10.1111/j.1365-2966.2009.16195.x.
  11. ^ Ramirez, I.; et al. "Elemental Abundances of Solar Sibling Candidates" (PDF). arXiv:1405.1723. Bibcode:2014ApJ...787..154R. doi:10.1088/0004-637X/787/2/154. Archived from the original (PDF) on 2014-05-12.
  12. ^ "Astronomers Find Sun's Sibling 'HD 162826'". Nature World News. May 9, 2014.
  13. ^ Netburn, Deborah (May 9, 2014). "Our Sun's long-lost stellar sibling found at last, astronomers say". Los Angeles Times.
  14. ^ Spotts, Pete (May 9, 2014). "Scientists make a positive ID: Nearby star is a 'sibling' of our Sun". The Christian Science Monitor. Retrieved May 10, 2014.
  15. ^
  16. ^
  17. ^
  18. ^ Gates, Sara (May 10, 2014). "Sun's 'Long-Lost Sibling' Star Identified By Texas Astronomers". The Huffington Post.

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Coordinates: Sky map 17h 51m 14.02204s, +40° 04′ 20.8772″