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Furuhjelm 46






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Coordinates: Sky map17h12m07.91s, +45° 39 57.2
 

From Wikipedia, the free encyclopedia
 


Furuhjelm 46
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 17h12m 07.91s
Declination +45° 39′ 57.2″
Apparent magnitude (V) 10.02/10.25
Characteristics
Spectral type M3 + M3.5
Astrometry
Radial velocity (Rv)–19 ± 5 km/s
Proper motion (μ) RA: +348.59 ± 5.68 mas/yr
Dec.: –1624.84 ± 6.80 mas/yr
Parallax (π)156.66 ± 1.37 mas[1]
Distance20.8 ± 0.2 ly
(6.38 ± 0.06 pc)
Orbit[2]
Period (P)12.9512 ± 0.0096 yr
Semi-major axis (a)0.7620 ± 0.0015
Eccentricity (e)0.7430 ± 0.008
Inclination (i)149.14 ± 0.25°
Longitude of the node (Ω)160.0 ± 1.3°
Periastron epoch (T)1991.032 ± 0.011[3]
Argument of periastron (ω)
(secondary)
99.0 ± 1.0°
Details
Temperature3,272 ± 28[4] K
Metallicity [Fe/H]–0.31 ± 0.17[4] dex
Other designations

BD+45° 2505, HD 155876, HIP 84140, WDS 17121+5450, KUI79

Gl 661 A: LFT 1326, LTT 15095, LHS 433, NLTT 44362
Gl 661 B: LFT 1327, LTT 15096, LHS 434, NLTT 44363
Database references
SIMBADThe system
A
B
Furuhjelm 46 is located in the constellation Hercules
Furuhjelm 46 is located in the constellation Hercules

Furuhjelm 46

Location of Furuhjelm 46 in the constellation Hercules


Furuhjelm 46, also known as HD 155876 and Gliese 661, is a nearby binary star system, consisting of two very similar red dwarfs, located in the constellation Hercules.

The star's duplicity was discovered by the Dutch astronomer Gerard Kuiper in 1934 in a systematic survey for duplicity of the known stars within about 25 parsecs from the Sun, carried out with the 36-inch telescope of the Lick Observatory.[5] Furuhjelm 46 is the nearest "true" (i. e. not brown dwarf) star system in Hercules, however, there is brown dwarf in this constellation, located closer: WISE 1741+2553.

References

[edit]
  1. ^ Söderhjelm, Staffan (1999). "HIP 84140". Visual binary orbits and masses post Hipparcos.
  • ^ From the Sixth Catalog of Orbits of Visual Binary Stars, based upon Hartkopf, W. I.; Mason, B. D.; McAlister, H. A. (1996), "Binary star orbits from speckle interferometry. VIII. Orbits of 37 close visual systems", Astronomical Journal, 111: 370–392, Bibcode:1996AJ....111..370H, doi:10.1086/117790
  • ^ Fractional Besselian year.
  • ^ a b Rojas-Ayala, Bárbara; et al. (April 2012). "Metallicity and Temperature Indicators in M Dwarf K-band Spectra: Testing New and Updated Calibrations with Observations of 133 Solar Neighborhood M Dwarfs" (PDF). The Astrophysical Journal. 748 (2): 93. arXiv:1112.4567. Bibcode:2012ApJ...748...93R. doi:10.1088/0004-637X/748/2/93. S2CID 41902340.
  • ^ Kuiper, Gerard (1934). "Two New Close M-Dwarf Binaries of Large Parallax". Publications of the Astronomical Society of the Pacific. 46 (373): 235. Bibcode:1934PASP...46..235K. doi:10.1086/124479. S2CID 119814250.
  • [edit]
    Retrieved from "https://en.wikipedia.org/w/index.php?title=Furuhjelm_46&oldid=1191747053"

    Categories: 
    Binary stars
    Hercules (constellation)
    M-type main-sequence stars
    Gliese and GJ objects
    Henry Draper Catalogue objects
    Hipparcos objects
    Durchmusterung objects
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
    Webarchive template wayback links
     



    This page was last edited on 25 December 2023, at 14:11 (UTC).

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