HD 165185 is the Henry Draper Catalogue designation for a star in the southern zodiac constellation of Sagittarius. It has an apparent visual magnitude of 5.94,[2] which indicates it is a sixth magnitude star that is faintly visible to the naked eye. (According to the Bortle scale, it can be viewed from dark suburban skies.) Parallax measurements give an estimated distance of 55.8 light years from the Sun.[1] It is drifting further away with a heliocentric radial velocity of +15.4 km/s.[2]

Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 165185
Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 18h 06m 23.720s[1]
Declination –36° 01 11.23[1]
Apparent magnitude (V) 5.94[2]
Characteristics
Spectral type G1 V[2]
U−B color index 0.07[3]
B−V color index 0.61[3]
Astrometry
Radial velocity (Rv)+15.4[2] km/s
Proper motion (μ) RA: +106.020 mas/yr[1]
Dec.: +8.812 mas/yr[1]
Parallax (π)58.4296 ± 0.0404 mas[1]
Distance55.82 ± 0.04 ly
(17.11 ± 0.01 pc)
Absolute magnitude (MV)+4.59[4]
Details
Mass1.13[5] M
Radius0.94[6] R
Luminosity (bolometric)1.15[7] L
Surface gravity (log g)4.46±0.06[8] cgs
Temperature5,940±18[8] K
Metallicity [Fe/H]−0.05±0.03[8] dex
Rotation5.90[6] days
Rotational velocity (v sin i)7.53[8] km/s
Age437±186[5] Myr
Other designations
29 G. Sgr[9], CD−36°12214, GJ 702.1, HD 165185, HIP 88694, HR 6748, SAO 209710, WDS J18064-3601A[10]
Database references
SIMBADdata
ARICNSdata
Close

This star is a pre-main-sequence[11] solar analog[12] with a stellar classification of G1 V.[2] It is spinning with a projected rotational velocity of 7.53 km/s[8] and a rotation period of 5.9 days.[6] Measurements of magnetic activity in the chromosphere show variations over time, much like the sunspot cycle. This activity showed a distinct peak in 2009.[13] Stellar models give an estimated mass equal to 1.13[5] times the mass of the Sun, but only 94%[6] of the Sun's radius. The total, or bolometric luminosity of the star is 15% higher than the Sun,[7] while the abundance of elements other than hydrogen and helium—what astronomer's term the metallicity—is nearly the same as in the Sun.[8] The stellar atmosphere has an effective temperature of 5,940[8] K, giving it the yellow-hued glow of a G-type star.[14]

HD 165185 completed its perihelion passage some 851,000 years ago when it came within 29 ly (8.9 pc) of the Sun,[15] and it is now moving away with a radial velocity component of 15.4 km/s.[2] Based upon the motion of this star through space, its age, and properties, this star is a probable member of the Ursa Major Moving Group; a stellar kinematic group that formed in the same region of space.[11] It has a suspected common proper motion companion at an angular separation of 12, corresponding to a projected separation of 220 AU. This is a red dwarf star with a stellar classification of M0 and an infrared K band magnitude of 8.11.[16]

References

Wikiwand in your browser!

Seamless Wikipedia browsing. On steroids.

Every time you click a link to Wikipedia, Wiktionary or Wikiquote in your browser's search results, it will show the modern Wikiwand interface.

Wikiwand extension is a five stars, simple, with minimum permission required to keep your browsing private, safe and transparent.