HD 201647

Last updated
HD 201647
Microscopium constellation map.svg
Red circle.svg
Location of HD 201647 on the map (circled)
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension 21h 12m 13.71281s [1]
Declination −40° 16 09.7010 [1]
Apparent magnitude  (V)5.83 [2] (5.83 - 5.86) [3]
Characteristics
Spectral type F5 V [4] [5]
B−V color index +0.45 [2]
Variable type suspected [3]
Astrometry
Radial velocity (Rv)4.5±0.9 [6]  km/s
Proper motion (μ)RA: +58.359  mas/yr [1]
Dec.: −218.773  mas/yr [1]
Parallax (π)31.4586 ± 0.0401  mas [1]
Distance 103.7 ± 0.1  ly
(31.79 ± 0.04  pc)
Absolute magnitude  (MV)+3.33 [7]
Details
Mass 1.28 [8]   M
Radius 1.47+0.07
0.04
[9]   R
Luminosity 3.79±0.01 [1]   L
Surface gravity (log g)4.21±0.01 [10]   cgs
Temperature 6,637±80 [11]   K
Metallicity [Fe/H]+0.06±0.01 [12]   dex
Rotational velocity (v sin i)25.1±2.5 [13]  km/s
Age 916 [8]   Myr
Other designations
55 G. Microscopii [14] , NSV  25506, CD−40°14216, CPD−40°9488, GC  29614, GJ  9726, HD  201647, HIP  104680, HR  8100, SAO  230575, LTT  8410, TIC  159670453 [15]
Database references
SIMBAD data

HD 201647 (HR 8100; Gliese 9726; LTT 8410) is a solitary star [16] located in the southern constellation Microscopium. It is faintly visible to the naked eye as a yellowish-white-hued star with an apparent magnitude of 5.83. [2] The object is located relatively close at a distance of light-years based on Gaia DR3 parallax measurements, but it is receding with a heliocentric radial velocity of 4.5  km/s . [6] At its current distance, HD 201647's brightness is diminished by 0.11 magnitudes due to interstellar extinction [17] and it has an absolute magnitude of +3.33. [7] It has a relatively high proper motion across the celestial sphere, moving at a rate of 226.331 mas/yr. [18]

HD 201647 has a stellar classification of F5 V, [5] [4] indicating that it is an ordinary F-type main-sequence star that is generating energy via hydrogen fusion at its core. It has 1.28 times the mass of the Sun [8] and 1.47 times the radius of the Sun. [9] It radiates 3.79 times the luminosity of the Sun [1] from its photosphere at an effective temperature of 6,637  K . [11] HD 201647 is slightly metal enriched with an iron abundance of [Fe/H] = +0.06 or 115% of the Sun's. [12] It is estimated to be 916 million years old [8] and it spins modestly with a projected rotational velocity of 25.1  km/s . [13]

In the discovery paper for Lacaille 8760, HD 201647 was reported to be a variable star that varied between 5.83 and 5.86 in the visual passband. [3] As of 2004 however, it has not been confirmed to be variable. [19]

Related Research Articles

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<span class="mw-page-title-main">HD 201772</span> Star in the constellation Microscopium

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<span class="mw-page-title-main">HD 168592</span> Star in the constellation of Corona Australis

HD 168592, also designated as HR 6862 or rarely 7 G. Coronae Australis, is a solitary star located in the southern constellation Corona Australis. It is faintly visible to the naked eye as an orange-hued star with an apparent magnitude of 5.07. Gaia DR3 parallax measurements place it at a distance of 490 light years and is currently receding with a heliocentric radial velocity of 18 km/s. At its current distance, HD 168592's brightness is diminished by 0.38 magnitudes due to interstellar dust. It has an absolute magnitude of −0.76.

<span class="mw-page-title-main">HD 45866</span> Star in the constellation of Camelopardalis

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<span class="mw-page-title-main">HD 23005</span> Star in Camelopardlis

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<span class="mw-page-title-main">HD 170521</span> Distant K-type giant; Corona Australis

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