HD 198357

Last updated
HD 198357
Microscopium constellation map.svg
Red circle.svg
Location of HD 198357 on the map (circled)
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension 20h 51m 00.75817s [1]
Declination −37° 54 47.9922 [1]
Apparent magnitude  (V)5.50±0.01 [2]
Characteristics
Spectral type K3 III [3] or K3 II [4]
B−V color index +1.38 [5]
Astrometry
Radial velocity (Rv)16.5±2.9 [6]  km/s
Proper motion (μ)RA: −7.436  mas/yr [1]
Dec.: −17.374  mas/yr [1]
Parallax (π)5.7348 ± 0.0797  mas [1]
Distance 569 ± 8  ly
(174 ± 2  pc)
Absolute magnitude  (MV)−0.75 [7]
Details
Mass 1.81±0.44 [8]   M
Radius 37.8±1.9 [9]   R
Luminosity 417+16
15
[1]   L
Surface gravity (log g)1.06 [10]   cgs
Temperature 4,318±51 [11]   K
Metallicity [Fe/H]−0.12 [10]   dex
Rotational velocity (v sin i)<1.0 [12]  km/s
Other designations
28 G. Microscopii [13] , CD−38°14250, CPD−38°8121, GC  29053, HD  198357, HIP  102916, HR  7971, SAO  212488 [14]
Database references
SIMBAD data

HD 198357 (HR 7971; 28 G. Microscopii) is a solitary star located in the southern constellation Microscopium. It is faintly visible to the naked eye as an orange-hued point of light with an apparent magnitude of 5.50. [2] Gaia DR3 parallax measurements imply a distance of 569 light-years [1] and the object is currently receding with a heliocentric radial velocity of 16.5  km/s . [6] At its current distance, HD 198357's brightness is diminished by 0.18 magnitudes due to interstellar extinction [15] and it has an absolute magnitude of −0.75. [7]

HD 198357 has a stellar classification of K3 III, [3] indicating that it is an evolved K-type giant star. David Stanley Evans gave a classification of K3 II, indicating a more evolved bright giant. [4] It has 1.81 times the mass of the Sun [8] but it has expanded to 37.8 times the radius of the Sun. [9] It radiates 417 times the luminosity of the Sun [1] from its photosphere at an effective temperature of 4,318  K . [11] HD 198357 is slightly metal deficient with an iron abundance three-quarters that of the Sun or [Fe/H] = −0.12 [10] and it spins too slowly for its projected rotational velocity to be measured accurately. [12] HD 198357 has a peculiar velocity of 27.7+3.9
−4.1
  km/s
, indicating that it may be a runaway star (46% chance). [16]

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References

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