93 Leonis

93 Leonis
Location of 93 Leonis (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 11h 47m 59.13595s
Declination +20° 13′ 08.1500″
Apparent magnitude (V) 4.522
Characteristics
Spectral type G5III + A7V
U−B color index +0.28
B−V color index +0.9 / +0.2
Variable type RS CVn
Astrometry
Radial velocity (Rv)0.750 ± 0.05 km/s
Proper motion (μ) RA: −145.49 mas/yr
Dec.: −4.34 mas/yr
Parallax (π)14.02±0.23 mas
Distance233 ± 4 ly
(71 ± 1 pc)
Absolute magnitude (MV)+0.23
Orbit
Period (P)71.69 d
Semi-major axis (a)7.5±0.1 mas
Eccentricity (e)0
Inclination (i)50.1±0.5°
Longitude of the node (Ω)138±1°
Periastron epoch (T)JD 2447642.6 ± 0.2
Argument of periastron (ω)
(secondary)
Semi-amplitude (K1)
(primary)
29.67±0.29 km/s
Semi-amplitude (K2)
(secondary)
33.8±2.1 km/s
Details
93 Leo Aa
Mass2.25±0.29 M
Radius9.1±0.5 R
Luminosity49.4±3.4 L
Temperature5,100±100 K
93 Leo Ab
Mass1.97±0.15 M
Radius2.7±0.2 R
Luminosity23.9±1.9 L
Temperature7,800±200 K
Other designations
DQ Leo, BD+21°2358, FK5 1304, HD 102509, HIP 57565, HR 4527, SAO 81998
Database references
SIMBADdata

93 Leonis (93 Leo) is a binary star in the constellation Leo. Its apparent magnitude is 4.522. Based on the system's parallax, 93 Leonis is located about 233 light-years (71 parsecs) away.

93 Leonis is a double-lined spectroscopic binary. Two components are known to exist, because their spectral lines shift periodically, due to the Doppler effect. The two stars are a G-type red giant and an A-type main-sequence star. They complete an orbit once every 71.69 days. The system is also known to be an RS Canum Venaticorum variable, due to its binarity. For that reason, it has been given the variable star designation DQ Leonis.

In Chinese astronomy, 93 Leonis is called 太子, Pinyin: Tàizǐ, meaning Crown Prince, because this star is marking itself and stand alone in Crown Prince asterism, Supreme Palace enclosure mansion (see : Chinese constellation).