Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Leo
Right ascension
11h 31m 44.94461s[1]
Declination
+14° 21′ 52.2131″[1]
Apparent magnitude (V)
6.27[2] + 9.22[3]
Characteristics
Spectral type
F9.5V[4] + G5[3]
B−V color index
0.570[2]
Astrometry
Radial velocity (Rv)
−4.81±0.09[2] km/s
Proper motion (μ)
RA: −330.279[1] mas/yr Dec.: −190.081[1] mas/yr
Parallax (π)
42.2619 ± 0.0812 mas[1]
Distance
77.2 ± 0.1 ly (23.66 ± 0.05 pc)
Absolute magnitude (MV)
4.46[2]
Details
88 Leo A
Mass
1.06[5]M☉
Radius
1.10+0.03 −0.05[1]R☉
Luminosity
1.470±0.004[1]L☉
Surface gravity (log g)
4.25[6] cgs
Temperature
6,060+140 −76[1] K
Metallicity [Fe/H]
−0.06±0.02[2] dex
Rotation
14.32 days[7]
Age
5.7+1.6 −3.1[2] Gyr
88 Leo B
Mass
0.74[8]M☉
Other designations
STF 1547 AB, 88 Leonis, BD+15°2345, HD 100180, HIP 56242, HR 4437, WDS J11317+1422, Wolf 401[9]
88 Leo A: AG+14°1209, GJ 3669, SAO 99648, LTT 13145[9]
88 Leo B: AG+14°1208, GJ 3670, SAO 99647, LTT 13146[10]
Database references
SIMBAD
data
88 Leonis is a wide binary[5] star system in the equatorial constellation of Leo, the lion. The system is near the lower limit of visibility to the naked eye with an apparent visual magnitude of 6.27.[2] It is located at a distance of 77 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −4.8 km/s.[2] It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.379 arc seconds per annum.[11]
The primary member of the system, component A, is a yellow-white hued F-type main-sequence star with a stellar classification of F9.5V.[4] It is an estimated 5.7[2] billion years old and is spinning with a rotation period of 14.3 days.[7] The star has a short magnetic activity cycle that averages around 3.5 years. A second cycle appears to vary over time, lasting 13.7 years at the start of observations then decreasing to 8.6 years over a span of 34 years of measurement.[7] The star has 1.06[5] times the mass of the Sun and 1.10[1] times the Sun's radius. It is radiating 1.47[1] times the luminosity of the Sun from its photosphere at an effective temperature of 6,060 K.[1]
The secondary, component B, is a magnitude 9.22[3] star at an angular separation of 15.46″ from the primary along a position angle of 326°.[8] It has a class of G5[3] and 74% of the Sun's mass. The pair share a common proper motion through space with a projected separation of 360.6 AU.[8]
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^Cite error: The named reference Hinkel2017 was invoked but never defined (see the help page).
^ abcCite error: The named reference Oláh2009 was invoked but never defined (see the help page).
^ abcCite error: The named reference Tokovinin2016 was invoked but never defined (see the help page).
^ abCite error: The named reference SIMBADA was invoked but never defined (see the help page).
^Cite error: The named reference SIMBADB was invoked but never defined (see the help page).
^Cite error: The named reference Lepine2005 was invoked but never defined (see the help page).
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