Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Leo
Right ascension
11h 27m 56.23976s[1]
Declination
+02° 51′ 22.5609″[1]
Apparent magnitude (V)
5.00[2]
Characteristics
Spectral type
G8- IIIa[3]
U−B color index
+0.80[2]
B−V color index
+1.005[2]
Astrometry
Radial velocity (Rv)
−8.90[4] km/s
Proper motion (μ)
RA: +16.89[1] mas/yr Dec.: −9.81[1] mas/yr
Parallax (π)
5.80 ± 0.33 mas[1]
Distance
560 ± 30 ly (172 ± 10 pc)
Absolute magnitude (MV)
−1.12±0.124[5]
Details
Mass
3.90±0.19[6]M☉
Radius
25.14±1.55[6]R☉
Luminosity
329.6±39.6[6]L☉
Surface gravity (log g)
2.25±0.05[6] cgs
Temperature
4,910±33[6] K
Metallicity [Fe/H]
−0.07±0.10[6] dex
Age
190±20[6] Myr
Other designations
τ Leo, 84 Leo, BD+03°2504, FK5 1297, HD 99648, HIP 55945, HR 4418, SAO 118875[7]
Database references
SIMBAD
data
Tau Leonis (τ Leo) is a star in the zodiac constellation of Leo. Because it is located near the ecliptic, it is subject to occultations by the Moon.[8] It has an apparent visual magnitude of 5.00,[2] which is bright enough to be seen with the naked eye. The distance to this star, as estimated using parallax measurements,[1] is 560 light years. It is moving closer to the Sun with a radial velocity of −9 km/s.[4]
This G-type giant star has a stellar classification of G8- IIIa[3] and currently resides on the red giant branch. It has about 390% of the Sun's mass. The star is much younger than the Sun, with an age of around 190 million years. As an evolved giant, it has expanded to about 25 times the Sun's radius and radiates 330 times the luminosity of the Sun. The effective temperature of the outer atmosphere is 4,910 K.[6]
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^Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
^Cite error: The named reference Richichi2017 was invoked but never defined (see the help page).
TauLeonis (τ Leo) is a star in the zodiac constellation of Leo. Because it is located near the ecliptic, it is subject to occultations by the Moon. It...
Tau Ceti, Latinized from τ Ceti, is a single star in the constellation Cetus that is spectrally similar to the Sun, although it has only about 78% of...
Tristan de Leonis y del rey don Tristan de Leonis el joven su hijo ("Newly Revised and Expanded Chronicle of the Great Knight Sir Tristan of Leonis and His...
AD Leonis is a main sequence star with a spectral classification of M3.5V. It is a flare star that undergoes random increases in luminosity. AD Leonis is...
t ] ⊆ I {\displaystyle d\left(f(s),f(t)\right)\leq \int _{s}^{t}m(\tau )\,d\tau {\text{ for all }}[s,t]\subseteq I} for some m in the Lp space Lp(I)...
system 1.97 1.87 Beta Canis Majoris Star 1.97 Alphard Star 2.00 1.84 Gamma Leonis Binary star system 2.01 Hamal Star 2.01 Beta Ceti Star 2.01 Mizar Quadruple...
"Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And ?lpha Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105.0740. Bibcode:2011ApJ...
nationally recognized fraternities: Alpha Tau Omega, Pi Kappa Alpha, Theta Chi, Sigma Alpha Epsilon and Tau Kappa Epsilon. There are three nationally...
the mid-ultraviolet spectrum of α Cygni (A2 Ia), β Orionis (B8 Ia), and η Leonis (A0 Ib)". The Astrophysical Journal. 223: 207. Bibcode:1978ApJ...223..207L...
Geminids (epsilon Geminids) Herculids (tau Herculids) Hydrids (sigma Hydrids) Leonids Leonis Minorids (Dec. Leonis Minorids) Lyrids eta Lyrids June Lyrids...
circumbinary planets around PSR B1620-26 and DP Leonis can almost retain their names (PSR B1620-26 b and DP Leonis b) as unofficial informal forms of the "(AB)b"...
Star (12.8 ly), Van Maanen 2 (14.1 ly), Groombridge 1618 (15.9 ly), AD Leonis (16.2 ly), VB 10 (19.3 ly), and Fomalhaut (25.1 ly). In 2021, a candidate...
designating an Alpha in Leo Minor, so it also has no Alpha. (The star 46 Leonis Minoris would have been the obvious candidate.) In Orion, Bayer first designated...
S2CID 16131273. Fedele; et al. (2005). "The K -Band Intensity Profile of R Leonis Probed by VLTI/VINCI". Astronomy & Astrophysics. 431 (3): 1019–1026....
Lacertae Leo /ˈliːoʊ/ Leo Leon Leonis /liːˈoʊnɪs/ ancient (Ptolemy) lion Regulus Leo Minor /ˈliːoʊ ˈmaɪnər/ LMi LMin Leonis Minoris /liːˈoʊnɪs mɪˈnɒrɪs/...
is stimulated by neurotrophic factors, such as nerve growth factor (NGF). Tau proteins can aid in the stabilization of microtubules by binding to the microtubules...
; Kim, K.-M. (June 2014). "Planetary companions in K giants β Cancri, μ Leonis, and β Ursae Minoris". Astronomy and Astrophysics. 566 (A67): 7. arXiv:1405...
the mass of the Sun and 17% of its radius. This star is unusually close to Tau Ceti, a star of spectral class G8. The two are only about 1.6 light years...
Bibliography - Image. HD 4391 at SIMBAD - Ids - Bibliography - Image. 20 Leonis Minoris at SIMBAD - Ids - Bibliography - Image. Nu Phoenicis at SIMBAD -...
their open-air kitchens. It was the name of an association of this star, Tau Draconis and Upsilon Draconis. According to a 1971 NASA memorandum, Athāfi...
main deity in the tentatively Indo-European pantheon of the Yazidis, Melek Taus, is similar to the devil in Christian and Islamic traditions, as he refused...
0036 ly) 2 planets: b, c Gliese 412 (15.9969±0.0026 ly) red dwarf B AD Leonis (16.1939±0.0024 ly) Gliese 832 (16.2005±0.0019 ly) planet b Gliese 682 (16...
0036 ly) 2 planets: b, c Gliese 412 (15.9969±0.0026 ly) red dwarf B AD Leonis (16.1939±0.0024 ly) Gliese 832 (16.2005±0.0019 ly) planet b Gliese 682 (16...
and Hotter: Interferometric imaging of {\beta} Cassiopeiae and {\alpha} Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105.0740. doi:10.1088/0004-637X/732/2/68...