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Tau Leonis information


τ Leonis
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]
Distance560 ± 30 ly
(172 ± 10 pc)
Absolute magnitude (MV)−1.12±0.124[5]
Details
Mass3.90±0.19[6] M
Radius25.14±1.55[6] R
Luminosity329.6±39.6[6] L
Surface gravity (log g)2.25±0.05[6] cgs
Temperature4,910±33[6] K
Metallicity [Fe/H]−0.07±0.10[6] dex
Age190±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
SIMBADdata

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]

  1. ^ a b c d e f Cite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference Mermilliod1986 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Keenan1989 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference aa546_A61 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference park2013 was invoked but never defined (see the help page).
  6. ^ a b c d e f g h Cite error: The named reference Hekker2007 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference Richichi2017 was invoked but never defined (see the help page).

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Tau Leonis

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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. It...

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Absolute continuity

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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)...

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List of brightest natural objects in the sky

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"Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And ?lpha Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105.0740. Bibcode:2011ApJ...

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Adrian College

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nationally recognized fraternities: Alpha Tau Omega, Pi Kappa Alpha, Theta Chi, Sigma Alpha Epsilon and Tau Kappa Epsilon. There are three nationally...

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Deneb

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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...

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Population index

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Geminids (epsilon Geminids) Herculids (tau Herculids) Hydrids (sigma Hydrids) Leonids Leonis Minorids (Dec. Leonis Minorids) Lyrids eta Lyrids June Lyrids...

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Exoplanet naming convention

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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"...

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List of nearest exoplanets

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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...

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Bayer designation

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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...

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List of exoplanet extremes

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S2CID 16131273. Fedele; et al. (2005). "The K -Band Intensity Profile of R Leonis Probed by VLTI/VINCI". Astronomy & Astrophysics. 431 (3): 1019–1026....

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IAU designated constellations

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Lacertae Leo /ˈliːoʊ/ Leo Leon Leonis /liːˈoʊnɪs/ ancient (Ptolemy) lion Regulus Leo Minor /ˈliːoʊ ˈmaɪnər/ LMi LMin Leonis Minoris /liːˈoʊnɪs mɪˈnɒrɪs/...

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Neurite

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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...

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Beta Ursae Minoris

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; 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...

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YZ Ceti

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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...

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Solar analog

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Bibliography - Image. HD 4391 at SIMBAD - Ids - Bibliography - Image. 20 Leonis Minoris at SIMBAD - Ids - Bibliography - Image. Nu Phoenicis at SIMBAD -...

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List of nearest stars and brown dwarfs

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−07° 14′ 43″ Y4 0.003-0.010 25.0 J 28.2 J 439.0 ±2.4 sub-brown dwarf Wolf 359 (CN Leonis) 7.8558 ±0.0013 Leo* 10h 56m 29.2s +07° 00′ 53″ M6.0V 0.090 13.44 16.55...

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Sigma Draconis

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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...

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Satan

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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...

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Gliese 229

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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...

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GJ 1002

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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...

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List of nearest giant stars

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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...

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