Delta Leonis
Zosma, δ Leo
Zosma is the δ star on the upper left of the map
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Observation data
Epoch J2000 Equinox J2000 |
Constellation |
Leo |
Right ascension |
11h 14m 06.5013s[1] |
Declination |
20° 31′ 25.381″[1] |
Apparent magnitude (V) |
2.56 [1] |
Characteristics |
Spectral type |
A4 V [1] |
U−B color index |
0.12 [1] |
B−V color index |
0.12 [1] |
Variable type |
Delta Scuti? |
Astrometry |
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Radial velocity (Rv) |
-20.2 [1] km/s |
Proper motion (μ) |
RA: 143.31 [1] mas/yr
Dec.: -130.43 [1] mas/yr |
Parallax (π) |
56.52 ± 0.83[2] mas |
Distance |
57.7 ± 0.8 ly
(17.7 ± 0.3 pc) |
Absolute magnitude (MV) |
1.29 |
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Details |
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Mass |
2.2 [3] M☉ |
Radius |
2[3] R☉ |
Luminosity |
23 [3] L☉ |
Temperature |
8,350 [3] K |
Metallicity |
? Fe/H |
Rotation |
180 km/s[4] (<1/2 day)[3] |
Age |
6-7.5×108 [3] years |
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Other designations |
Zosma, Zozma, Zosca, Duhr, Zubra, δ Leo, 68 Leo, HR 4357, BD +21°2298, HD 97603, SAO 81727, FK5 422, HIP 54872, Gl 419, GCTP 2614.00, GC 15438
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Database references |
SIMBAD |
data |
Delta Leonis (δ Leo, δ Leonis) is a star in the constellation of Leo. It has the traditional names Zosma (or Zozma) and Duhr. Rare spellings include Zozca, Zosca, Zubra, and Dhur. The name Zosma means girdle in ancient Greek, referring to the star's location in its constellation, on the hip of the lion.
Properties
Zosma is a relatively ordinary main sequence star, although it is somewhat larger and hotter than the Sun. It is a fairly well-studied star, allowing relatively accurate measurements of its age and size. Having a larger mass than the Sun it will have a shorter lifespan, and in another 600 million years or so will swell into an orange or red giant star before decaying quietly into a white dwarf. The absolute magnitude of Zosma is 1.29 while its apparent magnitude is 2.56.
See also
References
External links
- Jim Kaler's Stars, University of Illinois: ZOSMA (Delta Leonis)
- Star Names, Their Lore and Legend, Richard Hinckley Allen, New York, Dover, various dates
← «Bright» star systems within 50–60 light-years →
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Chi Eridani (57.0 ± 0.6 ly; 2 stars)
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Mu Arae (49.8 ± 0.6 ly; 1 star, 4 planets: planet d • planet e • planet b • planet c)‡ • 51 Pegasi ( 50.1 ± 0.6 ly; 1 star, 1 planet: planet b «Bellerophon»)‡ • HR 7368 ( 50.5 ± 0.5 ly; 1 star, 2 brown dwarfs: brown dwarf C • brown dwarf B) • HR 2007 ( 50.8 ± 0.9 ly; 1 star, 1 planet: planet b)‡ • HR 8323 ( 51.0 ± 0.6 ly; 1 star) • HR 7670 ( 51.8 ± 0.5 ly; 3 stars, 2 planets: planet c • planet b) • Psi⁵ Aurigae ( 53.9 ± 0.6 ly; 1 star) • HR 3538 ( 55.8 ± 0.8 ly; 1 star) • Iota Horologii ( 56.2 ± 0.5 ly; 1 star, 1 planet: planet b) • 37 Geminorum ( 56.3 ± 0.9 ly; 1 star) • Rho Coronae Borealis ( 56.8 ± 0.7 ly; 1 star, 1 planet: planet b) • GJ 3021 ( 57.5 ± 0.5 ly; 1 star, 1 planet: planet b) • 15 Sagittae ( 57.6 ± 0.6 ly; 1 star, 1 brown dwarf) • HR 7644 ( 57.8 ± 0.8 ly; 1 star, 1 planet: planet b) • HR 5534 ( 58.5 ± 0.9 ly; 1 star, 2 brown dwarfs) • Gliese 651 ( 58.9 ± 0.6 ly; 1 star, 1 planet: planet b) • 70 Virginis ( 59.1 ± 0.8 ly; 1 star, 1 planet: planet b) • Pi Mensae ( 59.4 ± 0.5 ly; 1 star, 1 planet: planet b)
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In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Italic are systems possibly located within declared distance interval, but probably not.
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Bayer |
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Flamsteed |
- 1 (κ, Al Minliar al Asad)
- 2 (ω)
- 3
- 4 (λ, Alterf)
- 5 (ξ)
- 6 (h)
- 7
- 8
- 9
- 10
- 11
- 12
- 13
- 14 (ο, Subra)
- 15 (f)
- 16 (ψ)
- 17 (ε, Algenubi)
- 18
- 19
- 20
- 21
- 22 (g)
- 23
- 24 (μ, Rasalas)
- 27 (ν)
- 29 (π)
- 30 (η)
- 31 (A)
- 32 (α, Regulus)
- 34
- 35
- 36 (ζ, Adhafera)
- 37
- 39
- 40
- 41 (γ, Algieba)
- 42
- 43
- 44
- 45
- 46
- 47 (ρ)
- 48
- 49
- 50
- 51 (m)
- 52 (k)
- 53 (l)
- 54
- 55
- 56
- 58 (d)
- 59 (c)
- 60 (b)
- 61 (p²)
- 62 (p³)
- 63 (χ)
- 64
- 65 (p4)
- 67
- 68 (δ, Zosma)
- 69 (p5)
- 70 (θ, Chertan)
- 71
- 72
- 73 (n)
- 74 (φ)
- 75
- 76
- 77 (σ)
- 78 (ι)
- 79
- 80
- 81
- 83
- 84 (τ)
- 85
- 86
- 87 (e)
- 88
- 89
- 90
- υ (91)
- 92
- 93
- 94 (β, Denebola)
- 95
- 18 LMi
- 37 Sex
- 52 LMi
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Nearby |
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Other |
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