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Lambda Crucis information


λ Crucis
Location of λ Crucis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Crux
Right ascension 12h 54m 39.18258s[1]
Declination −59° 08′ 48.1229″[1]
Apparent magnitude (V) 4.62[2]
Characteristics
Evolutionary stage main sequence
Spectral type B4 Vne[3]
U−B color index −0.60[4]
B−V color index −0.15[4]
Variable type β Cep?[2]
Astrometry
Radial velocity (Rv)+12.0±4.2[5] km/s
Proper motion (μ) RA: −32.92[1] mas/yr
Dec.: −14.60[1] mas/yr
Parallax (π)8.50 ± 0.21 mas[1]
Distance384 ± 9 ly
(118 ± 3 pc)
Absolute magnitude (MV)−1.2[6]
Details
Mass5.0±0.1[7] M
Radius3.00[8] R
Luminosity790[6] L
Surface gravity (log g)3.01[8] cgs
Temperature16,500[8] K
Rotational velocity (v sin i)290[8] km/s
Age53.3±8.1[7] Myr
Other designations
λ Cru, Lambda Cru, CD−58°4794, HD 112078, HIP 63007, HR 4897, SAO 240368[9]
Database references
SIMBADdata

λ Crucis, Latinized as Lambda Crucis, is a single,[10] variable star in the southern constellation Crux, near the constellation border with Centaurus. It is visible to the naked eye as a faint, blue-white hued point of light with an apparent visual magnitude that fluctuates around 4.62.[2] The star is located approximately 384 light-years distant from the Sun based on parallax, and is drifting further away with a radial velocity of +12 km/s.[5] It is a proper motion member of the Lower Centaurus–Crux sub-group in the Scorpius–Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.[6]

A light curve for Lambda Crucis, plotted from Hipparcos data[11]

λ Crucis is listed in the General Catalogue of Variable Stars as a possible β Cephei-type variable. Its brightness varies with an amplitude of 0m.02 over a period of 0.3951 days.[2] However, it is currently thought more likely to be a different type of variable,[12] possibly a λ Eridani variable or rotating ellipsoidal variable.[13][14]

This object is a B-type main-sequence star with a stellar classification of B4 Vne,[3] where the suffix notation indicates "nebulous" (broad) lines due to rapid rotation, along with emission lines from circumstellar material, making it a Be star.[13] It is around 53[7] million years old and is spinning rapidly with a projected rotational velocity of 341 km/s.[15] The star has five[7] times the mass of the Sun and about 3.0[8] times the Sun's radius. It is radiating 790[6] times the luminosity of the Sun from its photosphere at an effective temperature of 16,500 K.[8]

  1. ^ a b c d e 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 Samus2017 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Levenhagen2006 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference clpl4 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference rgcrv66 was invoked but never defined (see the help page).
  6. ^ a b c d Cite error: The named reference aaa216_1_44 was invoked but never defined (see the help page).
  7. ^ a b c d Cite error: The named reference mnras410_1_190 was invoked but never defined (see the help page).
  8. ^ a b c d e f Cite error: The named reference arcos was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference Rizzuto2013 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference HIPCurve was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference stankov was invoked but never defined (see the help page).
  13. ^ a b Cite error: The named reference balona was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference morris was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference uesugi_fukuda70 was invoked but never defined (see the help page).

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Lambda Crucis

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λ Crucis, Latinized as Lambda Crucis, is a single, variable star in the southern constellation Crux, near the constellation border with Centaurus. It is...

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moderately common. The K0 RGB star Arcturus is 36 light-years away, and Gamma Crucis is the nearest M-class giant at 88 light-years' distance. A red giant will...

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Archived from the original on 2020-10-08 – via IanRidpath.com. "Gacrux/Gamma Crucis 2?". Sol Station. Sol Company. Archived from the original on 2011-11-03...

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Beta Eridani Star 2.79 2.76 Cor Caroli Binary star system 2.79 2.78 Delta Crucis Star 2.79 Epsilon Virginis Star 2.79 Beta Hydri Star 2.800 Zeta Herculis...

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Miller, Nathan A. (June 2008). "Chandra spectroscopy of the hot star beta Crucis and the discovery of a pre-main-sequence companion". Monthly Notices of...

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1980 of Orion complex 23.1 1,340 2.77 combined 32,500 evolution SIMBAD κ Crucis Jewel Box Cluster of Centaurus OB1 23 7,500 5.98 16,300 evolution SIMBAD...

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2.96 α Volantis 4.00 Acubens A α Cancri A 4.26 Kurhah ξ Cephei 4.29 θ1 Crucis 4.30 π Virginis 4.64 μ Aurigae 4.88 2 Ursae Majoris 5.46 τ3 Gruis 5.72 WW...

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Astronomical naming conventions

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Alpha Centauri (α Cen), in the constellation Centaurus, Alpha Crucis (α Cru) and Beta Crucis (β Cru), the two brightest stars in the constellation Crux,...

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Hypergiant

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occasionally late O or early A: 2dFS 3235 AzV 2 AzV 65 AzV 76 AzV 78 AzV 367 BP Crucis (Wray 977 or GX 301-2), binary with a pulsar companion. Cygnus OB2-12 HD...

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Musca

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state in Brazil called Alpha and Beta Muscae (along with Beta and Kappa Crucis) Kutsu anangagï "Ornate Hawk-Eagle's double flutes". The Wardaman people...

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Hearnshaw, J. B. (1992-01-01). "The radial-velocity variability of gamma Crucis". Monthly Notices of the Royal Astronomical Society. 254: 27–29. Bibcode:1992MNRAS...

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ISSN 0004-6361. S2CID 15874925. Murdin, P.; Penston, M. V. (1977-12-01). "The Lambda Orionis association". Monthly Notices of the Royal Astronomical Society...

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Bardi people

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went to the Coalsack Nebula, and his presence may be represented by BZ Crucis. Galalaṇ (perhaps "belonging to the long-ago"), was the primordial figure...

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