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CW Leonis information


CW Leonis

CW Leonis in ultraviolet showing the bowshock
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 09h 47m 57.406s[1]
Declination +13° 16′ 43.56″[1]
Apparent magnitude (V) 14.5 (var.)[2]
Characteristics
Spectral type C9,5e[3]
Apparent magnitude (R) 10.96[1]
Apparent magnitude (J) 7.34[1]
Apparent magnitude (H) 4.04[1]
Apparent magnitude (K) 1.19[1]
Variable type Mira[4]
Astrometry
Proper motion (μ) RA: 35±1 mas/yr
Dec.: 12±1[5] mas/yr
Parallax (π)10.56 ± 2.02 mas[6]
Distanceapprox. 310 ly
(approx. 90 pc)
Details
Mass0.7 - 0.9[5] M
Radius560[7] R
Luminosity8,500 (average), 11,850 (maximum)[7] L
Temperature2,300[7] (1,915 - 2,105)[8] K
Other designations
CW Leo, Peanut Nebula, IRC+10216, IRAS 09452+1330, PK 221+45 1, Zel 0945+135, RAFGL 1381, 2MASS J09475740+1316435, SCM 50[9]
Database references
SIMBADdata

CW Leonis or IRC +10216 is a variable carbon star that is embedded in a thick dust envelope. It was first discovered in 1969 by a group of astronomers led by Eric Becklin, based upon infrared observations made with the 62-inch Caltech Infrared Telescope at Mount Wilson Observatory. Its energy is emitted mostly at infrared wavelengths. At a wavelength of 5 μm, it was found to have the highest flux of any object outside the Solar System.[10]

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  5. ^ a b Cite error: The named reference matthews was invoked but never defined (see the help page).
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  7. ^ a b c Cite error: The named reference schmidt was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference bergeat 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 apj158_L133 was invoked but never defined (see the help page).

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CW Leonis

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CW Leonis or IRC +10216 is a variable carbon star that is embedded in a thick dust envelope. It was first discovered in 1969 by a group of astronomers...

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List of stars in Leo

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nearest star system; Proxima Leonis; flare star Caffau's Star 10h 29m 15.15s +17° 29′ 28″ 16.92 4469 Caffau's Star DP Leonis DP 11h 17m 16.00s +17° 57′ 41...

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CIT 6

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the variable star designation RW Leonis Minoris. It is perhaps the second most studied carbon star, after CW Leonis. CIT 6 was discovered in 1966 by a...

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Mira variable

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Giacobbe, P.; Lattanzi, M. G. (2017). "Evidence for orbital motion of CW Leonis from ground-based astrometry". Monthly Notices of the Royal Astronomical...

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Carbon star

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millimeter wavelengths and submillimeter wavelengths. In the carbon star CW Leonis more than 50 different circumstellar molecules have been detected. This...

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List of interstellar and circumstellar molecules

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subsequently detected there. A rich source of circumstellar molecules is CW Leonis (also known as IRC +10216), a nearby carbon star, where about 50 molecules...

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Water vapor

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evidence of atmospheric water vapor beyond the Solar System. A star called CW Leonis was found to have a ring of vast quantities of water vapor circling the...

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Nibiru cataclysm

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Another piece of claimed evidence drawn from Google Sky is the carbon star CW Leonis, which is the brightest object in the 10 μm infrared sky and has been...

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List of largest stars

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the largest known stars. 119 Tauri (CE Tauri, Ruby Star) 587 – 593 AD CW Leonis 560 L/Teff The nearest carbon star. V838 Monocerotis 364 L/Teff During...

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List of star extremes

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323 light-years (99 pc) List of nearest supergiants Nearest carbon star CW Leonis 310 light-years (95 pc) Nearest F-type star Procyon A 11.46 light-years...

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Mu Leonis

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Mu LeonisLeonis, abbreviated Mu Leo, μ Leo), also named Rasalas /ˈræsəlæs/, is a star in the constellation of Leo. The apparent visual magnitude of...

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Upsilon Leonis

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Upsilon Leonis (υ Leo) is a star in the zodiac constellation of Leo. It is visible to the naked eye with an apparent visual magnitude of 4.33. The distance...

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Omega Leonis

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ω Leonis (Latinised as Omega Leonis, abbreviated to ω Leo or Omega Leo), is a star system located in the zodiac constellation of Leo. It is visible to...

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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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Chi Leonis

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Chi Leonis, Latinized from χ Leonis, is a double star in the constellation Leo. It is visible to the naked eye with an apparent visual magnitude of 4...

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Lambda Leonis

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Lambda LeonisLeonis, abbreviated Lam Leo, λ Leo), formally named Alterf /ælˈtərf/, is a star in the constellation of Leo. The star is bright enough...

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88 Leonis

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88 Leonis is a wide binary star system in the equatorial constellation of Leo, the lion. The system is near the lower limit of visibility to the naked...

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Phi Leonis

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Phi Leonis (φ Leo) is a single star in the constellation Leo. It is bright enough to be seen with the naked eye, having an apparent visual magnitude of...

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Nu Leonis

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ν Leonis, Latinised as Nu Leonis, is a binary star system in the zodiac constellation of Leo. It is faintly visible to the naked eye with an apparent visual...

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89 Leonis

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89 Leonis is a single star in the equatorial constellation of Leo, the lion. It has a yellow-white hue and is faintly visible to the naked eye with an...

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Xi Leonis

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Xi Leonis (ξ Leo, ξ Leonis) is a solitary star in the zodiac constellation of Leo. It has an apparent visual magnitude of 5.0 and is faintly visible to...

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Psi Leonis

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ψ Leonis (Latinised as Psi Leonis, abbreviated to ψ Leo or psi Leo), is a solitary star located in the zodiac constellation of Leo, to the east-northeast...

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Pi Leonis

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Pi Leonis, Latinised from π Leonis, is a single star in the zodiac constellation Leo. It is a red-hued star that is visible to the naked eye with an apparent...

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Gliese 414

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direction of the constellation Ursa Major. The closest star to the star system is CW Ursae Majoris, at a distance of 5.3 light-years. The primary star, Gliese...

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Mysteries Decoded

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American television documentary series that premiered on January 10, 2019 on The CW. The show is hosted by Jennifer Marshall, a United States Navy veteran turned...

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Pucci, Douglas (May 15, 2018). "Live+7 Weekly Ratings: The Originals on CW More Than Doubles its Live Plus Same Day Figures in Delayed Viewing". Programming...

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