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Choose the design that fits your site. Islamic scholar Abū Rayḥān al-Bīrūnī referred to Orion as Kalb al-Jabbār, "the Dog of the Giant".
[55] Mu is a multiple star system located around 1244 light-years distant,[56] its components discernible in a small telescope as a 5.3-magnitude yellow-hued and 7.1-magnitude bluish star.
The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it. It is bright because of its proximity to the Solar System. [90] NGC 2362 is a small, compact open cluster, 5200 light-years from Earth.
[69], Tau Canis Majoris is a Beta Lyrae-type eclipsing multiple star system that varies from magnitude 4.32 to 4.37 over 1.28 days. Also called Mirzam or Murzim, Beta is a blue-white Beta Cephei variable star of magnitude 2.0, which varies by a few hundredths of a magnitude over a period of six hours. For other uses, see, The IUE Mega Campaign: Wind Structure and Variability of HD 50896 (WN5), Journal of the British Astronomical Association, "Al Achsasi Al Mouakket, on a Catalogue of Stars in the Calendarium of", Monthly Notices of the Royal Astronomical Society, "Empirical Luminosities and Radii of Early-Type Stars after Hipparcos", "A systematic study of variability among OB-stars based on HIPPARCOS photometry", "Observations and Analysis of the System R Canis Majoris", "Distant World in Peril Discovered from La Silla: Giant Exoplanet Orbits Giant Star", "The HARPS Search for Southern Extra-solar Planets XVI.
[5] Among the Merazig of Tunisia, shepherds note six constellations that mark the passage of the dry, hot season. Its outer envelope is beginning to expand and cool, and in the next 100,000 years it will become a red supergiant as its core fuses heavier and heavier elements.
[42] With a traditional name meaning "the weight", Wezen is 17 times as massive and 50,000 times as luminous as the Sun.
Add new content to your site from Sensagent by XML. | [47] It is a spectroscopic binary, whose components orbit each other every 1.85 years, the combined spectrum indicating a main star of spectral type B2.5V. Parent Objects Star data and search provided by About The Stars. Located 4 degrees south of Sirius, it contains contrasting blue, yellow and orange stars and covers an area the apparent size of the full moon—in reality around 25 light-years in diameter.
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8 Planetary Companions to Low-activity Solar-type Stars", The Deep Photographic Guide to the Constellations: Canis Major, Warburg Institute Iconographic Database (over 160 medieval and early modern images of Canis maior), https://en.wikipedia.org/w/index.php?title=Canis_Major&oldid=983078305, Articles containing Chinese-language text, Articles containing Tuamotuan-language text, Articles containing Wergaia-language text, Creative Commons Attribution-ShareAlike License, This page was last edited on 12 October 2020, at 03:19.
Kappa Canis Majoris (κ CMa / 13 Canis Majoris / HD 50013) ye una estrella na constelación del Can Mayor de magnitú aparente +3,51. ; Chesneau, O.; Jones, C. (October 2009), "VLTI/MIDI observations of 7 classical Be stars", an offensive content(racist, pornographic, injurious, etc.
Also called Mirzam or Murzim, Beta is a blue-white Beta Cephei variable star of magnitude 2.0, which varies by a few hundredths of a magnitude over a period of six hours. Letters must be adjacent and longer words score better. Cookies / About Us / Contact Us / Twitter / Facebook, Kap Cma, HD 50013, HIP 32759, HR 2538, TYC 7092-2576-1, 13 Canis Majoris, 13 Cma, CD-32 3404, kap CMa, Variable Magnitude Range (Brighter - Dimmer). Using the most recent figures given by the 2007 Hipparcos data, the star is 658.92 light years away from us. The red hypergiant VY Canis Majoris is one of the largest stars known, while the neutron star RX J0720.4-3125 has a radius of a mere 5 km. It is approximately 790 light years from Earth. situated south of the celestial equator, as such, it is more easily visible from the southern emisphere.
[6] The star marked the Great Dog's mouth on Bayer's star atlas. Its name is Latin for "greater dog" in contrast to Canis Minor, the "lesser dog"; both figures are commonly represented as following the constellation of Orion the hunter through the sky.
[6] Furthermore, two other stars are thought to have previously outshone all others in the night sky—Adhara (Epsilon Canis Majoris) shone at −3.99 around 4.7 million years ago, and Mirzam (Beta Canis Majoris) peaked at −3.65 around 4.42 million years ago. Sirius was the basis for the ancient Egyptian calendar. For Kappa Canis Majoris, the location is 06h 49m 50.47 and -32° 30` 30.6 .
Although of similar spectra and nearby each other as viewed from Earth, they are unrelated.
The Sun's radius is 695,800km, therefore the star's radius is an estimated 7,254,788.04.km. [45] Classified as an Alpha Cygni type variable star, Aludra varies in brightness from magnitude 2.38 to 2.48 over a period of 4.7 days. 3.4 – 3.97), and 27 Canis Majoris (mag. The items in red are values that I've calculated so they could well be wrong.
Meilland, A.; Stee, Ph. The brightest is a 6.3-magnitude star of spectral type K3. The New Horizons space probe is the fastest probe that we've sent into space at the time of writing. It is a blue-white supergiant of spectral type B2Iab, around 404 light-years from Earth.
[45] Classified as an Alpha Cygni type variable star, Aludra varies in brightness from magnitude 2.38 to 2.48 over a period of 4.7 days. [18][19] The Tuamotu people called Canis Major Muihanga-hetika-o-Takurua, "the abiding assemblage of Takarua".
EZ Canis Majoris is a Wolf–Rayet star of spectral type WN4 that varies between magnitudes 6.71 and 6.95 over a period of 3.766 days; the cause of its variability is unknown but thought to be related to its stellar wind and rotation. Privacy policy
Its traditional name means "the virgins", having been transferred from the group of stars to Epsilon alone.
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