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ɒ n /) [17] is the brightest star in the constellation of Canis Minor and usually the eighth-brightest star in the night sky, with an apparent visual magnitude of 0.34. [3] It has the Bayer designation α Canis Minoris, which is Latinized to Alpha Canis Minoris, and abbreviated α CMi or Alpha CMi, respectively.
Polynesian peoples often did not recognize Canis Minor as a constellation, but they saw Procyon as significant and often named it; in the Tuamotu Archipelago it was known as Hiro, meaning "twist as a thread of coconut fiber", and Kopu-nui-o-Hiro ("great paunch of Hiro"), which was either a name for the modern figure of Canis Minor or an ...
HD 66141 is a single [8] star in the equatorial constellation of Canis Minor.It has the Bayer designation G Canis Minoris, [6] the Gould designation 50 G. Canis Minoris, [7] and has the HR 3145 identifier from the Bright Star Catalogue. [6]
Gamma Canis Minoris (γ Canis Minoris) is a binary star system in the equatorial constellation Canis Minor. Its orange colour is obvious when seen through binoculars. [ 7 ] The system is visible to the naked eye with a combined apparent visual magnitude of +4.33. [ 2 ]
Demodicosis is most often seen in folliculitis (inflammation of the hair follicles of the skin). Depending on the location, it may result in small pustules (pimples) at the base of a hair shaft on inflamed, congested skin. Demodicosis may also cause itching, swelling, and erythema of the eyelid margins. Scales at the base of the eyelashes may ...
Includes Canis Minor and the obsolete constellation Printer's Workshop In Western astronomy, Monoceros is a relatively modern constellation, not one of Ptolemy 's 48 in the Almagest . [ 9 ] Its first certain appearance was on a globe created by the cartographer Petrus Plancius in 1612 or 1613 [ 10 ] and it was later charted by German astronomer ...
The primary component, η Canis Minoris A, is a yellow-white F-type giant with an apparent magnitude of +5.24. Its companion, η Canis Minoris B , is an eleventh-magnitude star located 4 arcseconds from the primary, though is actually around 440 AU from the main star and takes around 5,000 years to orbit it.
BG Canis Minoris is a binary star system in the equatorial constellation of Canis Minor, abbreviated BG CMi. With an apparent visual magnitude that fluctuates around 14.5, [3] it is much too faint to be visible to the naked eye. Parallax measurements provide a distance estimate of approximately 2,910 light years from the Sun. [2]