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epsilon canis majoris distance from earth

The Variable Type is usually named after the first star of that type to be spotted. If the R.A. is positive then its eastwards.

If you used the 1997 Parallax value, you would get an absolute magnitude of -5.02 If you used the 2007 Parallax value, you would get an absolute magnitude of -9.40. Answer. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. Top Answer.

A name is preferred even if its a random made up one by yourself. And the following 10 interesting facts Adhara star: Search Terms: Adhara Star, Canis Majoris Distance From Earth, Canis Major Constellation Facts, Canis Majoris Facts, Canis Major Facts, Adara Star. In the case of a star, its the galactic centre.

Proper Motion details the movements of these stars and are measured in milliarcseconds. The star has a B-V Colour Index of 1.74 which means the star's temperature is about 3,298 Kelvin. Astronomy Science ~ Adhara or Epsilon Canis Majoris (ε CMa, ε Canis Majoris) is the second brightest star in the constellation Canis Major, and one of the brightest star in the night sky. 2010-05-10 07:28:30 2010-05-10 07:28:30. VY Canis Majoris is a red hypergiant with a radius of around 1,500 times larger than the sun. Canis Major has done some calculations as to how long it will take going at differing speeds. Based on the star's spectral type of K3Iab , Omicron1 Canis Majoris's colour and type is orange to red supergiant star.

The Declination is how far north or south the object is compared to the celestial equator and is expressed in degrees. The figure is derived at by using the formula from Omicron1 Canis Majoris Iron Abundance is -0.10 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. Adhara - ε Canis Majoris (epsilon Canis Majoris) Adhara, also designated as ε Canis Majoris (epsilon Canis Majoris), is a double bright giant star in the constellation of Canis Major. The star is a pulsating Slow Irregular variable type which means that its size changes over time. is the number of times that the star is from the Earth compared to the Sun. In the second century, it was included in Ptolemy's 48 constellations, and is counted among the 88 modern constellations. Epsilon Canis Majoris is a binary star system consisting of Epsilon Canis Majoris A, a bright giant, and Epsilon Canis Majoris B, a faint companion at a separation of 7.5 arcseconds from the primary.
Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. 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.

It should not be taken as though the star is moving closer or further away from us. If you need the diameter of the star, you just need to multiple the radius by 2. The Milky Way passes through Canis Major and several open clusters lie within its borders, most notably M41.

When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. The Sun's radius is 695,800km, therefore the star's radius is an estimated 200,879,589.22.km.
For Omicron1 Canis Majoris, the location is 06h 54m 07.95 and -24° 11` 03.2 . U.G. Apparent Magnitude is also known as Visual Magnitude. If you want that in miles, it is about 11,620,572,706,440,701.07, based on 1 Ly = 5,878,625,373,183.61 miles.In 2007, Hipparcos data was revised with a new parallax of 0.22000 which put Omicron1 Canis Majoris at a distance of 14825.61 light years or 4545.45 parsecs. Omicron1 Canis Majoris brightness ranges from a magnitude of 4.200 to a magnitude of 3.939 over its variable period. The designations of the two components as ε Canis Majoris A and B derive from the convention used by the Washington Multiplicity Catalog for multiple star systems, and adopted by the International Astronomical Union. All messages will be reviewed before being displayed. Comments may be merged or altered slightly such as if an email address is given in the main body of the comment.You can decline to give a name which if that is the case, the comment will be attributed to a random star. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 2170.1731601636002937279401678.

ε Canis Majoris bore the traditional name Adhara, derived from the Arabic word عذارى ‘aðāra’, "virgins". How far is the star Epsilon from the Earth? The value comes from the Hipparcos Extended Catalog.

Wiki User. Canis Major is a constellation in the southern celestial hemisphere. The temperature was calculated using information from Omicron1 Canis Majoris estimated radius has been calculated as being 288.70 times bigger than the Sun.

Even though the angular distance between the components is considerable, the two stars can only be resolved in large instruments because Epsilon CMa A is about 250 times brighter than Epsilon CMa B. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. The smaller the magnitude, the brighter the star. VY Canis Majoris is around 4,000 light years from Earth in the constellation of Canis Major. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever. ε Canis Majoris is the binary system's Bayer designation.

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