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Theta2 OrionisTheta2 Orionis BS490 B She and Theta2 Orionis are best friends, as is the whole system. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Apparent Magnitude is also known as Visual Magnitude. Using the original Hipparcos data that was released in 1997, the parallax to the star was given as -2.00000 which gave the calculated distance to Theta1 Orionis C as -1630.82 light years away from Earth or -500 parsecs. The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point.
A name is preferred even if its a random made up one by yourself. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator.
The source of the info is Simbad. Theta2 Orionis C
You can decline to give a name which if that is the case, the comment will be attributed to a random star. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
Theta2 Orionis C is a blue-white star, she is part of a multi-star system, but her binary partner is S490 B, for she also has the name S490, and her partner is between her sister Theta2 Orionis B, and her brother V1073 Orionis. Theta1 Orionis C is a O6PE multiple star system based on the spectral type that was recorded in the Michigan Catalogue of Two-Dimensional Spectral Types for the HD stars, Vol. 5. Theta1 Orionis C is a Multiple Star System type star. This star is amongst the hottest stars in the Universe. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.
Simple Cosmos Official Wiki is a FANDOM Lifestyle Community. The star C is the most massive of the four bright stars at the heart of the cluster. If the R.A. is positive then its eastwards. Female Cookies / About Us / Contact Us / Twitter / Facebook, HD 37022, HIP 26221, HR 1895, TYC 4774-931-1, 41 Orionis C, 41 Ori C, 05 1315.
La dernière modification de cette page a été faite le 1 août 2018 à 22:17. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. All messages will be reviewed before being displayed. Theta2 Orionis C is a blue-white star, she is part of a multi-star system, but her binary partner is S490 B, for she also has the name S490, and her partner is between her sister Theta2 Orionis B, and her brother V1073 Orionis. If you want that in miles, it is about -9,586,979,831,095,294.86, based on 1 Ly = 5,878,625,373,183.61 miles. The source of the information if it has a Hip I.D. (Theta1 Orionis C) is the Bayer Classification for the star.
The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star.
The information was obtained as of 12th Feb 2017. θ 1 Orionis, l'amas du Trapèze, amas ouvert d'étoiles, l'association OB d'Orion 1d . The location of the multiple star system in the night sky is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. The Declination is how far north or south the object is compared to the celestial equator and is expressed in degrees. The Bayer Classification was created by Johann Bayer in 1603. Theta Orionis (tet Ori, θ Ori), Thêta d'Orion en français, est le nom de plusieurs objets astronomiques situés autour de 05h 35,3m d'ascension droite et -05° 24′ de déclinaison : L'ensemble d'objets θ Orionis sont situés à l'intérieur de la nébuleuse NGC 1977. Take your favorite fandoms with you and never miss a beat.
Using the supplied Parallax value, you would get an absolute magnitude of Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Parent Objects Based on the spectral type (O6pe) of the star, the star's colour is blue - white.
Type of Star None Poor Relationships
Dernière modification le 1 août 2018, à 22:17, système d'étoiles binaire spectroscopique, https://fr.wikipedia.org/w/index.php?title=Theta_Orionis&oldid=150897924, licence Creative Commons attribution, partage dans les mêmes conditions, comment citer les auteurs et mentionner la licence.
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