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Master of Orion: Conquer the Stars (also called simply Master of Orion) is a science fiction turn-based strategy 4X game. It is the fourth game in the Master of Orion series and a reboot of the series, developed by Argentina -based Nimble Giant Entertainment and published by Wargaming . [ 1 ]
Chi 2 Orionis (Chi 2 Ori / χ 2 Orionis / χ 2 Ori) / k aɪ. t uː ˈ ɒ r aɪ / is a B-type blue supergiant star in the constellation of Orion.It has an apparent visual magnitude of 4.63 but being quite distant, and heavily extinguished it burns with the greatest absolute visual light magnitude among stars in Orion within the near reaches of the galaxy, 0.9 of a magnitude brighter than Rigel.
In 2001, Star Lords, developed as Master of Orion prototype, was released as freeware as part of the promotion for Master of Orion III. Also a potential future release of the MOO and MOO2 source code was indicated by the MOO3 developers in 2001. [55] In 2011, a clone of MoO II, titled Starbase Orion, was published by Chimera Software, LLC for ...
The Trapezium or Orion Trapezium Cluster, also known by its Bayer designation of Theta 1 Orionis (θ 1 Orionis), is a tight open cluster of stars in the heart of the Orion Nebula, in the constellation of Orion. It was discovered by Galileo Galilei. On 4 February 1617 he sketched three of the stars (A, C and D), but missed the surrounding ...
• Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] See also [ edit ]
Pi 2 Orionis (π 2 Ori, π 2 Orionis) is the Bayer designation for a solitary star in the equatorial constellation of Orion. Although the Bright Star Catalogue lists this as a spectroscopic binary star system, [10] this does not appear to be the case. [11] It is visible to the naked eye with an apparent visual magnitude of 4.35. [2]
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θ 1 Orionis A is a star system with three known members. Components A1 and A2 are separated by around 0.2 " , while A1 is itself a spectroscopic binary with two stars separated by about 1 au . θ 1 Orionis A1 is an eclipsing binary but the secondary is not detected in the spectrum and is far less luminous than the primary.