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In 2016, the International Astronomical Union (IAU) organized a Working Group on Star Names (WGSN) [2] to catalog and standardize proper names for stars. The WGSN's first bulletin, dated July 2016, [3] included a table of 125 stars comprising the first two batches of names approved by the WGSN (on 30 June and 20 July 2016) together with names of stars adopted by the IAU Executive Committee ...
A multiple star system consists of two or more stars that appear from Earth to be close to one another in the sky. [dubious – discuss] This may result from the stars actually being physically close and gravitationally bound to each other, in which case it is a physical multiple star, or this closeness may be merely apparent, in which case it is an optical multiple star [a] Physical multiple ...
Grades [1] [2] [3] Post-nominal Title Wife's title Ribbon The Most Exalted Order of the Star of Sarawak Darjah Utama Yang Amat Mulia Bintang Sarawak: Knight Grand Commander: Satria Bintang Sarawak
A star is a luminous spheroid of plasma held together by self-gravity. [1] The nearest star to Earth is the Sun.Many other stars are visible to the naked eye at night; their immense distances from Earth make them appear as fixed points of light.
Recipients of the Bintang Republik Indonesia Adipradana wore the star on a ribbon which was worn around the neck. Both of Adipurna and Adipradana classes wore a breast star on the left chest. Recipients of the Bintang Republik Indonesia Utama, Pratama, and Nararya wore the star on a ribbon on the left chest; with rosette for the Pratama class. [4]
A B-type main-sequence star (B V) is a main-sequence (hydrogen-burning) star of spectral type B and luminosity class V. These stars have from 2 to 16 times the mass of the Sun and surface temperatures between 10,000 and 30,000 K. [1]
The Darjah Yang Amat Mulia Bintang Kenyalang Sarawak (Order of the Star of the Hornbill of Sarawak) is the second highest order group (in the group of orders) of the orders, decorations, and medals of Sarawak. The order was instituted in 1970, and was redesigned in 1988.
Gamma Centauri, Latinized from γ Centauri, is a binary star system in the southern constellation of Centaurus.It has the proper name Muhlifain, [10] not to be confused with Muliphein, which is γ Canis Majoris; both names derive from the same Arabic root.