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Cody Rhodes / Stardust / Cody Goldust / Dustin Rhodes: Name(s) The Brotherhood Cody Rhodes and Goldust Gold and Stardust [1] The Rhodes Brothers Cody and Dustin Rhodes [2] Billed heights: Cody: 6 ft 2 in (1.88 m) [3] Dustin: 6 ft 6 in (1.98 m) [4] Combined billed weight: 452 lb (205 kg) [3] [4] Debut: October 6, 2013: Disbanded: 2020: Years ...
Owl Cluster, E.T. Cluster: Open Cluster - Cassiopeia: 6.4 C14 NGC 869 & NGC 884: Double Cluster, h & χ Persei: Open Cluster: 7.3 Perseus: 4 C15 NGC 6826: Blinking Planetary: Planetary Nebula: 2.2 Cygnus: 10 C16 NGC 7243 Open Cluster: 2.5 Lacerta: 6.4 C17 NGC 147 Dwarf Spheroidal Galaxy: 2,300 Cassiopeia: 9.3 C18 NGC 185 Dwarf Spheroidal Galaxy ...
NGC 1850 is a double cluster and a super star cluster in the Dorado constellation, located in the northwest part [3] of the bar of the Large Magellanic Cloud, [4] at a distance of 168 kly (51.5 kpc) from the Sun. [citation needed] It was discovered by Scottish astronomer James Dunlop in 1826.
The Jewel Box (also known as the Kappa Crucis cluster, NGC 4755, or Caldwell 94) is an open cluster in the constellation Crux, originally discovered by Nicolas Louis de Lacaille in 1751–1752. [4] This cluster was later named the Jewel Box by John Herschel when he described its telescopic appearance as "... a superb piece of fancy jewellery".
The GC contained 5,079 entries. Later, a complementary edition of the catalog was published posthumously as the General Catalogue of 10,300 Multiple and Double Stars. The small "h" followed with the catalogue entry number represented the item. [4] In 1878, John Louis Emil Dreyer published a supplement to the General Catalogue. [6]
Pandora's Cluster: Sculptor: 00 h 14 m 19.5 s: −30° 23′ 19″ 3 III It seems to have formed from four different clusters involved in a series of collisions over a period of some 350 million years. [6] 3128: Shapley 20 Cluster: 03 h 30 m 34.6 s: −52° 33′ 12″ 3 I-II 3158: Shapley 17 Cluster: 03 h 42 m 39.6 s: −53° 37′ 50″ 2 I ...
The Double Cluster in Perseus (lower left of center, wide angle view) Greek astronomer Hipparchus cataloged the object (a patch of light in Perseus) as early as 130 BCE. To Bedouin Arabs the cluster marked the tail of the smaller of two fish they visualized in this area, and it was shown on illustrations in Abd al-Rahman al-Sufi's Book of Fixed Stars. [4]
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 ...