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The Sagittarius Dwarf Spheroidal Galaxy (Sgr dSph), also known as the Sagittarius Dwarf Elliptical Galaxy (Sgr dE or Sag DEG), is an elliptical loop-shaped satellite galaxy of the Milky Way. It contains four globular clusters in its main body, [8] with the brightest of them — NGC 6715 (M54) — known well before the discovery of the galaxy ...
Nearest galaxy to the Milky Way Sagittarius Dwarf Spheroidal Galaxy: 1994 0.070 Mly The closest, undisputed galaxy. The disputed dwarf galaxy Canis Major Overdensity is even closer at 25,000 light-years. [citation needed] Nearest dwarf galaxy Sagittarius Dwarf Spheroidal Galaxy: 1994 0.070 Mly Nearest major galaxy to the Milky Way Andromeda ...
Previously thought to belong to the Milky Way at a distance from Earth of about 50,000 light-years, it was discovered in 1994 that M54 most likely belongs to the Sagittarius Dwarf Elliptical Galaxy (SagDEG), [9] making it the first globular cluster formerly thought to be part of our galaxy reassigned to extragalactic status, even if not ...
Sagittarius Dwarf Galaxy may refer to: The Sagittarius Dwarf Spheroidal Galaxy (also known as the Sagittarius Dwarf Elliptical Galaxy), a satellite galaxy of the Milky Way; The Sagittarius Dwarf Irregular Galaxy, a small member of the Local Group
Pages in category "Sagittarius Dwarf Spheroidal Galaxy" The following 5 pages are in this category, out of 5 total. This list may not reflect recent changes. ...
Terzan 7 is a sparse and young globular cluster that is believed to have originated in the Sagittarius Dwarf Spheroidal Galaxy (Sag DEG) and is physically associated with it. It is relatively metal rich with [Fe/H] = -0.6 [6] and an estimated age of 7.5 Gyr. [4]
Sagittarius contains two well-known star clouds, both considered fine binocular objects. The Large Sagittarius Star Cloud is the brightest visible region of the Milky Way. It is a portion of the central bulge of the galaxy seen around the thick dust of the Great Rift, and is the innermost galactic structure that can be observed in visible ...
Segue 2 is a dwarf spheroidal galaxy situated in the constellation Aries and discovered in 2009 in the data obtained by Sloan Digital Sky Survey.The galaxy is located at the distance of about 35 kiloparsecs (35,000 parsecs; 110,000 light-years) from the Sun and moves towards the Sun at a speed of 40 kilometres per second (25 mi/s).