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Located in the Milky Way's extreme outer halo, far beyond the galactic disc. [6] Oldest star 2MASS J18082002−5104378: 2018 13.53 billion years [7] [8] List of oldest stars: Youngest Stars are being formed constantly in the universe so it is impossible to tell which star is the youngest.
The Sagittarius A* cluster is the cluster of stars in close orbit around Sagittarius A*, the supermassive black hole at the center of the Milky Way (in the Galactic Center). The individual stars are often listed as "S-stars", but their names and IDs are not formalized, and stars can have different numbers in different catalogues.
The disk of stars in the Milky Way does not have a sharp edge beyond which there are no stars. Rather, the concentration of stars decreases with distance from the center of the Milky Way. Beyond a radius of roughly 40,000 light years (13 kpc) from the center, the number of stars per cubic parsec drops much faster with radius. [120]
Sh2-310 is also host to the stars Tau Canis Majoris [35] which is the brightest member of NGC 2362, [36] UW Canis Majoris and HD 58011 [35] which along with VY Canis Majoris [37] are thought to be probable sources of ionization of gases in Sh2-310. [35] Sh2-310 itself is located on the outer edge of the Orion Arm of the Milky Way. [32]
The Gaia Sausage or Gaia Enceladus is the remains of a dwarf galaxy (the Sausage Galaxy, or Gaia-Enceladus-Sausage, or Gaia-Sausage-Enceladus) that merged with the Milky Way about 8–11 billion years ago. At least eight globular clusters were added to the Milky Way along with 50 billion solar masses of stars, gas and dark matter. [1]
The Orion OB1 association occupies a large portion of a spiral arm of the Milky Way and contains many of the brighter stars of the constellation Orion. About 1 in 800 (0.125%) of the main-sequence stars in the solar neighborhood are B-type main-sequence stars .
Stars that are at least sometimes visible to the unaided eye have their apparent magnitude (6.5 or brighter) highlighted in blue. The first list gives stars that are estimated to be 60 M ☉ or larger; the majority of which are shown. The second list includes some notable stars which are below 60 M ☉ for the purpose of comparison. The method ...
The Milky Way Galaxy.. The Monoceros Ring (from Greek monoceros 'unicorn') is a long, complex ring of stars that wraps around the Milky Way three times. This is proposed to consist of a stellar stream torn from the Canis Major Dwarf Galaxy by tidal forces as part of the process of merging with the Milky Way over a period of billions of years, although this view has long been disputed. [1]
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