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  2. Sagittarius A* - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_A*

    Sagittarius A*, abbreviated as Sgr A* (/ ˈ s æ dʒ ˈ eɪ s t ɑːr / SADGE-AY-star [3]), is the supermassive black hole [4] [5] [6] at the Galactic Center of the Milky Way.Viewed from Earth, it is located near the border of the constellations Sagittarius and Scorpius, about 5.6° south of the ecliptic, [7] visually close to the Butterfly Cluster (M6) and Lambda Scorpii.

  3. Sagittarius A* cluster - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_A*_cluster

    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 .

  4. Sagittarius A - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_A

    Sagittarius A (Sgr A) is a complex radio source at the center of the Milky Way, which contains a supermassive black hole. It is located between Scorpius and Sagittarius , and is hidden from view at optical wavelengths by large clouds of cosmic dust in the spiral arms of the Milky Way.

  5. Andrea M. Ghez - Wikipedia

    en.wikipedia.org/wiki/Andrea_M._Ghez

    Andrea Mia Ghez (born June 16, 1965) is an American astrophysicist, Nobel laureate, and professor in the Department of Physics and Astronomy and the Lauren B. Leichtman & Arthur E. Levine chair in Astrophysics, at the University of California, Los Angeles. [1]

  6. V4641 Sagittarii - Wikipedia

    en.wikipedia.org/wiki/V4641_Sagittarii

    V4641 Sagittarii is a variable X-ray binary star system in the constellation Sagittarius.It is the source of one of the fastest superluminal jets in the Milky Way galaxy.. In 1999 a violent X-ray outburst revealed it to contain a black hole. [6]

  7. S62 (star) - Wikipedia

    en.wikipedia.org/wiki/S62_(star)

    S62 is a star in the cluster surrounding Sagittarius A* (Sgr A*), the supermassive black hole in the center of the Milky Way.S62 was initially thought to orbit extremely close to Sgr A*, with a period of 9.9 years and a closest approach of only 16 astronomical units (2.4 × 10 9 km), less than the distance between Uranus and the Sun.

  8. S4716 - Wikipedia

    en.wikipedia.org/wiki/S4716

    It orbits the Sgr A* in 4.0 years, on an elliptical orbit with an eccentricity of 0.75. Its closest approach to Sgr A* is 15 billion kilometers (about the distance to the space probe Voyager 2 in 2022, or three times the distance of Neptune from the Sun), while its farthest approach is 100 billion kilometers.

  9. Scutum–Centaurus Arm - Wikipedia

    en.wikipedia.org/wiki/Scutum–Centaurus_Arm

    The Scutum–Centaurus Arm lies between the minor Carina–Sagittarius Arm and the minor Norma Arm. The Scutum–Centaurus Arm starts near the core as the Scutum Arm, then gradually turns into the Centaurus Arm. [5] The region where the Scutum–Centaurus Arm connects to the bar of the galaxy is rich in star-forming regions and open clusters.