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  2. Messier 69 - Wikipedia

    en.wikipedia.org/wiki/Messier_69

    Messier 69 or M69, also known NGC 6637, and NGC 6634, [9] [10] is a globular cluster in the southern constellation of Sagittarius. [a] It can be found 2.5° to the northeast of the star Epsilon Sagittarii and is dimly visible in 50 mm aperture binoculars. The cluster was discovered by Charles Messier on August 31, 1780, the same night he ...

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  4. Sagittarius A* cluster - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_A*_cluster

    One of the most studied stars is S2, a relatively bright star that also passes close by Sgr A*. As of 2020 [update] , S4714 is the current record holder of closest approach to Sagittarius A*, at about 12.6 astronomical units (1.88 × 10 9 km), almost as close as Saturn gets to the Sun, traveling at about 8% of the speed of light.

  5. NGC 6530 - Wikipedia

    en.wikipedia.org/wiki/NGC_6530

    NGC 6530 is a young [8] open cluster of stars in the southern constellation of Sagittarius, located some 4,300 light years from the Sun. [3] It exists within the H II region known as the Lagoon Nebula, or Messier 8, [9] and spans an angular diameter of 14.0′. [5]

  6. V1017 Sagittarii - Wikipedia

    en.wikipedia.org/wiki/V1017_Sagittarii

    V1017 Sagittarii is a cataclysmic variable star system in the constellation Sagittarius. It first erupted in 1919, reaching magnitude 7. It first erupted in 1919, reaching magnitude 7. Its other eruptions in 1901, 1973 and 1991 only reached magnitude 10, leading it to be reclassified from a recurrent nova to a dwarf nova .

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  8. Rho Sagittarii - Wikipedia

    en.wikipedia.org/wiki/Rho_Sagittarii

    The Bayer designation Rho Sagittarii (Rho Sgr, ρ Sagittarii, ρ Sgr) is shared by two stars in the constellation Sagittarius.. ρ 1 Sagittarii [1]; ρ 2 Sagittarii [2]; The two stars are separated by 0.46° in the sky.

  9. Chi1 Sagittarii - Wikipedia

    en.wikipedia.org/wiki/Chi1_Sagittarii

    This is a visual binary with an orbital period of 5.72 years, an eccentricity of 0.710, and an angular semimajor axis of 69 mas. The primary, component A, is an A-type star showing a mixed spectrum that matches a stellar classification of A3/5 IV/V. [ 3 ] Helmut Abt classified it as an Am star with a spectral type of kA5hF0VmF0. [ 11 ]

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