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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 ...

  3. 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]

  4. AOL Mail

    mail.aol.com

    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  5. 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.

  6. Xi Sagittarii - Wikipedia

    en.wikipedia.org/wiki/Xi_Sagittarii

    The Bayer designation Xi Sagittarii (ξ Sagittarii) is shared by two stars, ξ 1 Sagittarii and ξ² Sagittarii, in the constellation Sagittarius, separated by 0.46° in the sky.

  7. 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.

  8. HD 165185 - Wikipedia

    en.wikipedia.org/wiki/HD_165185

    Based upon the motion of this star through space, its age, and properties, this star is a probable member of the Ursa Major Moving Group; a stellar kinematic group that formed in the same region of space. [11] It has a suspected common proper motion companion at an angular separation of 12″, corresponding to a projected separation of 220 AU.

  9. Fix problems signing into your AOL account - AOL Help

    help.aol.com/articles/help-signing-in

    To manage and recover your account if you forget your password or username, make sure you have access to the recovery phone number or alternate email address you've added to your AOL account. If you know your username but need to reset your password, make sure you create a strong password after you're back in your account.