ᱛᱳᱣᱟ ᱰᱟᱦᱟᱨ ᱥᱮ (en;Milky Way/hi;आकाशगंगा) ᱫᱚ ᱢᱤᱫ ᱜᱮᱞᱟᱠᱥᱤ (Galaxy) ᱠᱟᱱᱟ ᱾ ᱥᱤᱧ ᱪᱟᱸᱫᱚ ᱢᱟᱱᱰᱮᱨ ᱨᱮᱱᱟᱜ ᱛᱟᱞᱟ ᱥᱤᱧ ᱪᱟᱸᱫᱚ ᱫᱚ ᱱᱚᱶᱟ ᱜᱮᱞᱟᱠᱥᱤ ᱨᱮᱱᱟᱜ ᱜᱮ ᱢᱤᱫ ᱯᱟᱦᱟᱴᱟ ᱠᱟᱱᱟ ᱾ ᱢᱮᱱᱮᱫ ᱟᱵᱚ ᱦᱚ ᱱᱚᱶᱟ ᱜᱮᱞᱟᱠᱥᱤ ᱨᱮᱜᱮ ᱵᱚ ᱛᱟᱦᱮᱱ ᱠᱟᱱᱟ ᱾
ᱛᱳᱣᱟ ᱰᱟᱦᱟᱨ Milky Way GalaxyType Sb, Sbc, or SB(rs)bcFrommert, Hartmut; Kronberg, Christine (August 26, 2005). "Classification of the Milky Way Galaxy" . SEDS . Archived from the original on May 31, 2015. Retrieved May 30, 2015 . </ref> (barred spiral galaxy ) Diameter 1.5–2.3 Mly (460–710 kpc )Croswell, Ken (March 23, 2020). "Astronomers have found the edge of the Milky Way at last" . Archived from the original on March 24, 2020. Retrieved March 27, 2020 . </ref> Thickness of thin stellar disk ≈2 kly (0.6 kpc) Number of stars 100–400 billion [(1–4)×1011 ] Mass 0.8–1.5 × 1012 M ☉ Angular momentum ≈7067100000000000000♠ 1× 1067 J s[ ᱑] Sun's distance to Galactic Center 26.4 ± 1.0 kly (8.09 ± 0.31 kpc)ᱪᱷᱟᱸᱪ:Additional citation needed Sun's Galactic rotation period 240 Myr Spiral pattern rotation period 220–360 Myr Bar pattern rotation period100–120 Myr Speed relative to CMB rest frame 552.2 ± 5.5 km/s Escape velocity at Sun's position 550 km/s Dark matter density at Sun's position 0.0088ᱪᱷᱟᱸᱪ:Sup sub M ☉ pc−3 or 0.35ᱪᱷᱟᱸᱪ:Sup sub GeV cm−3 See also: Galaxy , List of galaxies
ᱫᱷᱟᱹᱨᱛᱤ ᱠᱷᱚᱱ ᱪᱮᱫ ᱞᱮᱠᱟ ᱧᱮᱞᱚᱜᱼᱟ
ᱥᱟᱯᱲᱟᱣ
ᱫᱷᱟᱹᱨᱛᱤ ᱫᱚ ᱱᱚᱶᱟ ᱜᱮᱞᱟᱠᱥᱤ ᱨᱮᱱᱟᱜ ᱜᱮ ᱢᱤᱫ ᱯᱟᱦᱴᱟ ᱠᱟᱱᱟ ᱾ ᱱᱚᱶᱟ ᱜᱮᱞᱟᱠᱥᱤ ᱫᱚ ᱧᱤᱫᱟᱹ ᱵᱮᱞᱟ ᱥᱮᱨᱢᱟ ᱨᱮᱱᱟᱜ ᱢᱤᱫ ᱯᱟᱦᱟᱴᱟ ᱠᱷᱚᱱ ᱮᱴᱟᱜ ᱯᱟᱦᱴᱟ ᱫᱷᱟᱹᱨᱤᱡ ᱦᱟᱞᱠᱟ ᱨᱮᱢᱮᱞ ᱞᱮᱠᱟ ᱯᱟᱥᱱᱟᱣ ᱜᱮ ᱧᱮᱞᱚᱜᱼᱟ ᱾
↑ Karachentsev, Igor. "Double Galaxies §7.1" . ned.ipac.caltech.edu . Izdatel'stvo Nauka. Archived from the original on March 4, 2016. Retrieved April 5, 2015 .