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ᱛᱳᱣᱟ ᱰᱟᱦᱟᱨ

ᱣᱤᱠᱤᱯᱤᱰᱤᱭᱟ, ᱨᱟᱲᱟ ᱜᱮᱭᱟᱱ ᱯᱩᱛᱷᱤ ᱠᱷᱚᱱ
(ᱛᱚᱣᱟ ᱰᱟᱦᱟᱨ ᱠᱷᱚᱱ ᱟᱹᱪᱩᱨ ᱦᱮᱡᱠᱟᱱᱟ)
ᱛᱳᱣᱟ ᱰᱟᱦᱟᱨ
Milky Way Galaxy
The Galactic Center as seen from Earth's night sky (the laser creates a guide-star for the telescope)
Observation data
TypeSb, 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)
Diameter1.5–2.3 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 stars100–400 billion [(1–4)×1011]
Mass0.8–1.5 × 1012 M
Angular momentum1×1067 J s[]
Sun's distance to Galactic Center26.4 ± 1.0 kly (8.09 ± 0.31 kpc)ᱪᱷᱟᱸᱪ:Additional citation needed
Sun's Galactic rotation period240 Myr
Spiral pattern rotation period220–360 Myr
Bar pattern rotation period100–120 Myr
Speed relative to CMB rest frame552.2 ± 5.5 km/s
Escape velocity at Sun's position550 km/s
Dark matter density at Sun's position0.0088ᱪᱷᱟᱸᱪ:Sup sub Mpc−3 or 0.35ᱪᱷᱟᱸᱪ:Sup sub GeV cm−3
See also: Galaxy, List of galaxies

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 ᱾

ᱫᱷᱟᱹᱨᱛᱤ ᱠᱷᱚᱱ ᱪᱮᱫ ᱞᱮᱠᱟ ᱧᱮᱞᱚᱜᱼᱟ

[ᱥᱟᱯᱲᱟᱣ | ᱯᱷᱮᱰᱟᱛ 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 ᱾

  1. 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.