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There are more than 200 billion stars in
Milky Way Galaxy
 The largest neighboring galaxy to Milky
Way galaxy is the Andromeda Galaxy
 The oldest star in Milky Way Galaxy is
13.2 billion years old which is almost
same as old as the universe
 The diameter of Milky Way Galaxy is
100,000 light years
 There are black holes in Milky Way
Galaxy

Tars and gases at a wide range of
distances from the Galactic center
orbit at approximately 220
kilometers per second.
Yes, this rate of rotation means that the
Solar System – which is 28,000 light years
from the center of the Milky Way –
completely orbits the galaxy about every
225 million years.
The galactic year, also known as a cosmic
year, is the duration of time required for the
Solar System to orbit once around the
center of the Milky Way Galaxy.[1]
Estimates of the length of one orbit range
from 225 to 250 million "terrestrial" years.
There are gravitational forces
between every particle of mass in
the universe and every
other particle of mass.

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Milky way

  • 1.
  • 2. There are more than 200 billion stars in Milky Way Galaxy  The largest neighboring galaxy to Milky Way galaxy is the Andromeda Galaxy  The oldest star in Milky Way Galaxy is 13.2 billion years old which is almost same as old as the universe  The diameter of Milky Way Galaxy is 100,000 light years  There are black holes in Milky Way Galaxy 
  • 3. Tars and gases at a wide range of distances from the Galactic center orbit at approximately 220 kilometers per second.
  • 4.
  • 5. Yes, this rate of rotation means that the Solar System – which is 28,000 light years from the center of the Milky Way – completely orbits the galaxy about every 225 million years.
  • 6. The galactic year, also known as a cosmic year, is the duration of time required for the Solar System to orbit once around the center of the Milky Way Galaxy.[1] Estimates of the length of one orbit range from 225 to 250 million "terrestrial" years.
  • 7. There are gravitational forces between every particle of mass in the universe and every other particle of mass.