Question:

Let us assume that our galaxy consists of 2.5 × 1011 stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution ? Take the diameter of the Milky Way to be 105 ly.

Updated On: Nov 5, 2023
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Solution and Explanation

Mass of our galaxy Milky Way, M = 2.5 × 1011
solar mass Solar mass = Mass of Sun = 2.0 × 1036 kg
Mass of our galaxy, M = 2.5 × 1011 × 2 × 1036 = 5 ×1041 kg
Diameter of Milky Way, d = 105 ly
7 Radius of Milky Way, r = 5 × 104 ly 
1 ly = 9.46 × 1015 m
∴ r = 5 × 104 × 9.46 × 1015 
= 4.73 ×1020 m

Since a star revolves around the galactic centre of the Milky Way, its time period is given by the relation:

\(T = (\frac{4π^2 \,r^3 }{ GM})^{\frac{1}{2}}\)
\(= (\frac{4 × (3.14)^2 × (4.73)^3 × 10^{60} }{6.67 ×10 ^{-11 }× 5 × 10^{41}}) ^{\frac{1}{2}} =\frac{ 39.48 × 105.82 ×10^{30} }{33.35 }) ^{\frac{1}{2}}\)

\(=(125.27 ×  10^{30} )^{\frac{1}{2}} = 1.12 × 10^{16}\) s 
1 year = 365 x 324 x 60x60 s
\(1s = \frac{1}{365 ×324 × 60×60}\) year
\(∴ 1.12 × 10^{16}s = \frac{1.12 × 10^{16} }{365 × 324 × 60×60}\)
\(= 3.55×   10 ^8 \) years

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Concepts Used:

Newtons Law of Gravitation

Gravitational Force

Gravitational force is a central force that depends only on the position of the test mass from the source mass and always acts along the line joining the centers of the two masses.

Newton’s Law of Gravitation:

According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,

  • Directly proportional to the product of their masses i.e. F ∝ (M1M2) . . . . (1)
  • Inversely proportional to the square of the distance between their center i.e. (F ∝ 1/r2) . . . . (2)

By combining equations (1) and (2) we get,

F ∝ M1M2/r2

F = G × [M1M2]/r2 . . . . (7)

Or, f(r) = GM1M2/r2 [f(r)is a variable, Non-contact, and conservative force]