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The time period of a geostationary satellite is 24 hr24 \text{ hr} at a height 6RE6R_E (RER_E is the radius of the Earth) from the surface of the earth. The time period of another satellite whose height is 2.5RE2.5R_E from the surface will be:

A

62 hr6\sqrt{2} \text{ hr}

B

122 hr12\sqrt{2} \text{ hr}

C

242.5 hr\frac{24}{2.5} \text{ hr}

D

122.5 hr\frac{12}{2.5} \text{ hr}

Step-by-Step Solution

  1. Kepler's Third Law: The square of the time period of revolution of a planet (or satellite) is proportional to the cube of the semi-major axis (radius for circular orbit) of its orbit. [Eq. 7.7, Eq. 7.38] T2r3    T12T22=r13r23T^2 \propto r^3 \implies \frac{T_1^2}{T_2^2} = \frac{r_1^3}{r_2^3}
  2. Determine Orbital Radii: The distance rr is measured from the center of the Earth. Given RER_E is the Earth's radius.
  • Satellite 1 (Geostationary): Height h1=6REh_1 = 6R_E. Orbit radius r1=RE+h1=RE+6RE=7REr_1 = R_E + h_1 = R_E + 6R_E = 7R_E.
  • Satellite 2: Height h2=2.5REh_2 = 2.5R_E. Orbit radius r2=RE+h2=RE+2.5RE=3.5REr_2 = R_E + h_2 = R_E + 2.5R_E = 3.5R_E.
  1. Calculate Ratio: T2T1=(r2r1)3/2=(3.5RE7RE)3/2=(12)3/2\frac{T_2}{T_1} = \left( \frac{r_2}{r_1} \right)^{3/2} = \left( \frac{3.5R_E}{7R_E} \right)^{3/2} = \left( \frac{1}{2} \right)^{3/2} T224=122\frac{T_2}{24} = \frac{1}{2\sqrt{2}}
  2. Solve for T2T_2: T2=2422=122=62 hrT_2 = \frac{24}{2\sqrt{2}} = \frac{12}{\sqrt{2}} = 6\sqrt{2} \text{ hr}
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