A satellite of mass 1000kg$1000\mathrm{kg}$ is launched to revolve around the earth in an orbit at a height of 270km$270\mathrm{km}$ from the earth's surface. Kinetic energy of the satellite in this orbit is \_ \times 10^{10}\mathrm{J}. (Mass of earth$ .
(Mass of earth $= 6\times 10^{24}\mathrm{kg},Radius of earth$
Radius of earth $= 6.4 \times 10^{6} \mathrm{~m}, Gravitational constant$ ,
Gravitational constant $= 6.67 \times 10^{-11} \mathrm{Nm}^2 \mathrm{kg}^{-2}$)
Numerical Answer Type:
Enter a numerical valueAnswer: 3 to 3+4 marks
Solution & Explanation
Related Formula
Orbital speed (v₀$v_0$) of a satellite at distance r$r$ from earth's center:
Sees: Kinetic energy of a satellite orbiting at an altitude above earth's surface.
Trap: Doing long division calculation for 6.67/2$6.67/2$. Check for clean cancellations in formulas first!
Shortcut: Notice that Rₑ + h = 6.4 × 10⁶ + 0.27 × 10⁶ = 6.67 × 10⁶$R_e + h = 6.4 \times 10^6 + 0.27 \times 10^6 = 6.67 \times 10^6$, which matches the value of the Gravitational constant G = 6.67 × 10⁻¹¹$G = 6.67 \times 10^{-11}$ perfectly. This clean cancellation leaves behind simple integer math to give 3 × 10¹⁰ ~J$3 \times 10^{10} \mathrm{~J}$ immediately.
Keywords:#kinetic energy of orbiting satellite calculation#JEE Main 2025 Evening Q25#orbital radius satellite gravitation#satellite mechanical energy physics
More Gravitation Previous-Year Questions — Page 5
Q46jee_main_2024_31_jan_eveningEscape Velocity
The mass of the moon is 1/144$1/144$ times the mass of a planet and its diameter 1/16$1/16$ times the diameter of a planet. If the escape velocity on the planet is v, the escape velocity on the moon will be:
For the planet: v = √((2GMₚ)/(Rₚ))$v = \sqrt{\frac{2GM_p}{R_p}}$
For the moon: Mm = (Mₚ)/(144)$M_m = \frac{M_p}{144}$ and Rm = (Rₚ)/(16)$R_m = \frac{R_p}{16}$.
Four identical particles of mass m$m$ are kept at the four corners of a square. If the gravitational force exerted on one of the masses by the other masses is ( 2√(2) + 132) Gm²L²$\left(\frac{2\sqrt{2} + 1}{32}\right)\frac{\mathrm{Gm}^2}{\mathrm{L}^2}$, the length of the sides of the square is
A.L2$\frac{\mathrm{L}}{2}$
B.4 L$4 L$
C.3L$3L$
D.2 L$2 L$
Solution
Related Formula
F = (G m₁ m₂)/(r²)$$F = \frac{G m_1 m_2}{r^2}$$
Core Logic
Superposition Principle diagram for Q37 - JEE Main 2024 Morning
Let the side length of the square be a$a$. Considering one corner mass, it experiences forces from the adjacent two masses (distance a$a$) and the diagonally opposite mass (distance √(2)a$\sqrt{2}a$).
The forces from the two adjacent masses are at 90^°$90^\circ$ to each other:
F = (Gm²)/(a²)$$F = \frac{Gm^2}{a^2}$$
The resultant of these two is √(2)F = √(2) (Gm²)/(a²)$\sqrt{2}F = \sqrt{2} \frac{Gm^2}{a^2}$, directed along the diagonal.
Step 2: Total Force Equation
The force from the diagonal mass is:
F' = Gm²(√(2)a)² = (Gm²)/(2a²)$$F' = \frac{Gm^2}{(\sqrt{2}a)^2} = \frac{Gm^2}{2a^2}$$
Total resultant force Fₙₑₜ = √(2)F + F'$F_{\text{net}} = \sqrt{2}F + F'$:
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