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 4
Q44jee_main_2024_29_january_eveningKepler's Laws of Planetary Motion
A planet takes 200 days$200\text{ days}$ to complete one revolution around the Sun. If the distance of the planet from Sun is reduced to one fourth of the original distance, how many days will it take to complete one revolution?
A.25$25$
B.50$50$
C.100$100$
D.20$20$
Solution
Related Formula
According to Kepler's Third Law (Law of Periods):
T² ∝ r³$T^2 \propto r^3$
where:
T$T$ is the time period of revolution.
r$r$ is the orbital radius of the planet.
Core Logic
Using the proportionality relationship for two states:
If orbital distance scales by x$x$, the period scales by x3/2$x^{3/2}$. Here, distance scales by (1)/(4)$\frac{1}{4}$, so the period scales by ((1)/(4))3/2 = (1)/(8)$\left(\frac{1}{4}\right)^{3/2} = \frac{1}{8}$. Thus, 200 × (1)/(8) = 25 days$200 \times \frac{1}{8} = 25\text{ days}$.
Chapter Mix
Class 11 Physics: Gravitation
Q35jee_main_2024_27_jan_morningAcceleration due to Gravity
Inverse square dependence means halving the distance scale amplifies the surface field metric by a factor of 2² = 4$2^2 = 4$ matching constant mass bounds.
Chapter Mix
Class 11 Physics: Gravitation
Qjee_main_2024_29_jan_morningAcceleration due to Gravity
At what distance above and below the surface of the earth a body will have same weight, (take radius of earth as R.)
A.√(5) R - R$\sqrt{5} \mathrm{R} - \mathrm{R}$
B.√(3) R - R2$\frac{\sqrt{3} \mathrm{R} - \mathrm{R}}{2}$
C.(R)/(2)$\frac{R}{2}$
D.√(5) R - R2$\frac{\sqrt{5} \mathrm{R} - \mathrm{R}}{2}$
Solution
Related Formula
Acceleration due to gravity at a height h$h$ above the Earth's surface:
Therefore, the required distance is √(5)R - R2$\frac{\sqrt{5}R - R}{2}$.
Pattern Recognition
Do not use the linear approximation formula gh ≈ g(1 - (2h)/(R))$g_h \approx g(1 - \frac{2h}{R})$ unless the problem explicitly states h ll R$h \ll R$. Equating the approximated form to depth gives hheight = (1)/(2) hdepth$h_{\text{height}} = \frac{1}{2} h_{\text{depth}}$, which fails when looking for a single unified distance value h$h$.
Escape velocity of a body from earth is 11.2 km/s$11.2 \,\mathrm{km/s}$. If the radius of a planet be one-third the radius of earth and mass be one-sixth that of earth, the escape velocity from the planet is:
A.11.2 ~km / s$11.2 \mathrm{~km / s}$
B.8.4 ~km / s$8.4 \mathrm{~km / s}$
C.4.2 ~km / s$4.2 \mathrm{~km / s}$
D.7.9 ~km / s$7.9 \mathrm{~km / s}$
Solution
Related Formula
Vₑ = √((2GM)/(R))$$V_e = \sqrt{\frac{2GM}{R}}$$
Core Logic
For Earth: Vₑ = √((2GME)/(RE)) = 11.2 ~km/s$V_e = \sqrt{\frac{2GM_E}{R_E}} = 11.2 \mathrm{~km/s}$
For the planet:
RP = RE3$\mathrm{R}_{\mathrm{P}} = \frac{\mathrm{R}_{\mathrm{E}}}{3}$ and MP = ME6$\mathrm{M}_{\mathrm{P}} = \frac{\mathrm{M}_{\mathrm{E}}}{6}$
We can express the escape velocity of the planet Vₚ$V_p$ as a ratio of the Earth's escape velocity.
Any scaling of a planet's mass by factor α$\alpha$ and radius by factor β$\beta$ scales the escape velocity by a factor of √(α / β)$\sqrt{\alpha / \beta}$.
Chapter Mix
Class 11 Physics: Gravitation
Q42jee_main_2024_30_jan_morningGravitational Potential and Field
The gravitational potential at a point above the surface of earth is -5.12 × 10⁷ ~J / kg$-5.12 \times 10^{7} \mathrm{~J / kg}$ and the acceleration due to gravity at that point is 6.4 ~m/s²$6.4 \mathrm{~m/s^2}$. Assume that the mean radius of earth to be 6400 ~km$6400 \mathrm{~km}$. The height of this point above the earth's surface is:
The gravitational potential (V$V$) and acceleration due to gravity (g'$g'$) at a distance r = RE + h$r = R_E + h$ from the center of the earth can be related by dividing their magnitudes: |V| / g' = r$|V| / g' = r$.
Practice past-year questions one chapter at a time. Pick an exam → subject → chapter and get every PYQ for that topic — pulled together from all past papers — with the chapter's key formulas alongside.