A satellite of mass 1000mathrmkg is launched to revolve around the earth in an orbit at a height of 270mathrmkm from the earth's surface. Kinetic energy of the satellite in this orbit is \_ \times 10^{10}\mathrm{J} . (Mass of earth = 6\times 10^{24}\mathrm{kg}, Radius of earth = 6.4 \times 10^{6} \mathrm{~m} , Gravitational constant = 6.67 \times 10^{-11} \mathrm{Nm}^2 \mathrm{kg}^{-2}$)

Numerical Answer Type:
Enter a numerical value Answer: 3 to 3 +4 marks

Solution & Explanation

### Related Formula 1. Orbital speed (v_0) of a satellite at distance r from earth's center: v_0 = sqrtfracG M_er 2. Orbital Radius: r = R_e + h 3. Kinetic Energy of the orbiting satellite: mathrmKE = frac12 m v_0^2 = fracG M_e m2(R_e + h) ### Core Logic Given parameters: - Mass of satellite m = 1000 \ mathrmkg = 10^3 \ mathrmkg - Orbit altitude h = 270 \ mathrmkm = 0.27 times 10^6 \ mathrmm - Earth Radius R_e = 6.4 times 10^6 \ mathrmm - Earth Mass M_e = 6 times 10^24 \ mathrmkg - Gravitational constant G = 6.67 times 10^-11 \ mathrmN cdot m^2 / kg^2 ### Step 1: Calculate kinetic energy First, compute the orbital radius r: r = R_e + h = 6.4 times 10^6 \ mathrmm + 0.27 times 10^6 \ mathrmm = 6.67 times 10^6 \ mathrmm Substitute r = 6.67 times 10^6 \ mathrmm into the kinetic energy equation: mathrmKE = fracG M_e m2 r mathrmKE = frac6.67 times 10^-11 times 6 times 10^24 times 10^32 times 6.67 times 10^6 Notice that the value 6.67 cancels out directly: mathrmKE = frac6 times 10^162 times 10^6 = 3 times 10^10 \ mathrmJ Thus, the kinetic energy coefficient is 3. ### Pattern Recognition Sees: Kinetic energy of a satellite orbiting at an altitude above earth's surface. Trap: Doing long division calculation for 6.67/2. Check for clean cancellations in formulas first! Shortcut: Notice that 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 times 10^-11 perfectly. This clean cancellation leaves behind simple integer math to give 3 times 10^10 mathrm~J immediately. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 11 Physics: Gravitation

Reference Study Guides

More Gravitation Previous-Year Questions — Page 4

Q42 jee_main_2024_30_jan_morning Gravitational Potential and Field
The gravitational potential at a point above the surface of earth is -5.12 times 10^7 mathrm~J / kg and the acceleration due to gravity at that point is 6.4 mathrm~m/s^2. Assume that the mean radius of earth to be 6400 mathrm~km. The height of this point above the earth's surface is:
  • A. 1600 mathrm\,km
  • B. 540 mathrm\,km
  • C. 1200 mathrm\,km
  • D. 1000 mathrm\,km

Solution

### Related Formula V = -fracGM_ER_E + h g' = fracGM_E(R_E + h)^2 ### Core Logic The gravitational potential (V) and acceleration due to gravity (g') at a distance r = R_E + h from the center of the earth can be related by dividing their magnitudes: |V| / g' = r. ### Step 1: Set Up Equations From the given data: -fracGM_ER_E + h = -5.12 times 10^7 quad dots (i) fracGM_E(R_E + h)^2 = 6.4 quad dots (ii) ### Step 2: Isolate Variable Divide equation (i) by (ii) (taking magnitudes): R_E + h = frac5.12 times 10^76.4 R_E + h = 0.8 times 10^7 mathrm~m = 8000 mathrm~km ### Step 3: Solve for h Given mean radius of the earth R_E = 6400 mathrm~km: 6400 + h = 8000 h = 1600 mathrm~km ### Pattern Recognition Always exploit the V/g = r relationship to extract distances cleanly without having to substitute large values for G or M_E. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 11 Physics: Gravitation
Q46 jee_main_2024_31_jan_evening Escape Velocity
The mass of the moon is 1/144 times the mass of a planet and its diameter 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:
  • A. fracv3
  • B. fracv4
  • C. fracv12
  • D. fracv6

Solution

### Related Formula v_textescape = sqrtfrac2GMR ### Core Logic For the planet: v = sqrtfrac2GM_pR_p For the moon: M_m = fracM_p144 and R_m = fracR_p16. ### Step 1: Setup the Ratio v_m = sqrtfrac2G M_mR_m v_m = sqrtfrac2G left(fracM_p144right)left(fracR_p16right) v_m = sqrtfrac2G M_pR_p times frac16144 ### Step 2: Simplification v_m = sqrtfrac2G M_pR_p times sqrtfrac19 v_m = v times frac13 = fracv3 ### Pattern Recognition Escape velocity scales as sqrtM/R. If M scales by x and R scales by y, velocity scales by sqrtx/y. Here, sqrt(1/144)/(1/16) = sqrt16/144 = sqrt1/9 = 1/3. ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 11 Physics: Gravitation
Q37 jee_main_2024_31_jan_morning Superposition Principle
Four identical particles of mass 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 left(frac2sqrt2 + 132right)fracmathrmGm^2mathrmL^2, the length of the sides of the square is
  • A. fracmathrmL2
  • B. 4 L
  • C. 3L
  • D. 2 L

Solution

### Related Formula F = fracG m_1 m_2r^2 ### Core Logic
Superposition Principle diagram for Q37 - JEE Main 2024 Morning
Superposition Principle diagram for Q37 - JEE Main 2024 Morning
Let the side length of the square be a. Considering one corner mass, it experiences forces from the adjacent two masses (distance a) and the diagonally opposite mass (distance sqrt2a). The forces from the two adjacent masses are at 90^circ to each other: F = fracGm^2a^2 The resultant of these two is sqrt2F = sqrt2 fracGm^2a^2, directed along the diagonal. ### Step 2: Total Force Equation The force from the diagonal mass is: F' = fracGm^2(sqrt2a)^2 = fracGm^22a^2 Total resultant force F_textnet = sqrt2F + F': F_textnet = sqrt2 fracGm^2a^2 + fracGm^22a^2 = fracGm^2a^2 left( sqrt2 + frac12 right) F_textnet = fracGm^2a^2 left( frac2sqrt2 + 12 right) Equating this to the given force value: left(frac2sqrt2 + 132right)fracGm^2L^2 = fracGm^2a^2 left( frac2sqrt2 + 12 right) frac132 L^2 = frac12 a^2 a^2 = 16 L^2 a = 4L ### Evaluation Rubric / Model Answer null ### Chapter Mix Class 11 Physics: Gravitation

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