Classical Dynamics of Particles and Systems
5th Edition
ISBN: 9780534408961
Author: Stephen T. Thornton, Jerry B. Marion
Publisher: Cengage Learning
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Check out a sample textbook solutionStudents have asked these similar questions
The gravitational force exerted by the planet Earth on a unit
mass at a distancer from the center of the planet is
GMr
if rR
where M is the mass of Earth, Ris its radius, and G is the
gravitational constant. Is F a continuous function of r?
Compute the gravitational attraction on a unit mass at the origin due to the mass (of constant density) occupying the volume inside the sphere r = 2a and above the plane z = a. Hint: The magnitude of the gravitational force on the unit mass due to the element of mass dM at (r, θ, φ) is (G/r2)dM. You want the z component of this since the other components of the total force are zero by symmetry. Use spherical coordinates.
(a) Calculate the magnitude of the gravitational force exerted by Mars on a 65 kg human standing on the surface of Mars. (The mass of Mars is 6.4x1023 kg and its
radius is 3.4x106 m.)
240.0277
✓ N
(b) Calculate the magnitude of the gravitational force exerted by the human on Mars.
240.0277
N
(c) For comparison, calculate the approximate magnitude of the gravitational force of this human on a similar human who is standing 2.5 meters away.
1.76e8
XN
(d) What approximations or simplifying assumptions must you make in these calculations? (Note: Some of these choices are false because they are wrong physics!)
✔Treat Mars as though it were spherically symmetric.
Ignore the effects of the Sun, which alters the gravitational force that one object exerts on another.
✔Treat the humans as though they were points or uniform-density spheres.
O Use the same gravitational constant in (a) and (b) despite its dependence on the size of the masses.
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- Let gM represent the difference in the gravitational fields produced by the Moon at the points on the Earths surface nearest to and farthest from the Moon. Find the fraction gM/g, where g is the Earths gravitational field. (This difference is responsible for the occurrence of the lunar tides on the Earth.)arrow_forwardHow to solve?arrow_forwardThe equation for exact gravity force, F = -Gm integral(p_vec * (p^2)^(-3/2) vdt). p would be the distance from B to P. I assume that vdt is dm.arrow_forward
- The density inside a solid sphere of radius a is given by p=Po a/r, where Po is the density at the surface and r denotes the distance from the center. Find the gravitational field due to this sphere at a distance 2 a from its center.arrow_forwardWrite down an expression for the velocity of a satellite of mass m in a circular orbit of radius R around the Earth. Take the mass of the Earth as M and use G for the gravitational constant. Please use appropriate algebraic symbols for multiplication (* for a × b), division (/ for a/b), exponents (a^b for a³), square root (sqrt(a*b/c) for √a × b/c) etc. Display responsearrow_forwardYou perform an experiment to verify the gravitational constant on the surface of the Earth, and get the readings recorded in the chart below. Find the average and standard deviation of this data, and fınd the relative error of the average (i.e. percent difference) compared to the known value of the gravitational constant g = 9.81m. Does this data verify the known value? Why? %3| Values 9.91 9.88 9.5 9.2 9.66 8.8 9.7 10.01 9.82 9.81arrow_forward
- (a) (i) Define gravitational field strength and state whether it is a scalar or vector quantity. A mass m is at a height h above the surface of a planet (ii) of mass M and radius R. The gravitational field strength at height h is g. By considering the gravitational force acting on massm, derive an equation from Newton's law of gravitation to express g in terms of M, R, h and the gravitational conșțant G.arrow_forwarda met icle an he $ 4 R ▼ 888 F4 Part A Consider a uniform gravitational field (a fair approximation near the surface of a planet). Find U(y)-U(yo)= Fg. ds. where F₁ = -mg j and ds = dy j. Express your answer in terms of m, g, yo, and yf. View Available Hint(s) IVD ΑΣΦ ? U(yf) - U (yo) = Submit Part B Consider the force exerted by a spring that obeys Hooke's law. Find II(₂) II(-). APR tv 28 % 5 F5 T 6 F6 Y & 7 F7 U * 8 ²² de DII F8 ( 9 A DD F9 0 ) O 3 of 26 Review | Constants F10 P Iarrow_forwardAn endless thin wire of density Y1 (unit: kg/m) is just above the x axis. An infinitely thin layer of density Y2 (unit: kg/m²) is parallel to the x-y plane and intersects the z-axis at the point z= -a. Find the gravitational field at (x,y,z) position. Give your answer in terms of (G,Y1,Y2, a, x, y, z, ^x, ^y, ^z(unit vectors)). Hint: A hint is given in the figure. The result will be (+ and -).arrow_forward
- The gravitational acceleration on the surface of earth of radius (R) mean density (p) is (a) (4n / 3) GR? p (b) (4т? / 3) GR? p (c) (2n / 3) GR? p (d) (4π / 3) GR ρarrow_forwardThe gravitational constant g is 9.807 m/s² at sea level, but it decreases as you go up in elevation. A useful equation for this decrease in g is g = a - bz, where z is the elevation above sea level, a = 9.807 m/s², and b = 3.32 × 10−6 1/s². An astronaut "weighs” 80.0 kg at sea level. [Technically this means that his/her mass is 80.0 kg.] Calculate this person's weight in N while floating around in the International Space Station (z = 355 km). If the Space Station were to suddenly stop in its orbit, what gravitational acceleration would the astronaut feel immediately after the satellite stopped moving? The person's weight in N while floating around in the International Space Station is The astronaut feels a gravitational acceleration of 692.928 m/s² 8.6616 N.arrow_forwardFour uniform spheres, with masses mA= 40 kg,mB = 35 kg, mC = 200 kg, and mD= 50 kg, have (x, y) coordinates of (0, 50 cm),(0, 0), (-80 cm, 0), and (40 cm, 0), respectively. In unit-vector notation,what is the net gravitational force on sphere B due to theother spheres?arrow_forward
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