A mass M is split into two parts, m and M - m, which are

A mass M is split into two parts, m and M - m, which are then separated by a certain distance. What ratio mlM maximizes the magnitude of the gravitational force between the parts?

Moon effect. Some people believe that the Moon controls their activities. If the Moon moves from being directly on the opposite side of Earth from you to being directly overhead, by what percent does (a) the Moon's gravitational pull on you increase and (b) your weight (as measured on a scale) decrease? Assume that the Earth - Moon (center-to-center) distance is 3.82 X 108 m and Earth's radius is 6.37 X 106 m.

What must the separation be between a 5.2 kg particle and a 2.4 kg particle for their gravitational attraction to have a magnitude of2.3 X 10-12 N?

The Sun and Earth each exert a gravitational force on the Moon. What is the ratio FsunlFEarth of these two forces? (The average Sun - Moon distance is equal to the Sun - Earth distance.)

Miniature black holes. Left over from the big-bang beginning of the universe, tiny black holes might still wander through the universe. If one with a mass of 1 X 1011 kg (and 1111 a radius of only 1 X 10-16 m) reached Earth, at what distance from your head would its gravitational pull on you match that of Earth's?

In Fig. 13-31, a square of edge length 20.0 cm is formed by four spheres of masses /111 = 5.00 g, m2 = 3.00 g, m3 = 1.00 g, and m4 = 5.00 g. In unit-vector notation, what is the net gravitational force from them on a central sphere with mass m5 = 2.50 g?

One dimension. In Fig. 13-32, two point particles are fixed on an x axis separated by distance d. Particle A has mass I11A and particle B has mass 3.00I11A' A third particle C, of ass 75.0mA' is to be placed on the x axis and near particles A and B. In terms of distance d, at what x coordinate should C be placed so that the net gravitational force on particle A from particles Band C is zero?

In Fig. 13-33, three 5.00 kg spheres are loFig. 13-32 Problem 7. cated at distances d1 = 0.300 m and d2 = 0.400 m. What are the (a) magnitude and (b) direction (relative to the positive direction of the x axis) of the net gravitational force on sphere B due to spheres A andC?

We want to position a space probe along a line that extends directly toward the Sun in order to monitor solar flares. How far from Earth's center is the point on the line where the Sun's gravitational pull on the probe balances Earth's pull?

Til'O dimensions. In Fig. 13- 34, three point particles are fixed in place in an xy plane. Particle A has mass mA, particle B has mass 2.00I11A, and particle C has mass 3.00I11A' A fourth particle D, with mass 4.00I11A' is to be placed near the other three particles. In terms of distance d, at what (a) x coordinate and (b) y coordinate Fig. 13-34 Problem 10.should particle D be placed so that the net gravitational force on particle A from particles B, C, and D is zero?

As seen in Fig. 13-35, two spheres of mass m and a third sphere of mass M form an equilateral triangle, and a fourth sphere of mass m4 is at the center of the triangle. The net gravitational force on that central sphere from the three other spheres is zero. (a) What is M in terms of m? (b) If we double the value of m4, what then is the magnitude of the net gravi- 111 tational force on the central sphere?

In Fig. 13-36a, particle A is fixed 11,1[ Fig. 13-35 Problem 11. 111 in place at x = -0.20 m on the x axis and particle B, with a mass of 1.0 kg, is fixed in place at the origin. Particle C (not shown) can be moved along the x axis, between particle B and x = 00. Figure 13-36b shows the x component Fnet. x of the net gravitational force on particle B due to particles A and C, as a function of position x of particle C. The plot actually extends to the right, approaching an asymptote of -4.17 X 10- 10 N as x - 00. What are the masses of (a) particle A and (b) particle C?

Figure 13-37 shows a spherical hollow inside a lead sphere of radius R = 4.00 cm; the surface of the hollow passes through the center of the sphere and "touches" the right side of the sphere. The mass /II of the sphere before hollowing Fig. 13-37 Problem 13. was M = 2.95 kg. With what gravitational force does the hollowed-out lead sphere attract a small sphere of mass m = 0.431 kg that lies at a distance d = 9.00 cm from the center of the lead sphere, on the straight line connecting the centers of the spheres and of the hollow?

Three point particles are fixed in position in an xy plane. Tho of them, particle A of mass 6.00 g and particle B of mass 12.0 g, are shown in Fig. 13-38, with a separation of dAB = 0.500 m at angle () = 30. Particle C, with mass 8.00 g, is not shown. The net gravitational force acting on particle A due to particles Band Cis 2.77 X 10- 14 N at an any B e -------L--~----x A Fig. 1 3-38 Problem 14. gle of -163.8 from the positive direction of the x axis. What are (a) the x coordinate and (b) the y coordinate of particle C?

Three dimensions. Three point particles are fixed in place in an xyz coordinate system. Particle A, at the origin, has mass mAo Particle B, at xyz coordinates (2.00d, l.OOd, 2.00d), has mass 2.00I11A, and particle C, at coordinates (-1.00d, 2.00d, - 3.00d), has mass 3.00I11A' A fourth particle D, with mass 4.00I11A, is to be placed near the other particles. In terms of distance d, at what (a) x, (b) y, and (c) z coordinate should D be placed so that the net gravitational force on A from B, C, and D is zero?

In Fig. 13-39, a particle of mass ml = 0.67 kg is a distance d = 23 cm from one end of a uniform rod with length L = 3.0 m and mass M = 5.0 kg. What is the magnitude of the gravitational force Fan the particle from the rod? /--ryd/ll -11~dr r- d -I' L -I Fig. 13-39 Problem 16.

(a) What will an object weigh on the Moon's surface if it weighs 100 N on Earth's surface? (b) How many Earth radii must this same object be from the center of Earth if it is to weigh the same as it does on the Moon?

Mountain pull. A large mountain can slightly affect the direction of "down" as determined by a plumb line. Assume that we can model a mountain as a sphere of radius R = 2.00 km and density (mass per unit volume) 2.6 X 103 kg/m3. Assume also that we hang a 0.50 m plumb line at a distance of 3R from the sphere'S center and such that the sphere pulls horizontally on the lower end. How far would the lower end move toward the sphere?

At what altitude above Earth's surface would the gravitational acceleration be 4.9 m/s2?

Mile-high bllilding. In 1956, Frank Lloyd Wright proposed the construction of a mile-high building in Chicago. Suppose the building had been constructed. Ignoring Earth's rotation, find the change in your weight if you were to ride an elevator from the street level, where you weigh 600 N, to the top of the building.

Certain neutron stars (extremely dense stars) are believed to be rotating at about 1 rev/s. If such a star has a radius of 20 km, what must be its minimum mass so that material on its surface remains in place during the rapid rotation?

The radius R" and mass M" of a black hole are related by R" = 2GM,,Ic2, where c is the speed of light. Assume that the gravitational acceleration ag of an object at a distance ro = 1.00lR" from the center of a black hole is given by Eq. 13-11 (it is, for large black holes). (a) In terms of M",find ag at roo (b) Does ag at ro increase or decrease as M" increases? (c) What is ag at to for a very large black hole whose mass is 1.55 X 1012 times the solar mass of 1.99 X 1030 kg? (d) If an astronaut of height 1.70 m is at to with her feet down, what is the difference in gravitational acceleration between her head and feet? (e) Is the tendency to stretch the astronaut severe?

One model for a certain planet has a core of radius Rand mass M surrounded by an outer shell of inner radius R, outer radius 2R, and mass 4M. If M = 4.1 X 1024 kg and R = 6.0 X 106 m, what is the gravitational acceleration of a particle at points (a) R and (b) 3R from the center of the planet?

Two concentric spherical shells with uniformly distributed masses Ml and M2 are situated as shown in Fig. 13-40. Find the magnitude of the net gravitational force on a particle of mass m, due to the shells, when the particle is located at radial distance (a) a, (b) b, and (c) c.

A solid uniform sphere has a M2 mass of 1.0 X 104 kg and a radius of Fig. 13-40 Problem 24. 1.0 m. What is the magnitude of the gravitational force due to the sphere on a particle of mass m located at a distance of (a) 1.5 m and (b) 0.50 m from the center of the sphere? (c) Write a general expression for the magnitude of the gravitational force on the particle at a distance r oS 1.0 m from the center of the sphere.

Consider a pulsar, a collapsed star of extremely high density, with a mass M equal to that of the Sun (1.98 X 1030 kg), a radius R of only 12 km, and a rotational period T of 0.041 s. By what percentage does the free-fall acceleration g differ from the gravitational acceleration ag at the equator of this spherical star?

Figure 13-41 shows, not to scale, a cross section through the interior of Earth. Rather than being uniform throughout, Earth is divided into three zones: an outer crust, a mantle, and an inner core. The dimensions of these zones and the masses contained within them are shown on the figure. Earth has a total mass of 5.98 X 1024 kg and a radius of 6370 km. Ignore rotation and assume that Earth is spherical. (a) Calculate ag at the surface. (b) Suppose that a bore hole (the Moho/e) is driven to the crust-mantle interface at a depth of 25.0 km; what would be the value of ag at the bottom of the hole? (c) Suppose that Earth were a uniform sphere with the same total mass and size. What would be the value of ag at a depth of 25.0 km? (Precise measurements of ag are sensitive probes of the interior structure of Earth, although results can be clouded by local variations in mass distribution.)

Assume a planet is a uniform sphere of radius R that (somehow) has a narrow radial tunnel through its center (Fig. 13-7). Also assume we can position an apple anywhere along the tunnel or outside the sphere. Let FR be the magnitude of the gravitational force on the apple when it is located at the planet's surface. How far from the surface is there a point where the magnitude is iFR if we move the apple (a) away from theplanet and (b) into the tunnel?

Figure 13-42 gives the potential energy function U(r) of a projectile, plotted outward from the surface of a planet of radius Rs. What least kinetic energy is required of a projectile launched at the surface if the projectile is to "escape" the planet?

In Problem 1, what ratio 111/M gives the least gravitational potential energy for the system?

The mean diameters of Mars and Earth are 6.9 X 103 km and 1.3 X 104 km, respectively. The mass of Mars is 0.11 times Earth's mass. (a) What is the ratio of the mean density (mass per unit volume) of Mars to that of Earth? (b) What is the value of the gravitational acceleration on Mars? (c) What is the escape speed on Mars?

(a) What is the gravitational potential energy of the two-particle system in Problem 3? If you triple the separation between the particles, how much work is done (b) by the gravitational force between the particles and ( c) by you?

What multiple of the energy needed to escape from Earth gives the energy needed to escape from (a) the Moon and (b) Jupiter?

Figure 13-42 gives the potential energy function U(r) of a projectile, plotted outward from the surface of a planet of radius Rs. If the projectile is launched radially outward from the surface with a mechanical energy of -2.0 X 109 J, what are (a) its kinetic energy at radius r = 1.25Rs and (b) its tllrning point (see Section 8-6) in terms of Rs?

Figure 13-43 shows four particles, each of mass 20.0 g, that form a square with an edge length of d = 0.600 m. If d is reduced to 0.200 m, what is the change in the gravitational potential energy of the four-particle system?

Zero, a hypothetical planet, has a mass of 5.0 X 1023 kg, a radius of 3.0 X 106 m, and no atmosphere. A 10 kg space probe is to Fig. 13-43 Problem 35. be launched vertically from its surface. (a) If the probe is launched with an initial energy of 5.0 X 107 J, what will be its kinetic energy when it is 4.0 X 106 m from the center of Zero? (b) If the probe is to achieve a maximum distance of 8.0 X 106 m from the center of Zero, with what initial kinetic energy must it be launched from the surface of Zero?

The three spheres in Fig. 13-44, with masses mA = 80 g, mB = 10 g, and me = 20 g, have their centers on a common line, with L = 12 cm and d = 4.0 cm. You move sphere B along the line until its center-to-center separation from C is d = 4.0 cm. How much work is done on sphere B (a) by you and (b) by the net gravitational force on B due to spheres A and C?

In deep space, sphere A of mass 20 kg is located at the origin of an x axis and sphere B of mass 10 kg is located on the axis at x = 0.80 m. Sphere B is released from rest while sphere A is held at the origin. (a) What is the gravitational potential energy of the twosphere system just as B is released? (b) What is the kinetic energy of B when it has moved 0.20 m toward A?

(a) What is the escape speed on a spherical asteroid whose radius is 500 km and whose gravitational acceleration at the surface is 3.0 mls2 ? (b) How far from the surface will a particle go if it leaves the asteroid's surface with a radial speed of 1000 m/s? (c) With what speed will an object hit the asteroid if it is dropped from 1000 km above the surface?

A projectile is shot directly away from Earth's surface. Neglect the rotation of Earth. What multiple of Earth's radius RE gives the radial distance a projectile reaches if (a) its initial speed is 0.500 of the escape speed from Earth and (b) its initial kinetic energy is 0.500 of the kinetic energy required to escape Earth? (c) What is the least initial mechanical energy required at launch if the projectile is to escape Earth?

1\\10 neutron stars are separated by a distance of 1.0 X 1010 m. They each have a mass of 1.0 X 1030 kg and a radius of 1.0 X 105 m. They are initially at rest with respect to each other. As measured from that rest frame, how fast are they moving when (a) their separation has decreased to one-half its initial value and (b) they are about to collide?

Figure 13-45a shows a particle A that can be moved along a y axis from an infinite distance to the origin. That origin lies at the midpoint between particles Band C, which have identical )' (em) )' I ~ I-- D~-D~ r ~x (a) (b) Fig. 13-45 Problem 42. masses, and the y axis is a perpendicular bisector between them. Distance D is 0.3057 m. Figure l3A5b shows the potential energy U of the three-particle system as a function of the position of particle A along the y axis. The curve actually extends rightward and approaches an asymptote of -2.7 X 10-11 J as y -.> 00. What are the masses of (a) particles Band C and (b) particle A?

(a) What linear speed must an Earth satellite have to be in a circular orbit at an altitude of 160 km above Earth's surface? (b) What is the period of revolution?

A satellite is put in a circular orbit about Earth with a radius equal to one-half the radius of the Moon's orbit. What is its period of revolution in lunar months? (A lunar month is the period of revolution of the Moon.)

The Martian satellite Phobos travels in an approximately circular orbit of radius 9.4 X 106 m with a period of 7 h 39 min. Calculate the mass of Mars from this information.

The first known collision between space debris and a functioning satellite occurred in 1996: At an altitude of 700 km, a yearold French spy satellite was hit by a piece of an Ariane rocket. A stabilizing boom on the satellite was demolished, and the satellite was sent spinning out of control. Just before the collision and in kilometers per hour, what was the speed of the rocket piece relative to the satellite if both were in circular orbits and the collision was (a) head-on and (b) along perpendicular paths?

The Sun, which is 2.2 X 1020 m from the center of the Milky Way galaxy, revolves around that center once every 2.5 X 108 years. Assuming each star in the Galaxy has a mass equal to the Sun's mass of 2.0 X 1030 kg, the stars are distributed uniformly in a sphere about the galactic center, and the Sun is at the edge of that sphere, estimate the number of stars in the Galaxy.

The mean distance of Mars from the Sun is 1.52 times that of Earth from the Sun. From Kepler's law of periods, calculate the number of years required for Mars to make one revolution around the Sun; compare your answer with the value given in Appendix C.

A comet that was seen in April 574 by Chinese astronomers on a day known by them as the Woo Woo day was spotted again in May 1994. Assume the time between observations is the period of the Woo Woo day comet and take its eccentricity as 0.11. What are (a) the semimajor axis of the comet's orbit and (b) its greatest distance from the Sun in terms of the mean orbital radius Rp of Pluto?

An orbiting satellite stays over a certain spot on the equator of (rotating) Earth. What is the altitude of the orbit (called a geosynchronous orbit)?

A satellite, moving in an elliptical orbit, is 360 km above Earth's surface at its farthest point and 180 km above at its closest point. Calculate (a) the semimajor axis and (b) the eccentricity of the orbit.

The Sun's center is at one focus of Earth's orbit. How far from this focus is the other focus, (a) in meters and (b) in terms of the solar radius, 6.96 X 108 m? The eccentricity is 0.0167, and the semimajor axis is 1.50 X 1011 m.

A 20 kg satellite has a circular orbit with a period of 2.4 h and a radius of 8.0 X 106 m around a planet of unknown mass. If the magnitude of the gravitational acceleration on the surface of the planet is 8.0 m/s2, what is the radius of the planet?

Hunting a black hole. Observations of the light from a certain star indicate that it is part of a binary (two-star) system. This visible star has orbital speed v = 270 kmis, orbital period T = 1.70 days, and approximate mass 1111 = 6M" where M, is the Sun's mass, 1.99 X 1030 kg. Assume that the visible star and its companion star, which is dark and unseen, are both in circular orbits (Fig. 13-46). What multiple of Ms gives the approximate mass 1112 of the dark star?

In 1610, Galileo used his telescope to discover four prominent moons around Jupiter. Their mean orbital radii a and periods T are as follows: Name a (108 m) T(days) 10 4.22 1.77 Europa 6.71 3.55 Ganymede 10.7 7.16 Callisto 18.8 16.7 (a) Plot log a (y axis) against log T (x axis) and show that you get a straight line. (b) Measure the slope of the line and compare it with the value that you expect from Kepler's third law. (c) Find the mass of Jupiter from the intercept of this line with the y axis.

In 1993 the spacecraft Cali/eo sent home an image (Fig. 13-47) of asteroid 243 Ida and a tiny orbiting moon (now known as Dactyl), the first confirmed example of an asteroid-moon system. In the image, the moon, which is 1.5 km wide, is 100 km from the center of the asteroid, which is 55 km long. The shape of the moon's orbit is not well known; assume it is circular with a period of27 h. (a) What is the mass of the asteroid? (b) The volume of the asteroid, measured from the Cali/eo images, is 14100 km3. What is the density (mass per unit volume) of the asteroid?

In a certain binary-star system, each star has the same mass as our Sun, and they revolve about their center of mass. The distance between them is the same as the distance between Earth and the Sun. What is their period of revolution in years?

The presence of an unseen planet orbiting a distant star can sometimes be inferred from the motion of the star as we see it. As the star and planet orbit the center of mass of the star-planet system, the star moves toward and away from us with what is called the line of sight velocity, a motion that can be detected. Figure 13-48 shows a graph of the line of sight velocity versus time for the star 14 Herculis. The star's mass is believed to be 0.90 of the mass of our Sun. Assume that only one planet orbits the star and that our view is along the plane of the orbit. Then approximate (a) the planet's mass in terms of Jupiter's mass 111J and (b) the planet's orbital radius in terms of Earth's orbital radius rEo ~ 70,- ~.-----------~~ S c- '0 o l' 0 ..0 ~ '0 0,) \:i J -70 '----1----"""-----+----' Time Fig. 13-48 Problem 58.

Three identical stars of mass M form an equilateral triangle that rotates around the triangle'S center as the stars move in a common circle about that center. The triangle has edge length L. What is the speed of the stars?

In Fig. 13A9, two satellites,A and B, both of mass m = 125 kg, move in the same circular orbit of radius r = 7.87 X 106 m around Earth but in opposite senses of rotation and therefore on a collision course. (a) Find the total mechanical energy EA + EE of the two satellites + Earth system before the collision. (b) If the collision is completely inelastic so that the wreckage remains as one piece of tan- \ \ \ \ " '-, Earth Fig. 13-49 Problem 60. gled material (mass = 2111), find the total mechanical energy immediately after the collision. (c) Just after the collision, is the wreckage falling directly toward Earth's center or orbiting around Earth?

(a) At what height above Earth's surface is the energy required to lift a satellite to that height equal to the kinetic energy required for the satellite to be in orbit at that height? (b) For greater heights, which is greater, the energy for lifting or the kinetic energy for orbiting?

Two Earth satellites, A and B, each of mass 111, are to be launched into circular orbits about Earth's center. Satellite A is to orhit at an altitude of 6370 km. Satellite B is to orbit at an altitude of 19110 km. The radius of Earth R is 6370 km. (a) What is the ratio of the potential energy of satellite B to that of satellite A, in orhit? (b) What is the ratio of the kinetic energy of satellite B to that of satellite A, in orbit? (c) Which satellite has the greater total energy if each has a mass of 14.6 kg? (d) By how much?

An asteroid, whose mass is 2.0 X 10-4 times the mass of Earth, revolves in a circular orbit around the Sun at a distance that is twice Earth's distance from the Sun. (a) Calculate the period of revolution of the asteroid in years. (b) What is the ratio of the kinetic energy of the asteroid to the kinetic energy of Earth?

A satellite orbits a planet of unknown mass in a circle of radius 2.0 X 107 m. The magnitude of the gravitational force on the satellite from the planet is F = 80 N. (a) What is the kinetic energy of the satellite in this orbit? (b) What would Fbe if the orbit radius were increased to 3.0 X 107 m?

A satellite is in a circular Earth orbit of radius r. The area A enclosed by the orbit depends on ,.2 because A = 7T/.2. Determine how the following properties of the satellite depend on r: (a) period. (b) kinetic energy, (c) angular momentum, and (d) speed

One way to attack a satellite in Earth orbit is to launch a swarm of pellets in the same orbit as the satellite but in the opposite direction. Suppose a satellite in a circular orbit 500 km above Earth's surface collides with a pellet having mass 4.0 g. (a) What is the kinetic energy of the pellet in the reference frame of the satellite just before the collision? (b) What is the ratio of this kinetic energy to the kinetic energy of a 4.0 g bullet from a modem army rifle with a muzzle speed of 950 m/s?

What are (a) the speed and (b) the period of a 220 kg satellite in an approximately circular orbit 640 km above the surface of Earth? Suppose the satellite loses mechanical energy at the average rate of 1.4 X 105 J per orbital revolution. Adopting the reasonable approximation that the satellite's orbit becomes a "circle of slowly diminishing radius," determine the satellite's ( c) altitude, (d) speed, and (e) period at the end of its 1500th revolution. (f) What is the magnitude of the average retarding force on the satellite? Is angular momentum around Earth's center conserved for (g) the satellite and (h) the satellite-Earth system (assuming that system is isolated)?

Two small spaceships, each with mass 111 = 2000 kg, are in the cii'cular Earth orbit of Fig. 13-50, at an altitude h of 400 km. Igor, the commander of one of the ships, arrives at any fixed point in the orbit 90 s ahead of Picard, the commander of the other ship. What are the (a) period To and (b) speed 1'0 of the ships? At point P in Fig. 13-50, Picard fires an instantaneous burst in the forward direction, reducing his ship's speed by 1.00%. After this burst, he follows the elliptical orbit shown dashed in the Fig. 13-50 Problem 68. figure. What are the (c) kinetic energy and (d) potential energy of his ship immediately after the burst? In Picard's new elliptical orbit, what are (e) the total energy E, (f) the semimajor axis a, and (g) the orbital period T? (h) How much earlier than Igor will Picard return to P?

In Fig. 13-17 b, the scale on which the 60 kg physicist stands reads 220 N. How long will the cantaloupe take to reach the floor if the physicist drops it (from rest relative to himself) at a height of 2.1 m above the floor?

itional Problems The radius R" of a black hole is the radius of a mathematical sphere, called the event horizon, that is centered on the black hole. Information from events inside the event horizon cannot reach the outside world. According to Einstein's general theory of relativity, R" = 2GM/c2, where M is the mass of the black hole and c is the speed of light. Suppose that you wish to study a black hole near it, at a radial distance of 50R". However, you do not want the difference in gravitational acceleration between your feet and your head to exceed 10 m/s2 when you are feet down (or head down) toward the black hole. (a) As a multiple of our Sun's mass Ms, approximately what is the limit to the mass of the black hole you can tolerate at the given radial distance? (You need to estimate your height.) (b) Is the limit an upper limit (you can tolerate smaller masses) or a lower limit (you can tolerate larger masses)?

Several planets (Jupiter, Saturn, Uranus) are encircled by rings, perhaps composed of material that failed to form a satellite. In addition, many galaxies contain ring-like structures. Consider a homogeneous thin ring of mass M and outer radius R (Fig. 13-51). (a) What gravitational attraction does it exert on a particle of mass 111 located on the ring's central axis a distance x from the ring center? (b) Suppose the particle falls Fig. 13-51 Problem 71. from rest as a result of the attraction of the ring of matter. What is the speed with which it passes through the center of the ring?

A typical neutron star may have a mass equal to that of the Sun but a radius of only 10 kill. (a) What is the gravitational acceleration at the surface of such a star? (b) How fast would an object be moving if it fell from rest through a distance of 1.0 m on such a star? (Assume the star does not rotate.)

Figure 13-52 is a graph of the kinetic energy K of an asteroid versus its distance r from Earth's center, as the asteroid falls directly in toward that center. (a) What is the (approximate) mass of the asteroid? (b) What is its speed at r = 1.945 X 107 m? 3 lL-~~~~ __ ~~-L-L-L~~~~~~~~ 1.75 1.85 1. 95 r (107 111) Fig. 13-52 Problem 73.

The mysterious visitor that appears in the enchanting story The Little Prince was said to come from a planet that "was scarcely any larger than a house!" Assume that the mass per unit volume of the planet is about that of Earth and that the planet does not appreciably spin. Approximate (a) the free- fall acceleration on the planet's surface and (b) the escape speed from the planet.

The masses and coordinates of three spheres are as follows: 20 kg, x = 0.50 m, y = 1.0 m; 40 kg, x = -1.0 m, y = -1.0 m; 60 kg, x = 0 m, y = -0.50 m. What is the magnitude of the gravitational force on a 20 kg sphere located at the origin due to these three spheres?

A very early, simple satellite consisted of an inflated spherical aluminum balloon 30 m in diameter and of mass 20 kg. Suppose a meteor having a mass of 7.0 kg passes within 3.0 m of the surface of the satellite. What is the magnitude of the gravitational force on the meteor from the satellite at the closest approach?

Four uniform spheres, with masses 111 A = 40 kg, m B = 35 kg, 111e = 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 the other spheres?

(a) In Problem 77, remove sphere A and calculate the gravitational potential energy of the remaining three-particle system. (b) If A is then put back in place, is the potential energy of the four-particle system more or less than that of the system in (a)? (c) In (a), is the work done by you to remove A positive or negative? (d) In (b), is the work done by you to replace A positive or negative?

A certain triple-star system consists of two stars, each of mass m, revolving in the same circular orbit of radius r around a central star of mass M (Fig. 13-53). The two orbiting stars are always at opposite ends of a diameter of the orbit. Derive an expression for the I I \ \ I I / / I'v! I / / period of revolution of the stars.

The fastest possible rate of rotation of Problem 79. III \ \ I I I a planet is that for which the gravitational force on material at the equator just barely provides the centripetal force needed for the rotation. (Why?) (a) Show that the corresponding shortest period of rotation is T=)37r Gp' where p is the uniform density (mass per unit volume) of the spherical planet. (b) Calculate the rotation period assuming a density of 3.0 g/cm3, typical of many planets, satellites, and asteroids. No astronomical object has ever been found to be spinning with a period shorter than that determined by this analysis.

In a double-star system, two stars of mass 3.0 X 1030 kg each rotate about the system's center of mass at radius 1.0 X 1011 m. (a) What is their common angular speed? (b) If a meteoroid passes through the system's center of mass perpendicular to their orbital plane, what minimum speed must it have at the center of mass if it is to escape to "infinity" from the two-star system?

A satellite is in elliptical orbit with a period of 8.00 X 104 s about a planet of mass 7.00 X 1024 kg. At aphelion, at radius 4.5 X 107 m, the satellite's angular speed is 7.158 X 10-5 rad/s. What is its angular speed at perihelion?

In a shuttle craft of mass 111 = 3000 kg, Captain Janewav orbits a planet of mass M = 9.50 X 1025 kg, in a circular orbit of ra~ dius r = 4.20 X 107 m. What are (a) the period of the orbit and (b) the speed of the shuttle craft? Janeway briefly fires a forwardpointing thruster, reducing her speed by 2.00%. Just then, what are (c) the speed, (d) the kinetic energy, (e) the gravitational potential energy, and (f) the mechanical energy of the shuttle craft? (g) What is the semimajor axis of the elliptical orbit now taken by the craft? (h) What is the difference between the period of the original circular orbit and that of the new elliptical orbit? (i) Which orbit has the smaller period?

A uniform solid sphere of radius R produces a gravitation;:]1 acceleration of ag on its surface. At what distance from the sphere's center are there points (a) inside and (b) outside the sphere where the gravitational acceleration is ag /3?

A projectile is fired vertically from Earth's surface with an initial speed of 10 km/s. Neglecting air drag, how far above the surface of Earth will it go?

An object lying on Earth's equator is accelerated (a) toward the center of Earth because Earth rotates, (b) toward the Sun because Earth revolves around the Sun in an almost circular orbit, and (c) toward the center of our galaxy because the Sun moves around the galactic center. For the latter, the period is 2.5 X lOR Y and the radius is 2.2 X 1020 m. Calculate these three accelerations as multiples of g = 9.8 m/s2

(a) If the legendary apple of Newton could be released from rest at a height of 2 m from the surface of a neutron star with a mass 1.5 times that of our Sun and a radius of 20 km, what would be the apple's speed when it reached the surface of the star? (b) If the apple could rest on the surface of the star, what would be the approximate difference between the gravitational acceleration at the top and at the bottom of the apple? (Choose a reasonable size for an apple; the answer indicates that an apple would never survive near a neutron star.)

With what speed would mail pass through the center of Earth if falling in a tunnel through the center?

The orbit of Earth around the Sun is almost circular: The closest and farthest distances are 1.47 X 108 km and 1.52 X lOB km respectively. Determine the corresponding variations in (a) total energy, (b) gravitational potential energy, ( c) kinetic energy, and (d) orbital speed. (Hint: Use conservation of energy and conservation of angular momentum.)

A 50 kg satellite circles planet Cruton every 6.0 h. The magnitude of the gravitational force exerted on the satellite by Cruton is 80 N. (a) What is the radius of the orbit? (b) What is the kinetic energy of the satellite? (c) What is the mass of planet Cruton?

We watch two identical astronomical bodies A and B, each of mass m, fall toward each other from rest because of the gravitational force on each from the other. Their initial center-to-center separation is Ri Assume that we are in an inertial reference frame that is stationary with respect to the center of mass of this twobody system. Use the principle of conservation of mechanical