Concept explainers
(a)
To Calculate:The maximum value of angular speed of sun and the time period corresponding to the maximum angular speed of the sun.
(a)
Answer to Problem 21P
The maximum value of angular speed of sun is
The time period corresponding to the maximum angular speed of the sun is
Explanation of Solution
Given data:
Universal gravitational constant,
Radius of the sun,
Measured
Moment of inertia for a sphere about axis through its center,
Time period of sun is
Formula used:
The gravitational attraction force on mass
The centripetal force on the mass
Here
Calculation:
The above two forces are equal in magnitude, but to estimate maximum angular speed, we must use inequality as below:
The maximum value of angular speed of sun is
The time period corresponding to the maximum angular speed of the sun is
Conclusion:
The maximum value of angular speed of sun is
The time period corresponding to the maximum angular speed of the sun is
(b)
To Calculate:
The angular momentum of the Jupiter
The angular momentum of the Saturn
To Compare: The calculated angular momentum value of Jupiter and Saturn with that of measured value of angular momentum of Sun.
(b)
Answer to Problem 21P
The angular momentum of the jupiter is
The angular momentum of Saturn is
Explanation of Solution
Given data:
Mean distance of the Jupiter is
Mean distance of the Saturn is
Orbital time period of Jupiter is
Orbital time period of Saturn is
Formula Used:
Angular momentum of the Jupiter,
Here, the linear velocity of the Jupiter,
Calculation:
The angular momentum of the Jupiter is
By substituting all known numerical values in the equation
Similarly, the angular momentum of the Saturn is
Consider the ratio,
Conclusion:
The angular momentum of the jupiter is
The angular momentum of Saturn is
The ratio is 0.00703.
(c)
To Calculate:The sun new rotational speed. Ratio of the time period of sun with the result in part (a).
(c)
Answer to Problem 21P
The sun new rotational speed is
The ratio of time period of sun with the result in part (a) is
Explanation of Solution
Given data:
Mean distance of the Jupiter is
Mean distance of the Saturn is
Time period of sun is
Formula Used:
The gravitational attraction force on mass
The
Here,
Calculation:
The final angular momentum of sun is
Substitute all known numerical values in the equation
The sun new rotational speed is:
The corresponding time period of the sun is
By comparing this time period of Sun with result in part
Conclusion:
The sun new rotational speed is
The ratio of time period of sun with the result in part (a) is
Want to see more full solutions like this?
Chapter 11 Solutions
Physics for Scientists and Engineers
- a) Calculate the angular momentum (in kg · m2/s) of Mercury in its orbit around the Sun. (The mass of Mercury is 3.300 ✕ 1023 kg, the orbital radius is 5.790 ✕ 107 km and the orbital period is 0.241 y.) kg · m2/s (b) Compare this angular momentum with the angular momentum of Mercury on its axis. (The radius of Mercury is 2.440 ✕ 103 km and the rotation period is 1408 h.) Lorbital Lrotation =arrow_forwardThe perihelion of the comet La Sagra is 1.37 AU and the aphelion is 7.49 AU. Given that its speed at perihelion is 33 km/s, what is the speed (in km/s) at aphelion (1 AU = 1.496 ✕ 1011 m)? (Hint: You may use either conservation of energy or angular momentum, but the latter is much easier.)arrow_forwardNeptune has a mass of 1.0 × 1026 kg and is 4.5 × 109 km from the Sun with an orbital period of 165 years. Planetesimals in the outer primordial solar system 4.5 billion years ago coalesced into Neptune over hundreds of millions of years. If the primordial disk that evolved into our present day solar system had a radius of 1011 km and if the matter that made up these planetesimals that later became Neptune was spread out evenly on the edges of it, what was the orbital period of the outer edges of the primordial disk?arrow_forward
- A meteor of mass m is approaching earth as shown on the sketch. The distance h on the sketch below is called the impact parameter. The radius of the earth is Re = 6400km . The 6x1024 kg mass of the earth is me = Suppose the meteor has an initial speed of vo = 30km/s. Assume that the meteor started very far away from the earth. Suppose the meteor just passes earth at a distance of 2.5Re from the earth's center. You may ignore all other gravitational forces except the earth. Find the moment arm h in km (called the impact parameter). G = 6.673x10-"Nm²kg 2 meteor very far away h impact parameter planetarrow_forwardCalculate the angular momentum (in kg · m2/s) of Mercury in its orbit around the Sun. (The mass of Mercury is 3.300 ✕ 1023 kg, the orbital radius is 5.790 ✕ 107 km and the orbital period is 0.241 y.) kg · m2/s (b) Compare this angular momentum with the angular momentum of Mercury on its axis. (The radius of Mercury is 2.440 ✕ 103km and the rotation period is 1408 h.) Lorbital Lrotation =arrow_forwardUranus has a mass of 8.68 1025 kg and a radius of 2.56 107 m. Assume it is a uniform solid sphere. The distance of Uranus from the Sun is 2.87 1012 m. (Assume Uranus completes a single rotation in 17.2 hours and orbits the Sun once every 3.06 104 Earth days.) (a)Calculate the angular momentum of Uranus in its orbit around the Sun, using kg · m2/s. __________kg · m2/s (b)Calculate the angular momentum of Uranus on its axis, using kg · m2/s. __________kg · m2/sarrow_forward
- Uranus has a mass of 8.68 1025 kg and a radius of 2.56 107 m. Assume it is a uniform solid sphere. The distance of Uranus from the Sun is 2.87 1012 m. (Assume Uranus completes a single rotation in 17.2 hours and orbits the Sun once every 3.06 104 Earth days.) (a) Calculate the angular momentum of Uranus in its orbit around the Sun, using kg · m2/s. (b) Calculate the angular momentum of Uranus on its axis, using kg · m2/s.arrow_forwardConsider a planet that has two layers. There is a core, which has density 9.9 x 103 kg/m3 and radius 3.9 x 106 m, and then there is a crust, which has density 4.9 x 103 kg/m3 and sits on top of the core. The planet has a total radius of 16.9 x 106 m. Calculate the acceleration due to gravity at the surface of this planet, in N/kg. Use G = 6.7 x 10-11 N m2/ kg2. (Please answer to the fourth decimal place - i.e 14.3225)arrow_forwardAt apogee, the center of the moon is 406,395 km from the center of Earth and at perigee, the moon is 357,643 km from the center of Earth. What is the orbital speed of the moon at perigee and at apogee? The mass of Earth is 5.98 x 1024 kg. speed at perigee| km/s speed at apogee m/s eBookarrow_forward
- (a) Calculate the angular momentum (in kg · m2/s) of Mercury in its orbit around the Sun. (The mass of Mercury is 3.300 ✕ 1023 kg, the orbital radius is 5.790 ✕ 107 km and the orbital period is 0.241 y.) (b) Compare this angular momentum with the angular momentum of Mercury on its axis. (The radius of Mercury is 2.440 ✕ 103 km and the rotation period is 1408 h.)arrow_forwardA 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 its eccentricity is 0.9932.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?arrow_forwardJupiter's moon Io has active volcanoes (in fact, it is the most volcanically active body in the solar system) that eject material as high as 500 km (or even higher) above the surface. Io has a mass of 8.93×1022kg8.93×1022kg and a radius of 1821 km. How high would this material go on earth if it were ejected with the same speed as on Io? (RE = 6370 km, mE=5.96×1024kg)arrow_forward
- Principles of Physics: A Calculus-Based TextPhysicsISBN:9781133104261Author:Raymond A. Serway, John W. JewettPublisher:Cengage Learning