**Kepler's Law****Image Description:** The image shows a detailed photo of an asteroid, highlighting its cratered surface.**Problem Statement:**What does Kepler's third law predict for the period of an Asteroid’s orbit around the Sun? Give your answer in years.**Given Values:**- Gravitational constant, \( G = 6.67 \times 10^{-11} \, \text{Nm}^2/\text{kg}^2 \)- Mass of the Asteroid, \( M_{\text{Asteroid}} = 8.8 \times 10^{20} \, \text{kg} \)- Mass of the Earth, \( M_{\text{Earth}} = 5.97 \times 10^{24} \, \text{kg} \)- Mass of the Sun, \( M_{\text{Sun}} = 2.00 \times 10^{30} \, \text{kg} \)- Distance from Sun to Asteroid, \( 5.50 \times 10^{12} \, \text{m} \)- There are \( 3.15 \times 10^7 \) seconds in 1 Earth year.**Objective:**Calculate the orbital period of the asteroid in Earth years using Kepler's third law. **Solution:**Insert the corrected formula and steps to find the period in years, if required, following the data given.(Note: This educational content would further include a detailed explanation or example calculations using Kepler's third law of planetary motion, though they are not included in the image text itself.)

Given data: The value of gravitational constant is G=6.67x10-11 N-m2/kg2. The mass of the asteroid…

What does Kepler's third law predict for the period of an Asteroid's orbit around the Sun? Give your answer in Years G=6.67x10 11 Nm2/kg2 MAsteroid=8.8x1020 kg MEarth=5.97x1024 kg Msun= 2.00x1030 kg Distance from Sun to Asteroid = 5.50x1012 m There are 3.15x107 seconds in 1 earth year. Years

What does Kepler's third law predict for the period of an Asteroid's orbit around the Sun? Give your answer in Years G=6.67x10 11 Nm2/kg2 MAsteroid=8.8x1020 kg MEarth=5.97x1024 kg Msun= 2.00x1030 kg Distance from Sun to Asteroid = 5.50x1012 m There are 3.15x107 seconds in 1 earth year. Years

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

See similar textbooks

Similar questions

The planet Saturn orbits the Sun at an average distance of 888 million miles. Use Kepler’s 3rd law to find the period of Saturn’s orbit, in Earth years.
You land on Mars and observe that one of its moons (Phobos) has an orbital period of 7.66 hours. If the Phobos were farther from Mars than it is now, it’s period would be a) less than 7.66 hrs. b) about 7.66 hrs. c) more than 7.66 hrs. d) difficult to predict without more information.
Describe your approach to the calculation of the period of a satellite moving in the gravitational field of a planet with mass M. a. Use Newton's 3rd law. b. Use Newton's law of universal gravitation. C. Use Kepler's 3rd law. d. Use Newton's 2nd law. e. Use Newton's 1st law.
Please use 9.81m/s^2 for earth gravity
Kepler's 1st law says that our Solar System's planets orbit in ellipses around the Sun where the closest distance to the Sun is called perihelion. Suppose I tell you that there is a planet with a perihelion distance of 2 AU and a semi-major axis of 1.5 AU. Does this make physical sense? Explain why or why not.
None
The radius of the Earth's orbit is 1.50 x 1011 m and that of Pluto is 5.93 x 1012 m. The star that this planet orbits is identical to our Sun. What is the orbital period of this planet? years eBook
According to Lunar Laser Ranging experiments the average distance LM from the Earth to the Moon is approximately 3.85 × 10° km. The Moon orbits the Earth and completes one revolution in approximately 27.5 days (a sidereal month). How can the mass of the Earth be calculated using the information above? Select the correct statements. Select one or more: O a. Use Newton's third law. O b. Use Newton's first law. c. Use Coulombs law. O d. Use Newton's second law.
Describe your approach to the calculation of the period of a satellite moving in the gravitational field of a planet with mass M. a. Use Newton's 3rd law. b. Use Newton's law of universal gravitation. c. Use Kepler's 3rd law. d. Use Newton's 2nd law. e. Use Newton's 1st law
Calculate the period of a satellite orbiting the Moon, 91 km above the Moon's surface. Ignore effects of the Earth. The radius of the Moon is 1740 km. Express your answer using three significant figures and include the appropriate units. μΑ ? T = Value Units Submit Request Answer
19. Saturn’s moon Mimas has an orbital period of T= 82,800 s at a distance of d= 1.87 × 10^8 m from Saturn. Using Kepler's 3rd law listed below for mass to determine Saturn’s mass. You must show your calculations for credit.
Kepler's third law of planetary motion describes a relationship between the__ * a, shape of orbit and the location of the Sun. b. orbital velocity and position in orbit c. distance from the Sun and length of year. d. path of epicycle and position.