Loose Leaf For Explorations: Introduction To Astronomy
9th Edition
ISBN: 9781260432145
Author: Thomas T Arny, Stephen E Schneider Professor
Publisher: McGraw-Hill Education
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Chapter 10, Problem 3P
To determine
The mass of the Jupiter using the orbital data for any of the Jupiter’s Moon.
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A classmate claims that if Jupiter’s Galilean moons were all the same distance from Jupiter, they would all experience the same amount of gravitational force. Using what you have learned and the evidence from the data table how would you respond to his claim?
(a) His claim is incorrect; if the moons were at an equal distance from Jupiter; then the pull of gravity would be the strongest on Ganymede because it has the greatest mass
(b) his claim is incorrect; if the moon were at an equal distance from Jupiter; then the pull of gravity would be the strongest on Europa; because it has the smallest mass
(c) his claim is incorrect; if the moon were at an equal distance from Jupiter; then the pull of gravity from Jupiter would be experienced equally by all four moons.
(d) his claim is incorrect; if the moon were at an equal distance from Jupiter; then the pull of gravity would be the strongest on Ganymede because it is the largest moon
I would like you to compare the size of some of the largest moons of the solar system to their host planets. Using diameters of 12,700 km, and 140,000 km, 116,000 km for Earth, Jupiter, and Saturn respectively, please provide the ratios of the following moons to their host planets (you can use Table 12.1 from the book to get the diameters of the moons): Luna (Earth's moon), Io, Callisto, Ganymede, Europa, and Titan. After collecting those ratios, please tell me one thing that you notice that stands out about those results.
You are given the following data from observations of an exoplanet: Using Kepler’s Third Law (r3 = MT2 where M is the mass of the central star) find the orbital radius in astronomical units of this planet. M = 1.5 times the mass of the sun. Remember to convert days to years using 365.25 as the length of a year in days. What is the semimajor axis of this planet in AU?
- Knowing the orbital radius in both kn and AU, use the value in km to find the circumference of the orbit, then convert that to meters. (Assume the orbit is a perfect circle).
- Knowing the orbital circumference and the period in days, convert the days to seconds (multiply by 86,400) and find the orbital velocity in m/s
- With that orbital velocity, the radius of the orbit in meters, find the centripetal acceleration of our exoplanet
- Knowing the acceleration that our planet experiences, calculate the force that the host star exerts on the planet
- Knowing the force on the planet, the orbital radius, and the mass of the…
Chapter 10 Solutions
Loose Leaf For Explorations: Introduction To Astronomy
Ch. 10 - Prob. 1QFRCh. 10 - What does Jupiter look like?Ch. 10 - How do astronomers know what lies inside the outer...Ch. 10 - What are the major gaseous substances that make up...Ch. 10 - What is the interior structure of Jupiter and...Ch. 10 - Do Jupiter and Saturn have solid surfaces?Ch. 10 - Prob. 7QFRCh. 10 - Prob. 8QFRCh. 10 - What sort of activity has been seen on Io? What is...Ch. 10 - What are the rings of Saturn made of? How do...
Ch. 10 - Prob. 11QFRCh. 10 - Prob. 12QFRCh. 10 - Prob. 13QFRCh. 10 - What is unusual about Uranuss rotation axis? What...Ch. 10 - Prob. 15QFRCh. 10 - Why are Uranus and Neptune so blue?Ch. 10 - Why are the outer planets so large?Ch. 10 - Prob. 18QFRCh. 10 - Prob. 1TQCh. 10 - Prob. 2TQCh. 10 - Ganymede and Callisto orbiting Jupiter and Tethys...Ch. 10 - Approximate the Roche limit as 2.44 times a...Ch. 10 - Prob. 5TQCh. 10 - (10.3) Is Uranuss sky blue for the same reason our...Ch. 10 - Prob. 7TQCh. 10 - Prob. 8TQCh. 10 - Prob. 9TQCh. 10 - Prob. 10TQCh. 10 - Prob. 1PCh. 10 - Prob. 2PCh. 10 - Prob. 3PCh. 10 - Prob. 4PCh. 10 - Prob. 5PCh. 10 - Prob. 6PCh. 10 - Prob. 7PCh. 10 - Prob. 8PCh. 10 - (10.1) The low average densities of Jupiter and...Ch. 10 - Prob. 2TYCh. 10 - Prob. 3TYCh. 10 - Prob. 4TYCh. 10 - Prob. 5TYCh. 10 - Prob. 6TYCh. 10 - Prob. 7TY
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- There is one part to this question. I need to know the km/s. Thank you!arrow_forwardhelpp plzarrow_forwardThis is a challenging problem. Solve it on paper, writing out each step carefully. When doing calculations, do not round intermediate values. Note: If you have approached the problem in a principled way, do not abandon your approach if your numerical answer is not accepted; check your calculations! This problem is closely related to the spectacular impact of the comet Shoemaker-Levy with Jupiter in July 1994. (More information about the event can be found here.) A rock far outside a solar system similar to ours is initially moving very slowly relative to its sun, in the plane of the orbit of a large planet (about the size of Jupiter) around its sun. The rock falls toward the sun, but on its way to the sun it collides with the planet. The mass of the planet is 4 x 1027 kg, the mass of its sun is 3.2 x 1030 kg, the radius of the planet is 1.4 x 10® m, and the center-to-center distance from the planet to the sun is 9.2 x 1011 m. Part 1 (a) Calculate the rock's speed just before it…arrow_forward
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