Activity 1: Drawing or IllustrationDraw or illustrate Kepler's Three Laws of Motion. Label andexplain each illustration. Include the equation used to describeKepler's Laws of Planetary Motion.Kepler's First Law of Planetary Kepler's Second Law ofMotion:Planetary Motion:Drawing/ IllustrationDrawing/IllustrationEquation:Explanation:Equation:Explanation:Kepler's Third Law of PlanetaryMotion:Drawing/ IllustrationEquation:Explanation:Activity 3: Problem Solving ActivityAnswer the following problems and show your process using thefour guide steps for solving problems.a. The mean solar distance of Earth is 1.50 x m with a period of1 year. What is the distance of mars from the sun if it has aperiod of 1.88 years?-b. Titan, the largest moon of Saturn, has a mean orbital radius of1.22x109 m. The orbital period of Titan is 15.95 days.Hyperion, another moon of Saturn, orbits at a mean radius of1.48x109 m. Use Kepler's third law of planetary motion topredict the orbital period of Hyperion in days.

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Activity 1: Drawing or Illustration Draw or illustrate Kepler's Three Laws of Motion. Label and explain each illustration. Include the equation used to describe Kepler's Laws of Planetary Motion. Kepler's First Law of Planetary Kepler's Second Law of Motion: Planetary Motion: Drawing/ Illustration Drawing/ Illustration Equation: Explanation: Equation: Explanation: Kepler's Third Law of Planetary Motion: Drawing/ Illustration Equation: Explanation:

Activity 1: Drawing or Illustration Draw or illustrate Kepler's Three Laws of Motion. Label and explain each illustration. Include the equation used to describe Kepler's Laws of Planetary Motion. Kepler's First Law of Planetary Kepler's Second Law of Motion: Planetary Motion: Drawing/ Illustration Drawing/ Illustration Equation: Explanation: Equation: Explanation: Kepler's Third Law of Planetary Motion: Drawing/ Illustration Equation: Explanation:

Stars and Galaxies

9th Edition

ISBN:9781305120785

Author:Michael A. Seeds, Dana Backman

Publisher:Michael A. Seeds, Dana Backman

Chapter4: Origins Of Modern Astronomy

Section: Chapter Questions

Problem 3DQ

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Using high resolution adaptive optical techniques, observations of a nearby (9.5 pc) cool star of mass 0.2 solar masses indicate the presence of a small rocky exoplanet in a circular orbit with a radius of 0.01 arcseconds. Using Kepler's Laws, estimate the period of the exoplanet's orbit in days. select units A
Let's use Kepler's laws for the inner planets. Use the following distances from the sun to calculate the orbital period for each of these planets. Express your answer in terms of Earth years to two significant figures. Answer for the highlighted planet in each question. Note: Use Kepler's law directly. Don't just Google the answers, as they will be a little bit different. When you have calculated them, only submit the value for Earth. Planet Distance from the sun Period of orbit around the sun Earth 150 million km ___ Earth years Mercury 58 million km ___ Earth years Venus 108 million km ___ Earth years Mars 228 million km ___ Earth years
Problem 4. Physical Features of the Giant Planets: Volume and Density of Jupiter (Palen, et. al. 1st Ed. Chapter 8 Problem 57 ) Jupiter is an oblate (Links to an external site.) planet with an average radius of 69,900 km, compared to Earth’s average radius of 6,370 km. How many Earth volumes could fit inside Jupiter? Jupiter is 318 times as massive as the Earth. How does Jupiter’s density compare (Links to an external site.) to that of Earth?
Let's use Kepler's laws for the inner planets. Use the following distances from the sun to calculate the orbital period for each of these planets. Express your answer in terms of Earth years to two significant figures. Note: Use Kepler's law directly. Don't just Google the answers, as they will be a little bit different. When you have calculated them, only submit the value for Mercury. Planet Distance from the sun Period of orbit around the sun Earth 150 million km ___ Earth years Mercury 58 million km ___ Earth years Venus 108 million km ___ Earth years Mars 228 million km ___ Earth years
Suppose there were a planet in our Solar System orbiting at a distance of 0.5 AU from the Sun, and having ten times the mass and four times the radius of Earth. For reference, the Earth has a mass of 5.97 × 10*24 kg and a radius of 6,378 km. a)Calculatethe density of this hypothetical planet. b)Basedon your answer from part a), what do you think this planet would be made of? Explain your c)Dothis planet’s properties agree with the condensation theory for the formation of our Solar System? Why or why not?
The table below presents the semi-major axis (a) and Actual orbital period for all of the major planets in the solar system. Cube for each planet the semi-major axis in Astronomical Units. Then take the square root of this number to get the Calculated orbital period of each planet. Fill in the final row of data for each planet. Table of Data for Kepler’s Third Law: Table of Data for Kepler’s Third Law: Planet aau = Semi-Major Axis (AU) Actual Planet Calculated Planet Period (Yr) Period (Yr) __________ ______________________ ___________ ________________ Mercury 0.39 0.24 Venus 0.72 0.62 Earth 1.00 1.00 Mars 1.52 1.88 Jupiter…
Task 5: Using the physical relationships to make predictions Now, imagine a giant disk with diameter D = 1 km with the same thickness and composition as the previous disks. Using the formulas for the straight lines found in Task 4: • What circumference do you predict for the giant disk? What mass do you predict for the giant disk?
O odysseyware A Ector County Independent Scho ector owschools.com/owsoo/studentAssignment/index?eh=785050194 I Other bool LEARN MESSAGE HELP SIGN OUT Assignment - 12. Quiz 2 ASSIGNMENTS COURSES SECTION I o 1 QUESTION 17 oF 20 Attempt 1 of 1 11 12 13 14 15 16 17 18 19 20 >> The acceleration due to gravity on Mars is less than that on Earth. On Mars, a person will weigh than on Earth. the same less more NEXT QUESTION O ASK FOR HELP TURN IT IN us v O 12:29 中 o8。
Part B. 1. The table below shows the gravitational force between Saturn and some ring particles that are at different distance from the planet. All of the particles have a mass of 1 kg. Table 1. Distance and Gravitational Force Data Distance of 1- Gravitational kg Ring Particle from Force between Saturn and 1-kg ring particle (in | 10,000 N) 2. Use the data in the table to make a graph of the relationship between distance and gravitational force. Label your graph "Gravitational Force and distance". Center of Saturn (in | 1,000 km) 100 38 Hint: Put the data for distance on the horizontal axis and the data for gravitational force on the vertical axis. 120 26 130 22 150 17 3. Look at your graphed data, and record in your answering sheet any relationship you notice. 180 12 200 9. 220 8 250 280 O 5
between a planet and its moon. Procedure/Analysis: Go to: https://www.physicsclassroom.com/Physics-Interactives/Circular-and-Satellite- Motion/Gravitational-Fields/Gravitational-Fields-Interactive Use the program to answer the following questions. 1. A planet and its moon are shown in the simulation window. Click and drag the moon to various positions about the planet and observe the gravitational force vector. In the diagram below, draw a force vector (arrow with arrowhead) to depict the direction and relative magnitude of the force acting upon the moon at the designated locations. Note: the size of the arrow should be representative of the strength of the force.
State and explain the implications of each of Kepler's three laws of planetary motion.
Procedure Table 11.1 presents Djup and Pday for the major Jovian satellites. First use these data and the equation above to calculate Jupiter’s mass in kilograms (kg). Enter your results in the table for each satellite. Next calculate the average Jupiter mass (Mjup, av) and enter the result in the table. Finally, calculate the percent difference (PD) using Mjup, av and the standard value for Jupiter’s mass (1.9 X 1027 kg). In the calculation of PD you can ignore 1027 because it will appear in both numerator and denominator. ________________________________________________________ Table 11.1 Calculated values for Jupiter’s Mass Satellite Djup Pday Mjup Io 2.95 1.77 Europa 4.69 3.55 Ganymede 7.50 7.15 Callisto 13.15 16.7 __________________________________________________________ Average Jupiter Mass = Percent Difference =