21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 3, Problem 3QP
To determine
What happens when Earth catches up to a slower-moving outer planet and passes it in its orbit.
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1. Mars takes 1.88 years to complete one orbit around the sun. What is its average distance from the sun?
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365 days, use Kepler's law of harmonies to predict the time for Mars to orbit the sun.
3. The period of rotation of Mars is 1 day and 37 minutes. Determine its frequency of rotation in Hertz.
Chapter 3 Solutions
21st Century Astronomy
Ch. 3.1 - Prob. 3.1ACYUCh. 3.1 - Prob. 3.1BCYUCh. 3.2 - Prob. 3.2CYUCh. 3.3 - Prob. 3.3CYUCh. 3.4 - Prob. 3.4CYUCh. 3 - Prob. 1QPCh. 3 - Prob. 2QPCh. 3 - Prob. 3QPCh. 3 - Prob. 4QPCh. 3 - Prob. 5QP
Ch. 3 - Prob. 6QPCh. 3 - Prob. 7QPCh. 3 - Prob. 8QPCh. 3 - Prob. 9QPCh. 3 - Prob. 10QPCh. 3 - Prob. 11QPCh. 3 - Prob. 12QPCh. 3 - Prob. 13QPCh. 3 - Prob. 14QPCh. 3 - Prob. 15QPCh. 3 - Prob. 16QPCh. 3 - Prob. 17QPCh. 3 - Prob. 18QPCh. 3 - Prob. 19QPCh. 3 - Prob. 20QPCh. 3 - Prob. 21QPCh. 3 - Prob. 22QPCh. 3 - Prob. 23QPCh. 3 - Prob. 24QPCh. 3 - Prob. 25QPCh. 3 - Prob. 26QPCh. 3 - Prob. 27QPCh. 3 - Prob. 28QPCh. 3 - Prob. 29QPCh. 3 - Prob. 30QPCh. 3 - Prob. 31QPCh. 3 - Prob. 32QPCh. 3 - Prob. 33QPCh. 3 - Prob. 34QPCh. 3 - Prob. 35QPCh. 3 - Prob. 36QPCh. 3 - Prob. 37QPCh. 3 - Prob. 38QPCh. 3 - Prob. 39QPCh. 3 - Prob. 40QPCh. 3 - Prob. 41QPCh. 3 - Prob. 42QPCh. 3 - Prob. 43QPCh. 3 - Prob. 44QPCh. 3 - Prob. 45QP
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- 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.arrow_forward8. The mean distance of Earth from the Sun is 149.6 x 10° km and the mean distance of Mercury from the Sun is 57.9 x 10° km. The period of Earth's revolutions is 1 year, what is the period of Mercury's revolution? a. 0.24 year on Earth b. 0.42 year on Earth C. 1.13 year on Earth d. 1.31 year on Earth 9. The planet Delta has 2 times the gravitational field strength and 3 times the radius of Earth. How does the mass of the planet Delta compare with the mass of Earth?arrow_forward9. Which of the following is NOT one of Kepler's Laws of Planetary Motion? A. The square of a planet's period is proportional to its distance from the sun cubed, B. The area of a planet's orbital plane is inversely proportional to its speed. C. A planet sweeps out equal area in an equal time interval. D. Planets move around the sun in elliptical orbits.arrow_forward
- 12. Which of the following lists of people contains three people who each supported a heliocentric model of the Universe? a. Copernicus, Kepler, Galileo. b. Ptolemy, Tycho, Kepler. c. Aristarchus, Plato, Ptolemy. d. Aristotle, Ptolemy, Plato.arrow_forward2. Outline Kepler's three lawsarrow_forwardA newly discovered planet orbits a star with the same mass as the Sun with a semi-major axis of 239.36 million kilometers. Its orbital eccentricity is 0.1.A. Find the planet's orbital period.B. Find the planet's perihelion distance.C. Find the planet's aphelion distance.arrow_forward
- The planet in the orbit shown in the drawing obeys Kepler s 2nd Law. B During which of the portions of the planet's orbit would the planet experience an increase in speed for at least one moment? A. Only during one of the portions shown. B. During two of the portions shown. C. During three of the portions shown. D. During four of the portions shown. O E. None of the above.arrow_forwardAccording 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.arrow_forward19. According to Isaac Newton, the value of the constant, k, in Kepler's Third Law (P2 = ka3) is dependent on which one of the following quantities for objects within the Solar System? a. The distance between the Sun and its planet. b. The mass of the planet. c. The electric charge of the Sun. d. The mass of the Sun.arrow_forward
- 3. Mars is 1.53 times as far from the Sun as Earth is. Use Kepler's third faw to predict the time required for Mars to orbit the sun in Earth days.arrow_forward2. From Kepler's Third Law, the period (P) squared divided by the cube of semi-major axis (d) is the same for all planets and is expressed as P2 / d = k, where k is a constant. One can conclude that A. In the same amount of time, every planet orbits the sun. B. At the same distance from the sun, every planet orbits the sun. C. It takes more time to orbit the sun if the planets are farthest from the sun. D. It takes less time to orbit the sun if the planets are farthest from the sun.arrow_forward1. What are Kepler's three laws of planetary motion and what is their significance?arrow_forward
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