Integrated Science
7th Edition
ISBN: 9780077862602
Author: Tillery, Bill W.
Publisher: Mcgraw-hill,
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Chapter 13, Problem 4PEB
To determine
The number of times Uranus rotated on its axis in the last
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Based on the orbital properties of Uranus, how far across the sky in arc seconds does it travel in one Earth
day? The average orbital radius is 2.88 x 109 km and the period is 84.0 years. (Assume Uranus and the Earth
are at the closest point to one another in their orbits.)
How many full Moons does this distance cover if the Moon has an angular diameter of 0.5 degrees?
Part 1 of 4
We first need to determine how fast the planet is moving across the sky. If we know the period and the
distance between the Sun and the planet we can calculate the velocity using:
2ar
which will tell us how many kilometers the planet travels in a day if we convert the period into days.
days
= (P
years'
|days/year
Pdays
days
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Uranus and neptune have almost similar masses. Which of them will exert the greater gravity towards the earth? Why? Explain
The Mars Robotic Lander for which we are making these calculations is designed to return samples of rock from Mars after a long time of collecting samples, exploring the area around the landing site, and making chemical analyses of rocks and dust in the landing area. One synodic period is required for Earth to be in the same place relative to mars as when it landed.
Calculate the synodic period (in years) using the following formula:
1/Psyn = (1/PEarth) - (1/PMars)
where PEarth is the sidereal period of the Earth (1 year) and PMars is the sidereal period of Mars.
If 3/4 of a Martian year was spent collecting samples and exploring the terrain around the landing site, calculate how long the Mars Robotic Lander expedition took!
Chapter 13 Solutions
Integrated Science
Ch. 13.1 - Prob. 1SCCh. 13.1 - Prob. 2SCCh. 13.1 - Prob. 3SCCh. 13.1 - Prob. 4SCCh. 13.1 - Prob. 5SCCh. 13.2 - Prob. 6SCCh. 13.2 - Prob. 7SCCh. 13.3 - Prob. 8SCCh. 13.3 - Prob. 9SCCh. 13.3 - Prob. 10SC
Ch. 13 - Describe the protoplanet nebular model of the...Ch. 13 - What are the basic differences between the...Ch. 13 - Prob. 3CQCh. 13 - Prob. 4CQCh. 13 - Prob. 5CQCh. 13 - Prob. 6CQCh. 13 - Prob. 7CQCh. 13 - Prob. 8CQCh. 13 - Prob. 9CQCh. 13 - Prob. 10CQCh. 13 - Prob. 11CQCh. 13 - Prob. 12CQCh. 13 - Prob. 13CQCh. 13 - Prob. 14CQCh. 13 - Prob. 15CQCh. 13 - Prob. 16CQCh. 13 - Prob. 17CQCh. 13 - Prob. 18CQCh. 13 - Prob. 19CQCh. 13 - What are the significant similarities and...Ch. 13 - Prob. 21CQCh. 13 - Prob. 22CQCh. 13 - Prob. 23CQCh. 13 - Prob. 24CQCh. 13 - Prob. 25CQCh. 13 - Prob. 1PEACh. 13 - Prob. 2PEACh. 13 - Prob. 3PEACh. 13 - Prob. 4PEACh. 13 - Prob. 5PEACh. 13 - Prob. 6PEACh. 13 - Prob. 1PEBCh. 13 - Prob. 2PEBCh. 13 - Prob. 3PEBCh. 13 - Prob. 4PEBCh. 13 - Prob. 5PEBCh. 13 - Prob. 6PEB
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- Which Jovian planet revolves on its side and has retrograde rotation? (16.5) (a) Jupiter (b) Neptune (c) Uranus (d) Saturnarrow_forwardThe Great Red Patch is the term given to the enormous red area on Jupiter's surface. Are there any predictions on how long it will take the planet to complete its rotation?arrow_forwardProminent on photos of Jupiter, is a large, reddish oval feature, named the Great Red Spot. How could this major feature be utilized to determine the rotation period of the planet?arrow_forward
- A)At what altitude would a geostationary sattelite need to be above the surface of Mars? Assume the mass of Mars is 6.39 x 1023 kg, the length of a martian solar day is 24 hours 39minutes 35seconds, the length of the sidereal day is 24hours 37minutes 22seconds, and the equatorial radius is 3396 km. The answer can be calculated using Newton's verison of Kepler's third law.arrow_forward) The diameter of the moon is about 11 million feet, and the diameter of Uranus is about170 million feet. If a scale model of the solar system is constructed so that the diameter of the moonis 1.2 feet, what will be the diameter of Uranus in feetarrow_forwardEstimate the length of period of Neptune assuming that the length of the semimajor axis of the ellipse is a = 449.51 x 101º m. For Earth, a = 15.0 × 1010 m. (Use decimal notation. Give your answer to two decimal places.)arrow_forward
- The Great Red Patch is the name given to Jupiter's large red spot.Is it possible to forecast how long it will take for the planet to complete its rotation?arrow_forwardWhy is pluto not considered a major planet? Explain.arrow_forwardEstimate in years how long summer lasts in Uranus's northern hemisphere.arrow_forward
- Calculate the semimajor axis of Jupiter given its orbital period as 11.862 years.arrow_forwardAsteroids are believed to be material that never collected into a planet. The asteroid Ceres has a period of 4.6 years. Assuming Ceres to be at the center of the planet if it had formed, how far would the planet be from the sun?arrow_forwardWhat is the observed angular speed of Neptune, along the ecliptic of Earth, when it is at opposition, in units of arc minutes / day? Presume the orbits are circular. Earth has orbital speeds of 30km/s and Neptune has 5.43km/s, Neptune here has orbital radius 30.1 AU. Now looking at Uranus for the same condition, in what direction along the ecliptic will it be traveling?arrow_forward
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