The Solar System
The Solar System
10th Edition
ISBN: 9781337672252
Author: The Solar System
Publisher: Cengage
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Chapter 2, Problem 14P
To determine

The number of precession periods in inclination change of one cycle of Earth’s axis, eccentricity variation of Earth’s orbit, and number of periods or period fractions of precision of Earth’s axis, nod, and change in shape of Earth’s orbit in time span given in figure 2.11b and also identify which one has more influence on changes plotted in figure 2.11.

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Mars is 1.5 times as far away from the Sun as Earth.  Earth’s axis is tilted at 23.5o compared to the ecliptic.  The axis of Mars is tilted at 25o compared to the ecliptic.   The atmosphere on Earth is 100 times as thick as the atmosphere on Mars.  Which of the following statements is true?     1.)Mars is so cold that the water there is ice, while Earth does not have any ice 2.)When it is summer in Earth’s northern hemisphere, it is winter on Mars’ southern hemisphere 3.) Earth has seasons, Mars does not 4.) All of the water on Mars is frozen, while Earth has water in solid, liquid and gas form
A planet's speed in orbit is given by     V = (30 km/s)[(2/r)-(1/a)]0.5   where V is the planet's velocity, r is the distance in AU's from the Sun at that instant, and a is the semimajor axis of its orbit.  Calculate the Earth's velocity in its orbit (assume it is circular):        What is the velocity of Mars at a distance of 1.41 AU from the Sun?       What is the spacecraft's velocity when it is 1 AU from the Sun (after launch from the Earth)?       What additional velocity does the launch burn have to give to the spacecraft? (i.e. What is the difference between the Earth's velocity and the velocity the spacecraft needs to have?)        How fast will the spacecraft be traveling when it reaches Mars?       Does the spacecraft need to gain or lose velocity to go into the same orbit as Mars?
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…

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