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Review figure 7.7 in section 7.4. What is the approximate orbital radius of Jupiter? a. 20 AU b. 1 AU c. 6 AU d. 10 AU e. 15 AU

Review figure 7.7 in section 7.4. What is the approximate orbital radius of Jupiter? a. 20 AU b. 1 AU c. 6 AU d. 10 AU e. 15 AU

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Review figure 7.7 in section 7.4. What is the approximate orbital radius of Jupiter? a. 20 AU b. 1 AU c. 6 AU d. 10 AU e. 15 AU
phys.libretexts.org next. This means that planets orbiting the r any central massive object like the Sun) should have orbital velocities that decrease with the square root of their distance from that object. This relationship is plotted for our Solar System in. Figure 7.7 below. A plot of velocity vs. distance is known as a rotation curve. 5x10 2:08 3.75x10 2.50x10 1.25x10 Mercury Earth Mars Asteroid Ceres Satum Uranus 20 Neptune Orbital Radius, AU Figure 7.7: The velocities of the planets are plotted as a function of their distance. The rotation curve illustrates that the orbital velocities decrease with the square root of their distance from the Sun. Note: the sizes of the planets are not to scale. Credit: NASA/SSU/Aurore All planets in our Solar System follow this relation, but stars in galaxies do not. They follow a different relation that is specific to the details of those systems. However, it is still derived from the laws of gravity. We can substitute an expression with time for expressions i How can we help %D 00 S of plane
Transcribed Image Text:phys.libretexts.org next. This means that planets orbiting the r any central massive object like the Sun) should have orbital velocities that decrease with the square root of their distance from that object. This relationship is plotted for our Solar System in. Figure 7.7 below. A plot of velocity vs. distance is known as a rotation curve. 5x10 2:08 3.75x10 2.50x10 1.25x10 Mercury Earth Mars Asteroid Ceres Satum Uranus 20 Neptune Orbital Radius, AU Figure 7.7: The velocities of the planets are plotted as a function of their distance. The rotation curve illustrates that the orbital velocities decrease with the square root of their distance from the Sun. Note: the sizes of the planets are not to scale. Credit: NASA/SSU/Aurore All planets in our Solar System follow this relation, but stars in galaxies do not. They follow a different relation that is specific to the details of those systems. However, it is still derived from the laws of gravity. We can substitute an expression with time for expressions i How can we help %D 00 S of plane
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