Lesson 9 Flashcards
Why do jovian planets bulge around the equator, that is, have a “squashed” appearance?
Their rapid rotation flings the mass near the equator outward
How many more times is the atmospheric pressure in Jupiter’s core greater than the atmospheric pressure at Earth’s surface?
100 million
Why is Jupiter denser than Saturn?
The extra mass of Jupiter compresses its interior to a greater extent than that of Saturn.
Why is Saturn almost as big as Jupiter, despite its smaller mass?
Jupiter’s greater mass compresses it more, thus increasing its density.
Why do the jovian planet interiors differ?
Accretion took longer further from the Sun, so the more distant planets formed their cores later and captured less gas from the solar nebula than the closer jovian planets.
The belts and zones of Jupiter are
alternating bands of rising and falling air at different latitudes.
Why are there no impact craters on the surface of Io?
Io did have impact craters but they all have been buried in lava flows.
What causes synchronous rotation?
A massive planet exerts a tidal force on a moon that causes the moon to align itself such that its tidal bulges always point toward and away from the planet.
What mechanism is most responsible for generating the internal heat of Io that drives the volcanic activity?
tidal heating
Which moon has the most substantial atmosphere?
Titan
Why does Titan have such a nitrogen-rich atmosphere?
The nitrogen comes from the breakup of ammonia (NH3) by solar radiation and subsequent thermal escape of the hydrogen.
Why do astronomers believe Triton may have been a planet that was captured by Neptune?
It orbits Neptune in the opposite direction of Neptune’s rotation.
Why are Saturn’s rings so thin?
Any particle in the ring with an orbital tilt would collide with other ring particles, flattening its orbit
What is the Cassini division of Saturn’s rings?
a large gap, visible from Earth
Which of the following best describes the internal layering of Jupiter, from the center outward?
core of rock, metal, and hydrogen compounds; thick layer of metallic hydrogen; layer of liquid hydrogen; layer of gaseous hydrogen; cloud layer