21st Century Astronomy 6E
6th Edition
ISBN: 9780393690675
Author: Laura Kay, Stacy Palen, George Blumenthal
Publisher: W. W. Norton
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Chapter 11, Problem 15QP
To determine
The affect of the volcanoes of Enceladus on the E Ring of Saturn.
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Ovals, spots, and storms do not appear prominently in the atmosphere of Saturn because the
a.
temperature is too low.
b.
temperature is too high.
c.
atmospheric chemistry does not permit their development.
d.
atmosphere is too dense.
e.
planet’s ring system interferes with storms.
Belt-zone circulation is not easily visible on Uranus because
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no clouds form in the pure hydrogen atmosphere.
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there is no differential rotation.
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clouds form very deep in the atmosphere.
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that atmosphere is stirred by cyclonic circulation.
e.
there is no liquid metallic core.
The odd orbits of Nereid and Triton, which are moons of Neptune, indicate that these
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moons were captured.
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moons formed simultaneously with the planet from the same piece of the solar nebula.
c.
moons broke off from the rapidly rotating planet.
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e.
orbits were disturbed long ago in an interaction with some other body.
Chapter 11 Solutions
21st Century Astronomy 6E
Ch. 11.1 - Prob. 11.1CYUCh. 11.2 - Prob. 11.2ACYUCh. 11.2 - Prob. 11.2BCYUCh. 11.3 - Prob. 11.3CYUCh. 11.4 - Prob. 11.4CYUCh. 11 - Prob. 1QPCh. 11 - Prob. 2QPCh. 11 - Prob. 3QPCh. 11 - Prob. 4QPCh. 11 - Prob. 5QP
Ch. 11 - Prob. 6QPCh. 11 - Prob. 7QPCh. 11 - Prob. 8QPCh. 11 - Prob. 9QPCh. 11 - Prob. 10QPCh. 11 - Prob. 11QPCh. 11 - Prob. 12QPCh. 11 - Prob. 13QPCh. 11 - Prob. 14QPCh. 11 - Prob. 15QPCh. 11 - Prob. 16QPCh. 11 - Prob. 17QPCh. 11 - Prob. 18QPCh. 11 - Prob. 19QPCh. 11 - Prob. 20QPCh. 11 - Prob. 21QPCh. 11 - Prob. 22QPCh. 11 - Prob. 23QPCh. 11 - Prob. 24QPCh. 11 - Prob. 25QPCh. 11 - Prob. 26QPCh. 11 - Prob. 27QPCh. 11 - Prob. 28QPCh. 11 - Prob. 29QPCh. 11 - Prob. 31QPCh. 11 - Prob. 32QPCh. 11 - Prob. 33QPCh. 11 - Prob. 34QPCh. 11 - Prob. 35QPCh. 11 - Prob. 36QPCh. 11 - Prob. 37QPCh. 11 - Prob. 38QPCh. 11 - Prob. 40QPCh. 11 - Prob. 41QPCh. 11 - Prob. 42QPCh. 11 - Prob. 43QPCh. 11 - Prob. 44QPCh. 11 - Prob. 45QP
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- The rings of Uranus were discovered a. during an occultation (an eclipse) of a star. b. during an eclipse of one of the moons by the rings. c. during an eclipse of Uranus by the rings. d. as Uranus and the rings passed behind Jupiter. e. by the Voyager 1 spacecraft.arrow_forwardThe high-speed winds, high-level white clouds of methane ice crystals, and cyclonic circulations on Neptune are produced by the a. large amount of heat from the sun that is received at Neptune’s distance. b. small amount of heat from the sun and the flow of heat from the interior of the planet. c. strong magnetic field of the planet. d. flow of heat from the interior of the planet. e. unusually rapid rotation of the planet.arrow_forward14. Saturn's rings a. were created by its incredibly large gravitational capture of asteroids and comets b. have looked basically the same since they formed along with Saturn c. are continually supplied by impacts into small moons d. were created long ago when tidal forces tore apart a large moonarrow_forward
- Earth-based telescopic observations of Neptune reveal a. a bluish-green disk with no visible surface detail. b. white clouds and a dark blue spot. c. belt-zone circulation as seen on Jupiter and Saturn. d. rapidly rising and sinking convection currents of different shades of blue. e. cyclonic storms near the planet’s equator.arrow_forwardThe narrowness of the rings of Uranus and Neptune is believed to be caused by a. gravitational interactions between ring particles. b. a spiral density wave which confines them. c. the magnetic field which holds them in place. d. the smaller mass of Uranus and Neptune as compared to that of Saturn. e. small shepherd moons that orbit near the rings.arrow_forwardAlthough Deimos is smaller than Phobos, Deimos has more debris on its surface. This difference in the two moons is probably the result of a. the greater number of impact craters on Deimos. b. Martian gravity, which is strong enough to pull debris off the surface of Phobos. c. the lack of volcanic activity on the surface of Phobos. d. the comparatively weaker gravity on Deimos. e. the slower rotation rate of Deimos on its axis.arrow_forward
- Saturn, as viewed through a telescope, appears as a a. spherical and heavily cratered object. b. bland and nearly featureless disk. c. disk composed of brightly colored belts and bands. d. highly elliptical and bright blue disk.arrow_forwardBecause of the lack of a temperature difference between the equator and poles of Jupiter, the a. cyclonic circulations on Earth are duplicated on Jupiter. b. high- and low-pressure regions are drawn into bands by the planet’s rapid rotation. c. belt-zone circulation is only a temporary phenomenon. d. belt-zone circulation is exceptionally stable. e. belt zone circulation is an illusion produced by the interaction of sunlight and chemicals in the Jovian atmosphere.arrow_forwardAstronomers concluded that there were several rings around Uranus when a. telescopic observations confirmed their existence. b. the light from an occulted (eclipsed) star repeatedly dimmed as the planet approached and again after it passed. c. the Voyager spacecraft photographed the ring system in visible light. d. Earth-based infrared telescopes examined the dust band around Uranus. e. reflected light from the ring particles was detected by orbiting spacecraft.arrow_forward
- How can Jupiter have a liquid interior and not have a definite liquid surface?arrow_forwardDescribe the composition of Saturn from its center outward. What causes these different internal layers?arrow_forwardDescribe and compare the rings of Saturn and Uranus, including their possible origins.arrow_forward
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