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.
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A: In this, it is asking about the unique feature of Enceladus.
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Q: Explain how the terrestrial and Jovian planets came to be so unlike.
A: This question explains about the terrestrial and Jovian planets came to be so unlike.
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Q: What advantages do large telescopes have over smaller ones? a. larger collecting areas b. both…
A: telescopes are used to get the information about the far most foreign bodies.
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Q: Why are the lunar mountains smooth and rounded rather than having sharp, pointed peaks?…
A: Thee lunar mountains smooth and rounded rather than having sharp, pointed peaks.
Q: Which process is primarily responsible for heating the interiors of many of the moons of Jupiter and…
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Q: What is the Roche limit, and what does it have to do with planetary rings?
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Q: Which of the following events can NOT be explained by a giant impact event? O The large metallic…
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Q: What is the range of density for the outer planets (in g/cm3)? 1.2 to 5.5 2.2 to 5.5 2.2 to 6.5 3.3…
A: Outer planets are less dense and having density about 1 g/cm3.
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Q: Explain how the terrestrial planets and Jupiter's planets became so different.
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Q: UESTION 3 The surface of Venus receives a. a lot more sunlight than the surface of the Earth…
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Q: On the "canteloupe" hemisphere of Neptune's moon Triton, we see channels that were carved by liquid…
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Q: 22. The Solar System A. formed about 14 billion years ago. B. formed about 4.5 billion years ago. C.…
A: The Solar System is formed about 4.5 billion years ago.
Q: The parallel grooves seen on the surface of Phobos may indicate that a. the moon formed elsewhere
A: We have to know about the basic here.
Q: Given the information below, use an energy balance to determine the surface temperature of the…
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Q: 15) Why is heat flow the key to understanding a planet's surface activity?
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Q: The ring particles around Jupiter are very small, as evidenced by the observation that light a.…
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Q: Which of these is not a criteria for the success of a solar system formation theory?
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Q: Pluto’s density is 1.8 g/cm 3. This implies that Pluto
A: We know that, density= mass/volume
Q: What allows moons of Jupiter and Saturn to have liquid interiors?
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a. |
spherical and heavily cratered object.
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b. |
bland and nearly featureless disk.
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c. |
disk composed of brightly colored belts and bands.
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d. |
highly elliptical and bright blue disk.
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