1.
| |
|
William Herschel thought he had found a comet when he spotted the green disk of: |
|
| Student Response | Correct Answer |
| Neptune. | |
| Oberon. | |
| Uranus. | |
| Titania. | |
| Triton. | |
|
Score: | 1/1 |
|
|
2.
| |
|
Uranus was discovered |
|
| Student Response | Correct Answer |
| less than 250 years ago. | |
| with a radio telescope. | |
| thousands of years ago. | |
| after examining perturbations in Neptune's orbit. | |
| by Galileo. | |
|
Score: | 1/1 |
|
|
3.
| |
|
Which three played a role in the finding of Neptune? |
|
| Student Response | Correct Answer |
| Adams, Leverrier, and Galle | |
| Herschel, Hubble, and Einstein | |
| Shapley, Hubble, and Whipple | |
| Bode, Herschel, and Fraunhofer | |
| Newton, Einstein, and Tombaugh | |
|
Score: | 1/1 |
|
|
4.
| |
|
In terms of axial tilt, which of the jovians shows us the largest inclination? |
|
| Student Response | Correct Answer |
| Neptune | |
| Pluto | |
| Uranus | |
| Jupiter | |
| Saturn | |
|
Score: | 1/1 |
|
|
5.
| |
|
The masses of Neptune and Uranus were first determined by |
|
| Student Response | Correct Answer |
| observations of their magnetic fields. | |
| observations of their motions around the Sun. | |
| their densities divided by their volumes. | |
| their compositions. | |
| observations of the motions of their satellites. | |
|
Score: | 1/1 |
|
|
6.
| |
|
Studying the magnetospheres of the jovians has allowed us to measure their |
|
| Student Response | Correct Answer |
| orbital period. | |
| rotation rates. | |
| orbital radius. | |
| ring system diameters. | |
| gravity. | |
|
Score: | 1/1 |
|
|
7.
| |
|
Unlike the other jovian planets, Uranus |
|
| Student Response | Correct Answer |
| rotates slowly. | |
| has a featureless atmosphere. | |
| has only a few satellites. | |
| has no internal energy source. | |
| has no ring system. | |
|
Score: | 1/1 |
|
|
8.
| |
|
The time between equinoxes on Uranus is about |
|
| Student Response | Correct Answer |
| 7 hours. | |
| 42 years. | |
| 21 years. | |
| 84 years. | |
| 8 hours. | |
|
Score: | 0/1 |
|
|
9.
| |
|
At the equator during the equinoxes on Uranus a day lasts |
|
| Student Response | Correct Answer |
| 21 years. | |
| 84 years. | |
| 7 hours. | |
| 8 hours. | |
| 42 years. | |
|
Score: | 1/1 |
|
|
10.
| |
|
Neptune and Uranus have a bluish tint because: |
|
| Student Response | Correct Answer |
| they are far away and distance makes objects appear bluish. | |
| ammonia ice reflects blue light better than any other color. | |
| their atmospheres contain methane, which absorbs red light. | |
| their atmospheres contain hydrogen and helium. | |
| at their distances, the Sun appears blue, the red absorbed by dust in the ecliptic. | |
|
Score: | 1/1 |
|
|
11.
| |
|
In 1989, Neptune was found to have a huge storm named the: |
|
| Student Response | Correct Answer |
| Hellas Basin. | |
| Great Dark Spot. | |
| Galileo Regio. | |
| Great Red Spot. | |
| South Tropical Disturbance. | |
|
Score: | 1/1 |
|
|
12.
| |
|
The most abundant component of the atmospheres of Uranus and Neptune is |
|
| Student Response | Correct Answer |
| Methane. | |
| Hydrogen. | |
| Nitrogen. | |
| Helium. | |
| Ammonia. | |
|
Score: | 1/1 |
|
|
13.
| |
|
In the atmospheres of the jovian planets, this component decreases, systematically, with distance from the Sun. |
|
| Student Response | Correct Answer |
| Hydrogen | |
| Methane | |
| Ammonia | |
| Nitrogen | |
| Helium | |
|
Score: | 0/1 |
|
|
14.
| |
|
Although the atmospheres of Uranus and Neptune are very similar, the atmosphere of Neptune contains more |
|
| Student Response | Correct Answer |
| Helium. | |
| Hydrogen. | |
| Nitrogen. | |
| Methane. | |
| Ammonia. | |
|
Score: | 0/1 |
|
|
15.
| |
|
The magnetic field tilts of which two bodies are the most unusual? |
|
| Student Response | Correct Answer |
| Uranus and Neptune | |
| Mars and Saturn | |
| Jupiter and Saturn | |
| Mercury and Earth | |
| Saturn and Venus | |
|
Score: | 1/1 |
|
|
16.
| |
|
In strength, the magnetic fields of Uranus and Neptune are: |
|
| Student Response | Correct Answer |
| perfect fits for the Dynamo theory. | |
| like Jupiter and Saturn, due to mantles of liquid metallic hydrogen. | |
| very different, with flopped over Uranus having no field, and Neptune a strong one. | |
| even stronger than that of Jupiter. | |
| similar, with both about 100 times stronger than our own. | |
|
Score: | 1/1 |
|
|
17.
| |
|
What is erupting out of the geysers on Triton? |
|
| Student Response | Correct Answer |
| liquid water with basalt | |
| liquid hydrogen with dark helium ash | |
| liquid methane with a dark hydrocarbon slush | |
| liquid carbon dioxide with graphite | |
| liquid nitrogen with carbon grit | |
|
Score: | 1/1 |
|
|
18.
| |
|
The rings of Uranus and Neptune are found: |
|
| Student Response | Correct Answer |
| in the ecliptic plane. | |
| outside the Roche limit. | |
| by the Hubble Space Telescope. | |
| above their equators. | |
| all of the above | |
|
Score: | 1/1 |
|
|
19.
| |
|
In addition to Saturn's Titan, which other moon has a nitrogen atmosphere? |
|
| Student Response | Correct Answer |
| Neptune's Triton | |
| Pluto's Charon | |
| Jupiter's Europa | |
| Uranus' Titania | |
| Jupiter's Ganymede | |
|
Score: | 1/1 |
|
|
20.
| |
|
The planet Neptune is |
|
| Student Response | Correct Answer |
| barely visible with the naked eye. | |
| only visible with a small telescope or binoculars. | |
| only visible with a space-based telescope. | |
| only visible with a large, high quality telescope. | |
| easily visible with the naked eye. | |
|
Score: | 0/1 |
|
|
21.
| |
|
Which of the Uranian moons displays the widest range of surface terrains, suggesting some catastrophic disruption? |
|
| Student Response | Correct Answer |
| Miranda | |
| Oberon | |
| Ariel | |
| Puck | |
| Umbriel | |
|
Score: | 1/1 |
|
|
No comments:
Post a Comment