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ASTR Exam 1
| Question | Answer |
|---|---|
| Two stars in the same constellation | may actually be very far apart from one another |
| Beijing and Philadelphia have about the same latitude but very different longitudes. Therefore, tonight's night sky in these two places: | will look about the same. |
| When it is summer in Australia, it is: | winter in the United States. |
| If the Sun rises precisely due east: | it must be the day of either the spring or fall equinox. |
| The fact that we always see the same face of the Moon tells us that: | the Moon's rotation period is the same as its orbital period. |
| In winter, Earth's axis points toward the star Polaris. In spring: | the axis also points toward Polaris. |
| A week after full moon, the Moon's phase is: | third quarter. |
| If there is going to be a total lunar eclipse tonight, then you know that: | the Moon's phase is full. |
| When we see Saturn going through a period of apparent retrograde motion, it means: | Earth is passing Saturn in its orbit, with both planets on the same side of the Sun. |
| Total solar eclipses and total lunar eclipses often happen two weeks apart. Which kind of eclipse can more people witness with their own eyes? | far more people could see the total lunar eclipse |
| Which of the following was not a major advantage of Copernicus's Sun-centered model over the Ptolemaic model? | It made significantly better predictions of planetary positions in our sky. |
| When we say that a planet has a highly eccentric orbit, we mean that: | in some parts of its orbit it is much closer to the Sun than in other parts. |
| Earth is closer to the Sun in January than in July. Therefore: | Earth travels faster in its orbit around the Sun in January than in July. |
| According to Kepler's third law: | Jupiter orbits the Sun at a faster speed than Saturn. |
| Galileo's contribution to astronomy included: | making observations and conducting experiments that dispelled scientific objections to the Sun-centered model. |
| Suppose you visit another planet: | Your mass would be the same as on Earth, but your weight would be different. |
| Consider the statement "There's no gravity in space." This statement is: | Completely false. |
| As an interstellar gas cloud shrinks in size, its gravitational potential energy: | gradually is transformed into other forms of energy. |
| If Earth were twice as far from the Sun, the force of gravity attracting Earth to the Sun would be: | one-quarter as strong. |
| According to the law of universal gravitation, what would happen to Earth if the Sun were somehow replaced by a black hole of the same mass? | Earth's orbit would not change. |
| Earth is located at one _____ of the Moon's orbit. | Focus |
| According to Kepler's second law, Jupiter will be traveling most slowly around the Sun when at ______. | Aphelion |
| Earth orbits in the shape of an ______ around the Sun. | Ellipse |
| The mathematical form of Kepler's third law measures the period in years and the _____ ____ in astronomical units. | Semimajor Axis |
| According to Kepler's second law, Pluto will be traveling fastest around the Sun when at _______. | Perihelion |
| The extent to which Mars' orbit differs from a perfect circle sis called its _______. | Eccentricity |
| A solar eclipse that occurs when the new moon is too far from Earth to completely cover the Sun can be either a partial solar eclipse or an _____ ______. | Annular eclipse |
| Anyone looking from the night side of Earth can see a _____ _____ ______. | Total lunar eclipse |
| During some lunar eclipses, the Moon's appearance changes only slightly, because it passes only through the part of Earth's shadow called the ______. | Penumbra |
| A _____ _____ ______ can occur only when the Moon is new and has an angular size larger than the Sun in the sky. | Total solar eclipse |
| A partial lunar eclipse beings when the Moon first touches Earth's _____. | Umbra |
| A point at which the Moon crosses Earth's orbital plane is called a ____. | Node |