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ASTRO 101 - Final Exam Questions And Answers 100% Pass

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constellations and the moon appear to move across the sky at night because - the earth spins on its axis T/F: in one day Earth rotates exactly once around it's axis - false What causes Earth's seasons? - 23.5 degree tilt of Earth's rotational axis a total lunar eclipse occurs - during the full moon phase T/F: our galaxy is about 1 million times bigger than Earth - false T/F: The stars in a constellation are physically close to one another - false T/F: The Solar Day is longer than a Sidereal Day - true T/F: The seasons are caused by the precession of Earth's axis - false T/F A lunar eclipse can occur only during the full phase. - true T/F: The angular diameter of an object is inversely proportional to its distance from the observer - true T/F: If we know the distance of an object from Earth, we can determine the object's size by measuring its parallax - false If Earth rotated twice as fast as it currently does, but its motion around the Sun stayed the same,

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ASTRO 101 - Final Exam Questions And Answers 100% Pass
constellations and the moon appear to move across the sky at night because - ✔✔✔the earth spins on its axis




T/F: in one day Earth rotates exactly once around it's axis - ✔✔✔false




What causes Earth's seasons? - ✔✔✔23.5 degree tilt of Earth's rotational axis




a total lunar eclipse occurs - ✔✔✔during the full moon phase




T/F: our galaxy is about 1 million times bigger than Earth - ✔✔✔false




T/F: The stars in a constellation are physically close to one another - ✔✔✔false




T/F: The Solar Day is longer than a Sidereal Day - ✔✔✔true




T/F: The seasons are caused by the precession of Earth's axis - ✔✔✔false




T/F A lunar eclipse can occur only during the full phase. - ✔✔✔true




T/F: The angular diameter of an object is inversely proportional to its distance from the observer - ✔✔✔true




T/F: If we know the distance of an object from Earth, we can determine the object's size by measuring its parallax - ✔✔✔false




If Earth rotated twice as fast as it currently does, but its motion around the Sun stayed the same, then - ✔✔✔the night would be half as long




When a thin crescent of the Moon is visible just before sunrise, the Moon is in its - ✔✔✔waning phase




If the Moon's orbit were a little larger, solar eclipses would be - ✔✔✔more likely to be annular




If the Moon orbited Earth twice as fast, but in the same orbit, the frequency of solar eclipses would - ✔✔✔stay the same




Considering the Moon's phases, everyone on Earth sees - ✔✔✔the same phase in 24 hours




How did the geocentric model account for day and night on Earth? - ✔✔✔the sun orbited the earth




Copernicus' important contribution to astronomy was - ✔✔✔proposing a model that easily explained the retrograde motion of the planets

,Who published the first astronomical observations made with a telescope? - ✔✔✔Galileo




Earth is closer to the Sun in January than in July. Therefore, in accord with Kepler's second law: - ✔✔✔Earth orbits faster in January




how many meters in 3.6 kilometers? - ✔✔✔36,100



1 km =



place the following prefixes in order from smallest to largest:

micro

centi

nano

milli - ✔✔✔nano

micro

milli

centi



Match the prefix with the scientific notation for the order of magnitude of the number.

kilo

mega

giga

tera



a. 10^3

b. 10^12

c. 10^9

d. 10^6 - ✔✔✔kilo - a. 10^3

mega - d. 10^6

giga - c. 10^9

tera - b. 10^12



Calculate, using Newton's law of gravity, the size of the force of attraction between Earth and a mass of 9.52 kg located on the surface of Earth. Data: Distance to
the center of Earth from the surface = 6370 km. Mass of Earh = 5.98x1024 kg. Gravitational constant G=6.67x10-11 Nm2/kg2 - ✔✔✔92.3




T/F: Aristotle proposed that all planets revolve around the sun - ✔✔✔false




T/F: During retrograde motion, planets actually stop and move backward in space. - ✔✔✔false

, T/F: The heliocentric model of the universe holds that Earth is at the center and everything else moves around it. - ✔✔✔false




T/F: Copernicus's theories gained widespread scientific acceptance during his lifetime. - ✔✔✔false




T/F Galileo's observations of the sky were made with the naked eye. - ✔✔✔false




T/F The speed of a planet orbiting the Sun is independent of the planet's position in the orbit - ✔✔✔false




T/F: Keppler's laws only hold for the 6 planets known in his time - ✔✔✔false




T/F: You throw a baseball to someone, before the ball is caught, it is temporarily in orbit around the Earth's center - ✔✔✔true




a major flaw in copernicus's model was that it still had - ✔✔✔circular orbits




a calculation of how long it would take a planet to orbit the sun would be closely related to Kepler's - ✔✔✔third law of planetary distances




If Earth's orbit around the Sun were twice as large as it is now, the new year would be - ✔✔✔more than 2 current earth years




An asteroid with an orbit lying entirely inside Earth's - ✔✔✔has an orbital semi-major axis of less than 1 AU




Newton's law of gravity states that the force between two objects - ✔✔✔increases with mass




Gravity is - ✔✔✔always an attractive force




in this wave motion people stand up and sit down as the wave passes, what type of wave is this? - ✔✔✔transverse




the distance between successive wave crests defines the ____ of a wave - ✔✔✔wavelength




which of these is not a form of electromagnetic radiation - ✔✔✔sound waves



Rigel appears as a bright bluish star, whereas

Betelgeuse appears as a bright reddish star.

Rigel is ______ Betelgeuse. - ✔✔✔hotter than




T/F: The wavelength of green light is about the size of an atom - ✔✔✔false

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