10 Jun PHSC 1203 – When rounded to the nearest day, the Sun takes
Question
Question:Question:Question 1
When rounded to the nearest day, the Sun takes approximately____ days to drift around the entire sky, while the Moon takes approximately___ days.
Question 2
Match the appropriate moon phase to the description given.
The phase between waxing gibbous and waning gibbous.
[ Choose ] full moon new moon first quarter last quarter
The phase between waxing crescent and waxing gibbous.
[ Choose ] full moon new moon first quarter last quarter
The phase between waning gibbous and waning crescent.
[ Choose ] full moon new moon first quarter last quarter
The phase between waning crescent and waxing crescent.
[ Choose ] full moon new moon first quarter last quarter
Question 3
Tonight is a full moon. Three nights from now, the moon’s phase will be [ Select ] [“waning gibbous”, “waning crescent”, “waxing gibbous”, “waxing crescent”] . Roughly a week from now, the moon’s phase will be [ Select ] [“last quarter”, “first quarter”] . Ten nights from now, the moon’s phase will be [ Select ] [“waning crescent”, “waxing gibbous”, “waxing crescent”, “waning crescent”] .
Question 4
Why does the Moon’s appearance change over the course of its cycle of phases?
Question 5
eclipses occur when the Moon’s shadow falls upon the Earth, which can happen during the moon phase. On the other hand, eclipses occur when the Earth’s shadow falls upon the Moon, which can occur during the moon phase.
Question 6
Why don’t eclipses occur dozens of times over the course of a year?
Question 7
Which of these are planets that are visible to the naked eye from Earth’s surface?
the Moon
Mars
Uranus
Mercury
Pluto
Jupiter
Saturn
Neptune
Venus
Question 8
Typically, the planets drift ward through the night sky from night to night, much like the Moon. However, they occasionally exhibit motion in which they appear to drift ward.
Question 9
The ptolemaic model of the universe is a centric model with the at its center.
The model supported by Copernicus and Kepler is a centric model with the at its center.
Question 10
Kepler’s first law states that the shape of the orbits of the planets is , with the Sun at one .
Kepler’s second law states that, if a line is drawn between a planet and the Sun, equal are swept out in equal times. In other words, planets move when closer to the Sun.
c. Kepler’s third law states that the square of a planet’s orbital is proportional to the cube of the planet’s average orbital .
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