
Understanding Cepheid Variables in Astronomy

Interactive Video
•
Physics
•
9th - 10th Grade
•
Hard

Patricia Brown
FREE Resource
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10 questions
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1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What was the main challenge astronomers faced before 1912 regarding stars?
Determining the age of stars
Measuring the distance to stars accurately
Understanding the lifecycle of stars
Identifying the chemical composition of stars
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What causes the brightness of Cepheid variables to change?
The star's size
The star's distance from Earth
The presence of helium in the star's atmosphere
The rotation speed of the star
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What did Henrietta Leavitt discover about Cepheid variables?
Their color changes over time
They are the largest stars in the universe
Their period is unrelated to their brightness
Their period is directly related to their brightness
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the significance of the period of a Cepheid variable?
It determines the star's color
It is directly related to the star's brightness
It is unrelated to the star's brightness
It indicates the star's age
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How did Leavitt's discovery help astronomers measure star distances?
By allowing them to calculate the star's temperature
By identifying the star's chemical composition
By measuring the star's gravitational pull
By providing a way to determine a star's true brightness
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What significant discovery did Edwin Hubble make using Cepheid variables?
The existence of black holes
The expansion of the universe
The age of the Milky Way
The Andromeda nebula is a separate galaxy
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What was the impact of identifying Cepheid variables on measuring distances in the universe?
It limited distance measurements to a few hundred light-years
It expanded distance measurements to a nearly limitless range
It made distance measurements irrelevant
It only helped measure distances within the Milky Way
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