
Estimating Star Ages and Characteristics

Interactive Video
•
Physics, Science, Biology
•
9th - 12th Grade
•
Hard

Patricia Brown
FREE Resource
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10 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Why is it difficult to determine the age of a star?
Stars are too far away to study.
Stars change their composition frequently.
Stars do not have a birth certificate.
Stars are too bright to observe closely.
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens to a star when it runs out of hydrogen fuel in its core?
It becomes a red giant.
It becomes a black hole.
It turns into a neutron star.
It explodes immediately.
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How do scientists estimate the age of a group of stars in a cluster?
By analyzing their chemical composition.
By plotting them on a Hertzsprung-Russell diagram.
By measuring their distance from Earth.
By observing their gravitational pull.
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the main sequence in the context of star clusters?
A phase where stars are invisible.
A line on the H-R diagram where stars are burning hydrogen.
A phase where stars are dying.
A line on the H-R diagram where stars are born.
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What observation in the 1970s helped scientists estimate the age of stars?
Stars in older clusters have more elements than those in young clusters.
Stars in young clusters are larger than those in older clusters.
Stars in older clusters are brighter than those in young clusters.
Stars in young clusters spin faster than those in older clusters.
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Why is measuring a star's rotation not always reliable for determining its age?
Stars stop rotating after a certain age.
Stars' rotation rates become constant after burning half their fuel.
Stars' rotation rates are too fast to measure accurately.
Stars' rotation rates vary too much to be useful.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the most accurate way to measure the age of a single star?
By measuring its distance from Earth.
By tracking how its brightness changes over time.
By analyzing its chemical composition.
By observing its gravitational pull.
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