
Biosignatures and Exoplanet Detection

Interactive Video
•
Biology, Chemistry, Science
•
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
What is the main challenge when trying to detect life on Earth from a distance?
The Earth's atmosphere is too thick.
The Earth is too small to be seen.
The complexity of life is hard to capture in a single image.
The Earth's rotation makes it difficult to observe.
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What significant contribution did the Kepler Space Telescope make to exoplanet discovery?
It discovered life on an exoplanet.
It was the first telescope to take images of exoplanets.
It discovered the first exoplanet.
It confirmed the existence of nearly 4,000 exoplanets.
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How can scientists estimate the size and mass of an exoplanet?
By detecting radio signals from the planet.
By analyzing the light blocked when the planet passes in front of its star.
By observing the star's color.
By measuring the planet's temperature.
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is a biosignature?
A method of communication with extraterrestrial life.
A type of star that supports life.
A chemical indicator that suggests the presence of life.
A natural process that creates life.
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Why is methane not a definitive biosignature?
It is only produced by intelligent life.
It can be created by both biological and non-biological processes.
It is only found on Earth.
It is too rare to be detected.
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What did Carl Sagan's Galileo experiment reveal about Earth's biosignatures?
Earth's biosignatures suggest a chemical disequilibrium.
Earth's biosignatures are unique and easily detectable.
Earth has no detectable biosignatures.
Earth's biosignatures are identical to those on Mars.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the 'vegetation red edge'?
A biosignature indicating the presence of chlorophyll.
A technique for measuring a planet's temperature.
A type of exoplanet with abundant vegetation.
A method of detecting water on exoplanets.
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