

Transit Method for Detecting Exoplanets
Interactive Video
•
Physics, Science, Other
•
9th - 10th Grade
•
Practice Problem
•
Easy
Patricia Brown
Used 1+ times
FREE Resource
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10 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the primary principle behind the transit method for discovering extrasolar planets?
Analyzing the star's magnetic field
Measuring the star's temperature
Observing light dimming when a body passes in front of a star
Detecting gravitational waves
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How is the transit method similar to a solar eclipse?
Both are caused by the Earth's rotation
Both involve a celestial body blocking light from a star
Both result in a permanent change in the star's brightness
Both involve the complete disappearance of the star
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What can the transit method detect when applied to smaller celestial bodies like Venus or Mercury?
The speed of the celestial body
The temperature of the celestial body
The dimming of light as the body passes in front of the sun
The color of the celestial body
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
Why is it important to observe regular intervals of light dimming in the transit method?
To calculate the star's mass
To determine the star's distance from Earth
To measure the star's age
To confirm the presence of a planet
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What distinguishes a planet from other celestial bodies like asteroids or comets in the transit method?
The size of the light dimming
The regularity of the dimming periods
The speed of the light dimming
The color of the light dimming
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is a key indicator that a celestial body is orbiting a star in the transit method?
Irregular light dimming
Increasing light intensity
Constant light intensity
Regular periods of light dimming
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How does the transit method help in identifying extrasolar planets?
By measuring the star's temperature changes
By detecting regular dimming of the star's light
By observing the star's color changes
By analyzing the star's magnetic field
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