Exoplanets and Stellar Observations

Exoplanets and Stellar Observations

Assessment

Interactive Video

Physics, Science

7th - 12th Grade

Hard

Created by

Emma Peterson

FREE Resource

The video discusses the challenges of discovering exoplanets, contrasting the direct observation method with indirect methods like the transit method and Doppler shift. It highlights the difficulty of finding exoplanets due to their small size and distance from Earth. The video also mentions the discovery of over 1800 exoplanets by 2014 using these methods. Additionally, it includes a sponsorship message from Audible, recommending Isaac Asimov's 'Foundation'.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Who discovered Pluto after examining photographic plates for half a year?

Isaac Newton

Albert Einstein

Clyde Tombaugh

Galileo Galilei

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a major challenge in directly observing exoplanets?

Exoplanets are too small to see

Stars are too bright compared to their planets

Stars are too close to each other

Exoplanets move too quickly

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary method used to discover most exoplanets?

Observing effects on parent stars

Listening for radio signals

Using gravitational lensing

Direct observation

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What happens to a star's brightness when a planet passes in front of it?

It becomes darker

It becomes brighter

It remains the same

It changes color

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What percentage of Earth-like planets have the right orbital orientation for the transit method?

Around 50%

About 10%

More than 90%

Less than 1%

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the radial velocity method used for?

Measuring the size of a planet

Detecting a star's wobble

Calculating a planet's temperature

Determining a star's age

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What causes the wobble in a star's motion detected by the radial velocity method?

The star's rotation

The gravitational pull of orbiting planets

Nearby black holes

Cosmic radiation

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