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Understanding Fast Radio Bursts and Cosmic Microwave Background

Understanding Fast Radio Bursts and Cosmic Microwave Background

Assessment

Interactive Video

Physics

11th - 12th Grade

Practice Problem

Hard

Created by

Jennifer Brown

FREE Resource

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are fast radio bursts (FRBs) characterized by?

Infrared emissions

Visible light emissions

Quick flashes of broad frequency radio emissions

Long-lasting radio emissions

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was the significant discovery about fast radio bursts in March 2016?

They are visible to the naked eye

They originate from the Milky Way

They are caused by supernovae

A fast radio burst repeated itself

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How far did the cosmic microwave background photons travel to reach us?

10 billion light years

13.7 billion light years

5 billion light years

20 billion light years

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was the universe filled with before the moment of recombination?

Only hydrogen gas

Dark matter

Plasma, atomic nuclei, and free electrons

Solid matter

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the Thomson scattering cross-section?

A measure of the size of protons

A measure of the size of electrons

A measure of the interaction region for electrons

A measure of the interaction region for protons

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the mean free path in the context of photon travel?

The average distance between stars

The distance between two galaxies

The distance light travels in a year

The average distance a photon travels before hitting an electron

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was the estimated electron density at the moment of recombination?

0.2 electrons per cubic meter

200 million electrons per cubic meter

10 electrons per cubic meter

1 billion electrons per cubic meter

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