Pulsars and Their Effects

Pulsars and Their Effects

Assessment

Interactive Video

Physics

11th - 12th Grade

Practice Problem

Hard

Created by

Patricia Brown

FREE Resource

The lecture discusses the energy content and loss in pulsars, comparing their slowdown to Earth's rotation due to tidal forces. It explains rotational kinetic energy and how pulsars lose energy over time. The energy output of pulsars is compared to the Sun, revealing pulsars emit energy equivalent to 100,000 suns. The lecture also explores the existence of planets around pulsars and their potential effects.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What causes the Earth to slow down its rotation over time?

Magnetic field interactions

Gravitational pull from the Sun

Atmospheric friction

Tidal forces due to the Moon

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the formula for calculating the rotational kinetic energy of a pulsar?

F = ma

mgh

1/2 mv^2

1/2 Iω^2

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the main source of energy loss in a pulsar?

Rotational kinetic energy

Nuclear fusion

Magnetic field decay

Gravitational waves

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How often does the pulsar inside the Crab Nebula complete one rotation?

Every 1 second

Every 0.033 seconds

Every 10 seconds

Every 0.1 seconds

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the energy loss of a pulsar compare to the energy output of the Sun?

It is equal to the Sun's energy output

It is half of the Sun's energy output

It is ten times the Sun's energy output

It is a hundred thousand times the Sun's energy output

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the approximate energy output of the Sun every second?

6 x 10^26 joules

2 x 10^26 joules

4 x 10^26 joules

8 x 10^26 joules

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What causes the nebula around a pulsar to light up?

The presence of dark matter

The gravitational pull of nearby stars

The pulsar's vast energy output

The pulsar's magnetic field

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