Earth's Axis and Solar Radiation

Earth's Axis and Solar Radiation

Assessment

Interactive Video

Science, Geography, Physics

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video explains Earth's journey through space, focusing on its orbit and rotation. It describes Earth's elliptical orbit around the Sun, the difference between sidereal and solar days, and the concept of leap years. The video also covers Earth's rotational axis tilt and its impact on solar radiation distribution, leading to seasonal changes. The explanation includes how different latitudes receive varying amounts of solar radiation, affecting temperatures and seasons in both hemispheres.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the shape of Earth's orbit around the Sun?

Perfectly circular

Triangular

Square

Elliptical

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the average distance from Earth to the Sun?

100 million kilometers

150 million kilometers

200 million kilometers

250 million kilometers

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How long does it take for Earth to complete one rotation on its axis?

23 hours and 56 minutes

24 hours

22 hours and 50 minutes

25 hours

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the difference between a sidereal day and a solar day?

A sidereal day is twice as long as a solar day

They are the same length

A sidereal day is shorter than a solar day

A sidereal day is longer than a solar day

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why do we have leap years?

To synchronize with the lunar calendar

To account for the tilt of Earth's axis

To adjust for the Earth's elliptical orbit

To correct the calendar for the difference between a sidereal and solar day

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the tilt of Earth's rotational axis?

23.5 degrees

0 degrees

15 degrees

45 degrees

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the tilt of Earth's axis affect solar radiation?

It results in varying solar radiation at different latitudes

It causes solar radiation to be concentrated at the poles

It causes equal solar radiation at all latitudes

It has no effect on solar radiation

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