Understanding Solar Time Concepts

Understanding Solar Time Concepts

Assessment

Interactive Video

Mathematics, Physics, Science

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

Harold York, a research scientist, explains how to calculate the hour angle of the Sun. The hour angle is the angle the Earth must rotate for the Sun to appear at high noon. At high noon, the angle is 0 degrees, and it changes by 15 degrees per hour. To calculate it, you need the local solar time, which can be determined using a sundial or by converting clock time to Universal Time, then to mean local solar time, and finally to local solar time using the time equation. The video covers these steps in detail, including adjustments for time zones and longitude.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the hour angle of the Sun at high noon?

15 degrees

45 degrees

0 degrees

30 degrees

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the hour angle of the Sun one hour before high noon?

-15 degrees

0 degrees

30 degrees

15 degrees

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

If it is 1:30 PM, what is the hour angle of the Sun?

45 degrees

30 degrees

22.5 degrees

15 degrees

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How do you calculate the hour angle if the local solar time is 2 hours before high noon?

Multiply 2 by 20

Multiply 2 by 15

Multiply 2 by 25

Multiply 2 by 10

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What tool can be used to determine local solar time directly?

A thermometer

A sundial

A compass

A clock

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How many hours should be added to Pacific Standard Time to convert it to Universal Time during daylight saving?

5 hours

7 hours

8 hours

6 hours

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the longitude of Pasadena, California, used for calculating mean local solar time?

110.14 degrees

100.14 degrees

118.14 degrees

120.14 degrees

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