3 Chapter 3 – Why are there seasons?

OpenStax Astronomy Chapter 4 Section 2: The Seasons

Earth’s Tilt

I.                                          are due to Earth’s tilt

A.                          reasons:

1. The                                                                             is more                               when Earth is tilted                                  the Sun (Summer), energy is more concentrated

2. The Sun is in the sky                                                    in the                                       , more hours of daylight

B.                                               in                                          :                            direct sunlight, tilted away, Sun in sky                              time

C.                                                                                                                                   of the Northern Hemisphere

1. When the Northern Hemisphere is tilted toward the Sun, the Southern is tilted away

D. This has                                             to do with                                                          

1. Earth will be                              to the Sun in                                             and farthest in July because orbit not quite circular

Solstices and Equinoxes

From a Northern Hemisphere viewpoint 

II.                                                      :

A.                                                       Solstice

1. Sun most directly in direction of                                                                                              , farthest                               at sunrise/sunset

2.                                                  day – around                                 20 – 22 in Northern Hemisphere

3. Sun                                                    in sky it will ever get at noon

4.                                          Hemisphere – solstice in                                                  , Sun moves toward South Pole

B.                                                         Solstice

1. Sun most directly                                                      of North Celestial Pole, farthest                                               

2.                                                 day – around                                                    21 – 22 (Northern Hemisphere)

3. Sun                                                   at noon

III.                                                      :

A.                                                    (fall) Equinox

1. Sun on the                                                                                     where it crosses the ecliptic

2. Sun moving farther                                                   , lower, in sky

3.                                                                                     of day and night – around                                    22 – 23 (Northern Hemisphere)

4.                                                    Hemisphere – autumnal equinox is in                                    

B.                                                        (spring) Equinox

1. Sun again on the celestial equator, moving                                                    in sky

2. Equal hours of day and night – around                                                20 – 21 (Northern Hemisphere)

 

When would the sun be in the sky for the longest (most daylight hours)?

I.  Northern Hemisphere in June
II. Southern Hemisphere in June
III. Northern Hemisphere in December
IV. Southern Hemisphere in December

 

A.  I only
B.  II only
C.  I & II
D.  II & III
E.  I & IV

 

If the ecliptic was at the celestial equator, what would happen to the seasons?

A. Nothing. They would be the same.
B. Each season would be longer.
C. Each season would be shorter.
D. We would not have seasons.

Resources

NAAP Seasons and Ecliptic simulation: https://astro.unl.edu/naap/motion1/animations/seasons_ecliptic.html

 

 Tutorial Activity – Seasons

“Elementary Astronomy Worksheet Handout 3: Motions of Stars, Seasons” (modified by Kaisa E. Young) by Catherine Whiting via OER Commons, licensed under CC BY 4.0, https://oercommons.org/courses/elementary-astronomy-worksheets

 

1. What property of the Earth’s motion causes seasons? Explain the 2 reasons why that property causes seasons.

 

 

 

 

2. In Figure 1 below, label the positions of Earth when it is the Summer and Winter Solstices, and the Spring
(Vernal) and Fall (Autumnal) Equinoxes in the Northern Hemisphere. Also include the (approximate) dates when these occur.

Figure 1: ”Seasons” (modified by Catherine Whiting) by Andrew Fraknoi, David Morrison, and Sidney
Wolff via OpenStax, licensed under CC BY 4.0

 

3. When is the ecliptic (Sun):

a) High in the sky?

 

b) Low in the sky?

 

c) When does the Sun cross the Celestial Equator?

 

 

4. What would change about the Earth if its axis were tilted by 45° instead of 23.5°?

 

 

 

 

 

5. What would change about the Earth if the ecliptic lined up with the celestial equator?

 

 

 

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Astronomy of the Solar System Copyright © 2024 by Kaisa Young is licensed under a Creative Commons Attribution 4.0 International License, except where otherwise noted.

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