2.5: Seasons and Latitude
- Page ID
- 39714
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Latitude
One of the biggest factors affecting a location’s climate is the location’s latitude – the distance from the equator (the equator represents a latitude of 0° and the poles are 90°N for the North Pole, and 90°S for the South Pole). Figure \(\PageIndex{1}\) displays lines of latitude on Earth for the Northern Hemisphere.
We’ll cover latitude more in depth when we investigate the Earth’s coordinate system in a future investigation. For now, just know that the further away you get from the equator, the larger your latitude is.
The key impact that latitude has on climate is the impact that it has on the angle of incoming sunlight, or the Angle of Insolation. To demonstrate the importance of the angle of insolation, do the following experiment:
Using a flashlight and in a dark room, hold the flashlight so that the light is directly over the ground Figure \(\PageIndex{2}\). Then, tilt the flashlight so it is low on the horizon Figure (\(\PageIndex{3}\)).

- When the flashlight is shining directly above the surface (Figure 2.5.2), the area illuminated on the surface is:
- A small, bright circle
- A large, dim area
- Now lower the flashlight on the horizon (Figure 2.5.3). The area illuminated on the surface becomes:
- Smaller and brighter
- Larger and Dimmer
- It doesn’t change
We can apply these conclusions to sunlight and how its intensity changes throughout the day. Specifically, when the sun is high in the sky, the incoming sunlight is more intense, whereas when the sun is low on the horizon, the incoming sunlight is less intense.
Now let’s take a look at how this would relate to latitude. There are a few things to note here:
- If the Earth were NOT tilted, the sun would be directly overhead year-round, and the overall set-up of incoming sunlight would look something like Figure \(\PageIndex{3}\)

Figure \(\PageIndex{4}\): Sunlight over the Equator (low latitude) vs. Sunlight near the poles (high latitude). - Sun is directly over the Equator. (CC BY 4.0; Alicia Mullens). Alternative description of image.
- Based on Figure 2.5.4, a beam of sunlight covers a __________________ area over higher latitudes than near the Equator.
- Smaller
- Larger
- As a result, the sunlight over the higher latitudes would be ________________________ than near the Equator (hint: if the beam covers a smaller area, it is more concentrated… if it covers a larger area, it is more diluted).
- More Intense
- Less Intense
This can be further reinforced with a quick look at how air temperatures vary with latitude across the world. A map of global average air temperatures is shown in Figure \(\PageIndex{5}\).
- While there is some variation caused by other factors (such as elevation, and ocean currents), the warmest temperatures are generally near the _________________ while the coldest temperatures are generally near the ____________________.
- Poles;Equator
- Equator;Poles
Earth’s orbit.
However, our Earth IS tilted. In fact, it is tilted at an Angle of 23.5°. The result of this is that as the Earth orbits around the sun (Figure \(\PageIndex{6}\)), the latitude that the sun is directly overhead changes. Figure \(\PageIndex{7}\) represents the conditions in June, when the sun is directly over 23.5°N, while Figure \(\PageIndex{8}\) represents the conditions in December, when the sun is directly over 23.5°S.
- Investigate the North Pole in Figure \(\PageIndex{7}\). Notice that it is completely covered with sunlight. Now imagine the Earth making one 24 hour rotation (with the North pole as the axis of rotation). In June, the North Pole would never:
- Experience any Sunlight
- Experience any Darkness
-
Now let’s investigate Figure \(\PageIndex{8}\), which represents conditions in December. In December, the sun is directly over.
-
The Equator - 23.5°N
- 23.5°S
-

