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Aphelion and Perihelion

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Format: Interactive (Online), Printable (PDF)
Grades: 6
Subjects: science
Standards: MS-ESS1-1: DEVELOP AND USE A MODEL OF THE EARTH-SUN-MOON SYSTEM TO DESCRIBE THE CYCLIC PATTERNS OF LUNAR PHASESECLIPSES OF THE SUN AND MOONAND SEASONS.
Languages: English, Spanish

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About this reader

This engaging reading passage, 'Aphelion and Perihelion,' delves into the fascinating aspects of Earth's elliptical orbit around the Sun. Students will learn about the two key points in our planet's journey: Aphelion, when Earth is farthest from the Sun, and Perihelion, when it is closest. The passage explains how these orbital positions, combined with Earth's tilt, influence our seasons. Key terms like 'orbit,' 'elliptical,' 'axis,' and 'seasons' are defined clearly for a Grade 6 reading level. This content aligns with NGSS MS-ESS1-1, helping students develop a model of the Earth-sun system to describe cyclic patterns. The passage and activities are audio integrated, making it accessible for all learners.

Written by Workybooks TeamPublished by Workybooks

Sample passage and quiz content

CONTENT PREVIEW

"Perihelion aphelion semimajor axis" by Maxmath12 / Wikimedia Commons.

Have you ever wondered why we have different seasons? Many people think that seasons are caused by how close Earth is to the Sun. It seems logical, right? When Earth is closer, it should be hotter, and when it's farther away, it should be colder. However, this common idea isn't entirely accurate! The true reason for seasons is more fascinating and has to do with Earth's axial tilt, not its distance from the Sun.

Earth travels around the Sun in an oval-shaped path called an elliptical orbit. This means Earth's distance from the Sun changes throughout the year. The point in Earth's orbit when it is farthest from the Sun is called aphelion. This usually happens around early July. The point when Earth is closest to the Sun is called perihelion, which occurs around early January.

Now, let's think about this. If being closer meant hotter, then January should be summer for everyone, and July should be winter. But that's not what happens! In the Northern Hemisphere, July is typically summer, and January is winter. This is because the Earth's distance from the Sun, even at aphelion, does not cause the seasons. The difference in distance is actually quite small compared to the overall distance.

So, what does cause seasons? The answer is Earth's axial tilt. Earth's axis, an imaginary line running through the North and South Poles, is tilted at an angle of about 23.5 degrees relative to its orbit. This tilt remains pointed in the same direction in space as Earth orbits the Sun. Imagine a spinning top that's leaning over – that's a bit like Earth!

Because of this tilt, different parts of Earth receive more direct sunlight at different times of the year. When the Northern Hemisphere is tilted towards the Sun, it receives more direct sunlight, and the sun's rays hit the surface at a steeper angle. This means the sunlight is more concentrated and spreads over a smaller area, leading to warmer temperatures and longer days – this is summer. At this time, the Southern Hemisphere is tilted away from the Sun, receiving less direct sunlight, resulting in winter.

Conversely, when the Southern Hemisphere is tilted towards the Sun, it experiences summer, while the Northern Hemisphere has winter. Aphelion, when Earth is farthest from the Sun, actually occurs during the Northern Hemisphere's summer. Even though Earth is slightly farther away, the Northern Hemisphere is tilted towards the Sun, receiving direct solar radiation, which outweighs the small difference in distance.

Think of it like this: a flashlight beam pointed directly at a surface makes a small, bright circle. That's like direct sunlight in summer. If you tilt the flashlight, the beam spreads out over a larger, dimmer area. That's like indirect sunlight in winter. The amount of energy received per square foot makes a big difference in temperature.

Therefore, while Earth's elliptical orbit and its aphelion and perihelion points are real, they are not the primary cause of seasons. It's the consistent tilt of Earth's axis that determines how much direct sunlight each hemisphere receives throughout the year, leading to the distinct patterns of our global climate and seasons. Understanding Earth's orbit around the Sun and its axial tilt is key to understanding our planet's seasonal cycles.

Fun Fact: During aphelion, Earth is about 3 million miles (4.8 million kilometers) farther from the Sun than it is during perihelion, which is a small fraction of the average 93 million miles (150 million kilometers) distance!

What is the main cause of Earth's seasons?

Earth's axial tiltEarth's distance from SunMoon's gravitational pullAmount of clouds

What is aphelion?

Farthest point from SunClosest point to SunEarth's fastest speedLongest day of year

Why does direct sunlight cause warmer temperatures?

Sunlight is more concentratedEarth spins fasterMore clouds appearOceans absorb heat

When the Northern Hemisphere has summer, what season is it in the Southern Hemisphere?

WinterSummerSpringAutumn

How does Earth's axial tilt affect the angle of sunlight?

Creates direct or indirect raysChanges Sun's colorBlocks all sunlightSpeeds up orbit

If Earth had no axial tilt, how would seasons be different?

No distinct seasonsOnly extreme seasonsSeasons would be longerMore predictable weather

What season is it in the Northern Hemisphere during aphelion?

SummerWinterSpringAutumn

Why is the difference in Earth-Sun distance not the main cause of seasons?

Distance change is smallEarth's orbit is circularSun's heat varies greatlyMoon blocks the sun

If a planet's axis was tilted 90 degrees, how would its seasons compare to Earth's?

More extreme seasonsLess noticeable seasonsNo seasons at allShorter seasonal cycles

Imagine Earth's tilt suddenly changed to 0 degrees. How would this impact the amount of sunlight at the poles?

Always receive similar sunlightOne pole always darkMore extreme light/darkNo impact on sunlight

Aphelion and Perihelion

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