Grade 7Social Studies

Earth and the Solar System

The solar system; planets; Earth's rotation, revolution; effects of these on life.

📖 5 min read · 3 worked examples · 6 practice questions

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The lesson

Today we'll explore the Sun, the planets, and how our own Earth spins and travels around the Sun. First, notice the focus statement: our lesson centers on the natural and built environment of Kenya, connecting what we learn to everyday experiences like weather, daylight, and the seasons. Our key objectives are threefold: describe the Sun and each planet, explain how Earth's rotation gives us day and night, and understand how Earth's revolution creates the seasons. Think about a sunny morning in Nairobi—how the Sun's position changes throughout the day and across the year. We'll see how those changes are tied to the concepts we're about to learn. This shape outlines today's agenda. We'll start with the Sun, move on to the planets, then dive into Earth's rotation and revolution, and finally link everything back to life here in Kenya. I'll also ask a few quick checks along the way to make sure we're all on the same page.

Next, let's explore our Solar System overview. At the heart of everything is the Sun, our central star that provides the energy for all planets. Around it orbit the eight planets, from the rocky Mercury closest to the Sun, out to the icy Neptune farthest away. Notice this simple diagram: the Sun sits on the left, and the planets line up in order—Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune—each farther from the Sun. In Kenya, the Sun's height in the sky tells farmers when the rainy season will begin in the Rift Valley, influencing planting schedules for maize and beans. Remembering the Sun's central role helps us understand both the motion of planets and everyday life here at home.

Everyone, let's dive into today's topic: Earth's Rotation and Its Effects. One full spin of our planet takes about 24 hours, which gives us the cycle of day and night. When the side of Earth facing the Sun is lit, we have daylight; when it turns away, we experience darkness. Think about our daily routines—school starts when it's bright, and we finish when the sun sets. Even farming activities, like watering crops, are planned around these light periods. A quick note on the Coriolis effect: because Earth rotates, moving air is deflected, shaping wind patterns that influence the highlands of Kenya. This is why some regions get more rain than others. To recap, Earth's 24‑hour spin creates day and night, guides our daily schedules, and even affects weather patterns through the Coriolis effect. Any questions before we move on?

Let's explore Earth's revolution and how it creates the seasons we experience here in Kenya. One full revolution around the Sun takes about 365.25 days—that's what we call a year. Because of this extra quarter day, we add a leap day every four years. At this line chart showing the solar angle throughout the year for Nairobi. Notice how the angle rises and falls as Earth tilts toward and away from the Sun. When the solar angle is higher, we get more direct sunlight—this corresponds to our long rains season. When the angle is lower, the Sun's rays are more spread out, leading to the short rains and drier periods.

Worked examples

– Calculating Planet Distance

Class, let's dive into our worked example titled Worked Example 1 – Calculating Planet Distance. First, we note the given numbers: the average distance from Earth to the Sun is 149.6 million kilometres, and from Mars to the Sun it is 227.9 million kilometres. Step 1: we subtract the Earth‑Sun distance from the Mars‑Sun distance. Doing the math, 227.9 − 149.6 equals 78.3 million kilometres. The average distance between Earth and Mars is about 78.3 million km. This distance matters because any spacecraft traveling between the two planets must cover that span, influencing launch windows, fuel requirements, and mission timing. To recap, we identified the two orbital distances, subtracted them, and obtained the Earth‑Mars gap of roughly 78 million kilometres—a key figure for planning space missions.

– Estimating Day Length at the Equator

Everyone, let's dive into Worked Example 2: estimating the length of daylight at the Equator. First, notice the key point: at the Equator we get roughly twelve hours of daylight and twelve hours of night all year round. Why is that? Because the Earth's tilt of 23.5 degrees means the Sun's path is symmetrical above and below the equatorial plane, so every day the Sun spends the same amount of time above the horizon. Think about Kenya, which sits just a few degrees north of the Equator. That's why our daylight doesn't change dramatically between the dry and rainy seasons. To recap: the equatorial region enjoys about 12 hours of daylight year‑round, the Earth's tilt explains the variation at higher latitudes, and Kenya's near‑equatorial location gives us fairly constant daylight.

– Determining Seasonal Change

All right, let's dive into Worked Example 3, where we'll determine the seasonal change by looking at when the Sun is directly overhead at the Tropic of Cancer. First, notice the bullet point: the Sun is overhead at the Tropic of Cancer around June 21, which is the summer solstice in the Northern Hemisphere. Why does this matter for Kenya? Even though Kenya lies just south of the equator, the slight tilt means we experience a modestly cooler and drier period when the Sun is highest over the Tropic of Cancer. We can use this seasonal cue to plan our maize planting: aim to sow just after the cooler, drier spell so the crops benefit from the upcoming rains. In summary, the Sun's position on June 21 signals a brief cooling in Kenya, and that timing helps us decide the optimal month for planting maize.

Practice questions

  • Remember: the Earth spins on its axis, which gives us day and night. It also travels around the Sun – that's called revolution – and the tilt of its axis is what creates the seasons.
  • Take a moment, and when you're ready, submit your answers. Afterward we'll go over the key points together so any confusion disappears.
  • Remember, the first question asks you to think about Earth's daily spin—if it turns once every 24 hours, how many turns does it make in a full week? Just multiply the daily rotation by the number of days.
  • For the planet ordering, picture the solar system like a bus route starting at the Sun. List each stop from closest to farthest, and then mark which stops are rocky, terrestrial worlds.
  • When you explain Kenya's short dry season, connect it to the movement of the Inter‑Tropical Convergence Zone and how the country's position near the equator brings quick shifts in wind patterns.
  • The distance problem is a simple subtraction: when Earth and Venus are on opposite sides of the Sun, add their distances from the Sun and you'll have an estimate of how far apart they are.

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