Have you ever looked up at the sky and wondered about Earth and what lies beyond it? Let's explore our solar system, learn how Earth moves, and discover phenomena like eclipses, gravity, and more.
In this lesson, we will also see how astronomers (scientists who study space) figured all these things out. Let's begin our journey from Earth to the edges of the Milky Way.
Our solar system is like a cosmic neighborhood with various members. At the center is the Sun, which is a star (a giant ball of hot glowing gas). Everything in the solar system orbits (travels around) the Sun. The major members of the solar system include eight planets, many moons, and other smaller bodies like asteroids and comets.
There are eight official planets in our solar system, in order from the Sun outward:
A handy way to remember the order is by using a mnemonic. For example: My Very Educated Mother Just Served Us Noodles – the first letter of each word stands for Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune. You can even try making your own funny sentences!
You might wonder, "Where is Pluto?" Pluto used to be called the ninth planet, but in 2006 astronomers reclassified it as a dwarf planet. It's still out there, orbiting the Sun, but it's now part of a group of smaller "dwarf planets."
Our solar system has five recognized dwarf planets (like Pluto, Ceres, Eris, etc.) in addition to the eight main planets. So, while Pluto isn't one of the main eight anymore, it's still an interesting world at the edge of the solar system.
It's important not to mix up stars, planets, and moons. The Sun is a star – the only star in our solar system. Planets (like Earth, Jupiter, etc.) are huge spheres that do not produce their own light; they shine by reflecting the Sun's light. At night when you see "stars," you are seeing other stars far outside our solar system. Those are not planets in our system.
Moons are smaller objects that orbit planets. For example, Earth's Moon orbits Earth. Other planets have their own moons (also called natural satellites). Moons shine by reflecting sunlight too. So remember: planets orbit a star (the Sun), and moons orbit planets. Stars (like the Sun) are huge and produce light, whereas planets and moons are relatively smaller and mostly just reflect light.
For a long time, Jupiter was known to have the most moons. But as of recent discoveries, Saturn has surpassed Jupiter in the number of known moons. Saturn is known to have at least 82 moons (and counting!). Jupiter is not far behind (around 79–80 known moons as of a couple years ago).
Why does Saturn have so many? One reason is its strong gravity. Big planets like Saturn and Jupiter have a strong gravitational pull that can capture many smaller objects as moons. Saturn's largest moon is Titan, which is even bigger than Mercury! In contrast, some planets have few or no moons: Mercury and Venus have 0 moons, Earth has 1, Mars has 2 small moons, the gas giants (Jupiter, Saturn, Uranus, Neptune) each have dozens of moons of various sizes.
Earth is much smaller than Saturn and has weaker gravity to grab moons. Also, our part of the solar system has fewer leftover chunks to become moons. This shows how different each planet can be.
Apart from moons, there are also asteroids (rocky bodies, mostly in the asteroid belt between Mars and Jupiter) and comets (icy bodies that develop glowing tails when near the Sun) in the solar system. All these things together – the Sun, eight planets, moons, asteroids, comets, and dwarf planets – make up our solar system.
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Our planet Earth is always in motion, even if we don't feel it. This can be tricky to imagine, and many students wonder about it. The reason is that Earth's movement is very smooth and constant. It's a bit like riding in a car or airplane at a steady speed – you only feel movement if the vehicle speeds up, slows down, or turns. Earth's spin and orbit don't have sudden changes, so we don't notice them in our bodies. But we do see the effects of Earth's motion in the sky.
There are two main types of motion Earth has: rotation and revolution.
To avoid confusion: rotation = spinning in place; revolution/orbit = traveling around something else. An easy comparison: "The Earth rotates on its axis, and revolves around the Sun." Rotation gives us day/night, and revolution (combined with the tilt of Earth's axis) gives us seasons.
Here's a quick reference:
Term | Meaning | Effect |
Rotation | Spinning on an axis | Causes day and night (24 hours for Earth) |
Revolution (Orbit) | Traveling around another object | Causes a year (Earth ~365 days) and seasons (with axial tilt) |
The reason we don't feel Earth's rotation or revolution? It's because the motions are steady. Earth's rotation speed at the equator is about 1670 km/hour – incredibly fast, but we are carried smoothly along. Also, the atmosphere (air around us) moves with Earth, so there's no rushing wind from Earth's spin.
You might have heard of solar eclipses and lunar eclipses. These special events happen due to the alignments of the Sun, Earth, and Moon.
Why don't we have eclipses every month? The Moon's orbit is tilted about 5° relative to Earth's orbit around the Sun. Most of the time the Moon is slightly above or below the exact line between Earth and Sun.
Earth's atmosphere is the layer of gases surrounding our planet. It's often called a blanket of air.
Earth's atmosphere is primarily made of 78% nitrogen and 21% oxygen, with tiny amounts of other gases like argon and carbon dioxide.
Roles of the Atmosphere:
Our atmosphere gradually thins out and fades into space. About 100 km (62 miles) up is considered the "edge of space."
Earth, our Sun, and all the planets are part of a much larger structure called a galaxy – the Milky Way.
Solar System < Galaxy < Universe
Almost everything we've learned about "Earth and beyond" comes from astronomers.
Astronomers:
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