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Planets of the Solar System

09/06/2026

The solar system planetary simulations online on this page will allow you to deepen your knowledge about the planetary system in which the Earth is located. You will learn about the inner and outer planets and you will visualize the characteristics of the motion of some of them.

This Thematic Unit is part of our Earth Sciences collection

STEM OnLine mini dictionary

Albedo

Proportion of sunlight that a planetary surface reflects back into space.

Earth

Third planet from the Solar System, the only one with confirmed life and surface liquid water.

Eccentricity

Measure of how much a planet’s orbit deviates from being a perfect circle.

Jupiter

The largest planet in the Solar System, a gas giant composed mainly of hydrogen and helium.

Mars

Fourth planet, called the Red Planet due to the iron oxide on its surface.

Neptune

The planet farthest from the Sun, an ice giant with the strongest winds in the Solar System.

Orbital Period

Time it takes for a planet to complete one full revolution around the Sun.

Rotation Period

Time it takes for a planet to rotate once on its own axis.

Saturn

Gas giant famous for its extensive and bright ring system.

Uranus

Ice giant with a highly tilted rotation axis, almost parallel to its orbit.

Venus

Second planet in the Solar System, known for its dense carbon dioxide atmosphere and high temperatures.

The planets of the solar system

The solar system is a planetary system composed of eight main planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. Each planet has unique characteristics that distinguish them and make them fascinating.

Inner planets of the solar system

The inner planets of the solar system, also known as terrestrial or rocky planets, are the planets that are closest to the Sun. They have a rocky composition and are relatively small in size compared to the outer planets.

Mercury, the world of extreme temperatures

Mercury is the planet closest to the Sun and the smallest in the entire solar system, only slightly larger than Earth’s Moon. Lacking a significant atmosphere capable of retaining heat or moderating temperatures, Mercury experiences the most extreme temperature fluctuations in the solar system: during the day, the surface reaches a scorching 430 degrees Celsius, while at night it drops dramatically to 180 degrees below zero. Its rocky, grayish surface is completely pockmarked with thousands of impact craters caused by asteroids and comets, an intact geological record due to the absence of wind or water to erode the landscape. Furthermore, the planet has an extremely high density, indicating that its interior is dominated by a gigantic iron core that occupies nearly 85% of its radius.

Venus, hell under a global greenhouse

Venus is often referred to as Earth’s twin planet because the two share very similar sizes, masses, and internal compositions. However, at the surface level, it is a radically inhospitable world. Venus has the densest atmosphere of the rocky planets, composed almost entirely of carbon dioxide and shrouded in perpetual clouds of sulfuric acid. This dense layer of gases traps massive amounts of solar radiation, generating a runaway greenhouse effect that constantly raises the surface temperature to 465 degrees Celsius, making it the hottest planet in the solar system, surpassing even Mercury. Its atmospheric pressure is crushing, equivalent to being nearly a kilometer deep beneath Earth’s oceans, and its surface is dominated by vast volcanic plains and rivers of solidified lava.

Earth, the oasis of liquid water and life

Earth is the largest of the four inner planets and the only place in the known universe to date that supports life. The fundamental characteristic that defines our planet is the abundance of liquid water, which covers approximately 71% of the surface in the form of oceans. Earth has a balanced atmosphere, rich in nitrogen and oxygen, which not only protects us from harmful solar radiation and impacts from smaller meteorites but also regulates the global climate to maintain moderate temperatures. Geologically, it is an extremely dynamic world and the only one with active plate tectonics; this constant movement of the crustal plates renews the landscape, raises mountain ranges, generates volcanic activity, and helps recycle carbon, allowing for a climatic stability that has made possible the evolution of an immense biodiversity of ecosystems.

Mars, the rust-colored desert and the promise of exploration

Mars, commonly known as the Red Planet, has fascinated humanity due to its historical resemblance to Earth. Its characteristic reddish color is due to the abundance of iron oxide (rust) in the dust and rocks that cover its surface. Although today it is a frozen desert with an extremely thin atmosphere of carbon dioxide and very low surface pressure, space missions have uncovered irrefutable evidence that in the past, liquid water flowed across Mars’ surface, with rivers, lakes, and even a vast northern ocean. The planet is home to colossal geological features, such as Mount Olympus, the largest volcano in the solar system at 22 kilometers high, and Valles Marineris, a massive rift valley that spans one-third of the planet. It has two small captured moons, Phobos and Deimos, and is currently the primary target of robotic exploration and future crewed missions in search of traces of ancient microscopic life.

Outer planets of the solar system

The outer planets of the solar system, also known as giant or gas planets, are farther from the Sun and have distinctive characteristics compared to the inner planets.

Jupiter, the colossal giant and the engine of the solar system

Jupiter is the largest planet in the entire solar system; its mass is more than double that of all the other planets combined, and its interior could hold more than a thousand Earths. It is a gas giant composed almost entirely of hydrogen and helium, similar to a star that never went through nuclear fusion. Its atmosphere is an extremely dynamic and violent environment, crisscrossed by bands of colorful clouds and hurricane-force winds. Jupiter’s most famous feature is the Great Red Spot, a gigantic anticyclonic storm that has been active for at least three hundred years and is larger than the diameter of Earth. Jupiter possesses a powerful magnetic field and has more than ninety moons, notably the four discovered by Galileo: Io, Europa, Ganymede, and Callisto.

Saturn, the jewel of the solar system and the lord of the rings

Saturn is the second-largest planet in the solar system and is world-famous for its spectacular and complex ring system. Although other gas giants also have rings, Saturn’s are the only ones visible with simple telescopes from Earth and are composed of billions of fragments of pure ice, dust, and rock, ranging in size from microscopic particles to boulders the size of a house. Physically, Saturn is the least dense planet in the solar system; its density is lower than that of water, meaning it would float in a sufficiently large ocean. Its gaseous atmosphere displays yellowish bands and features seasonal storms, as well as a fascinating storm shaped like a perfect hexagon at its north pole.

Uranus, the ice giant that orbits on its side

Uranus belongs to a subclass of outer planets known as ice giants, as its internal composition includes a thick mantle of frozen water, ammonia, and methane surrounding a rocky core. The methane gas in its upper atmosphere is responsible for absorbing red light and giving it its characteristic pale blue-green color. The most astonishing feature of Uranus is its extreme axial tilt: its axis of rotation is tilted nearly ninety-eight degrees, meaning the planet orbits practically “lying” on its side. As a result, its poles experience periods of absolute sunlight and darkness that last forty-two Earth years each.

Neptune, the blue world of supersonic winds

Neptune is the planet farthest from the Sun and the last of the ice giants. Its size and internal composition are very similar to those of Uranus, but it appears a much more intense and brilliant blue due to subtle differences in the chemistry of its atmosphere. Neptune is an extremely dynamic and cold world, home to the fastest and most violent storms in the entire solar system, with supersonic winds reaching speeds of over 2,000 kilometers per second—twice the speed of a passenger airplane. Giant dark vortices similar to Jupiter’s Great Red Spot have been observed in its atmosphere, and it has a fascinating primary moon, Triton, an icy world that orbits the planet in the opposite direction of Neptune’s rotation.

Galilean satellites and other objects in the solar system

In addition to these planets, the solar system also harbors other fascinating objects.

The Galilean satellites, discovered by Galileo Galilei in 1610, are the four largest satellites of Jupiter: Io, Europa, Ganymede and Callisto. These celestial bodies stand out for their unique characteristics and their relevance in astronomy. Io is the most volcanically active object in the solar system, with more than 400 active volcanoes. Europa, with its icy surface, is a prime candidate for the search for extraterrestrial life due to the possibility of having a subsurface ocean. Ganymede is the largest satellite in the solar system, even larger than the planet Mercury, and has its own magnetic field. Callisto, on the other hand, presents a surface full of craters and it is believed that it could also have an ocean under its crust.

Pluto, although no longer officially considered a planet, is an icy dwarf object orbiting beyond Neptune. There are also asteroids, comets, and small bodies known as dwarf planets, such as Ceres and Eris, scattered throughout the solar system.

Exploring the planets of the solar system

These planets and celestial objects have been explored in detail by space missions, such as those of NASA, ESA and other international space agencies. As we continue to research and learn about the solar system, more secrets and wonders are revealed that allow us to better understand our place in the universe.

STEM OnLine mini dictionary

Albedo

Proportion of sunlight that a planetary surface reflects back into space.

Earth

Third planet from the Solar System, the only one with confirmed life and surface liquid water.

Eccentricity

Measure of how much a planet’s orbit deviates from being a perfect circle.

Jupiter

The largest planet in the Solar System, a gas giant composed mainly of hydrogen and helium.

Mars

Fourth planet, called the Red Planet due to the iron oxide on its surface.

Neptune

The planet farthest from the Sun, an ice giant with the strongest winds in the Solar System.

Orbital Period

Time it takes for a planet to complete one full revolution around the Sun.

Rotation Period

Time it takes for a planet to rotate once on its own axis.

Saturn

Gas giant famous for its extensive and bright ring system.

Uranus

Ice giant with a highly tilted rotation axis, almost parallel to its orbit.

Venus

Second planet in the Solar System, known for its dense carbon dioxide atmosphere and high temperatures.

Explore the exciting STEM world with our free, online, simulations and accompanying companion courses! With them you’ll be able to experience and learn hands-on. Take this opportunity to immerse yourself in virtual experiences while advancing your education – awaken your scientific curiosity and discover all that the STEM world has to offer!

Simulations of the planets of the solar system

Inner planets of the solar system


In this first one of the online solar system planet simulations, you can see the motion of Mercury, Venus and the Earth along their orbits around the Sun. Observe how, due to their different translation speeds, the distances between the planets and the angular position of Mercury and Venus with respect to the Earth change.

Apparent motion of Venus


In this animation you can see the apparent motion of Venus as seen from the Earth.

Apparent motion of Mars


See what the motion of Mars is like with respect to the Earth and how it approaches or moves away, due to the different translation velocities of Mars and the Earth.

Galilean moons


In this last of the online solar system planet simulations, the motion of the Galilean moons, the four largest of those orbiting Jupiter: Io, Europa, Ganymede and Callisto, is depicted.

“If I have seen further, it is by standing on the shoulders of giants”

Isaac Newton

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The planets of the solar system are mainly classified into inner or rocky planets—Mercury, Venus, Earth and Mars—and outer or giant planets—Jupiter, Saturn, Uranus and Neptune. This division reflects clear differences in composition, size and distance from the Sun. The inner planets are small, dense and made of solid materials such as iron and silicates, while the outer planets are much larger and composed mostly of gases or ices. This classification reveals that the solar system formed from a protoplanetary disk where temperature decreased with distance from the Sun: close to it, only heavy materials could condense, whereas farther away, lighter gases and volatile compounds accumulated. The current distribution of planets is therefore not random but a direct consequence of the physical conditions present during the formation of the solar system.
Each planet provides essential clues about the history and evolution of the solar system. Rocky planets help us study processes such as atmospheric formation, geological activity and the presence of water in the past. Mars, for example, offers evidence of ancient climates and potentially habitable conditions. Gas giants like Jupiter and Saturn reveal how mass was distributed in the early solar system and how their strong gravity shaped the movement of asteroids and comets. Uranus and Neptune, classified as ice giants, show the role of compounds such as methane and ammonia in colder regions far from the Sun. Together, the planets act as layers of information that allow scientists to reconstruct how the solar system formed, how it changed over time and why its components are arranged as they are today.
Because the solar system formed from a cloud of gas and dust that spread out as it rotated around the Sun. Planets formed only in regions where enough material gathered, leaving huge gaps between them. Later, the gravity of the giant planets pushed many objects outward, increasing the distances even more. Their spacing isn’t random—it reflects how matter was distributed when the solar system was born.
Rings are made of ice, dust and rock fragments trapped by a planet’s gravity. Gas giants like Saturn or Jupiter have much more mass, so they can hold large amounts of material around them. Rocky planets are too small to maintain such structures. It’s not that they couldn’t have rings, but they don’t have enough gravitational pull to keep them stable.
Because each planet follows a stable orbit around the Sun. These orbits are well separated and don’t cross. The Sun’s gravity keeps every planet in its path, preventing them from drifting too close to one another. Even though they move very fast, they do so in an orderly and predictable way, which is why collisions don’t happen.

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