Planets of the Solar System
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.
Giants of science
“If I have seen further, it is by standing on the shoulders of giants”
Isaac Newton
Léon Foucault
–
Johannes Kepler
–
Become a giant
The Radio Sky II: Observational Radio Astronomy
The Radio Sky I: Science and Observations
Our Place in the Universe
The History of Ancient Environments, Climate, and Life
Our Global Ocean – An Introduction Course
Introduction to Deep Earth Science
Sensing Planet Earth – Water and Ice
Professional development for Educators
Teach teens computing: Impact of technology
Introduction to Data Wise: A Collaborative Process to Improve Learning & Teaching
Teach teens computing: Programming in Python
Teach teens computing: Cybersecurity
Giants of science
“If I have seen further, it is by standing on the shoulders of giants”
Isaac Newton
Johannes Kepler
–
Nicolaus Copernicus
–
Become a giant
The Radio Sky II: Observational Radio Astronomy
The Radio Sky I: Science and Observations
Our Place in the Universe
Introduction to Deep Earth Science
Sensing Planet Earth – Water and Ice
Our Global Ocean – An Introduction Course
The History of Ancient Environments, Climate, and Life
Professional development for Educators
HP Digital Skills for Educators – Microsoft 365 Copilot
Teach computing: Moving from Scratch to Python
Teach teens computing: How computers work
Higher education teaching in the age of AI
Test your knowledge
What criteria are used to classify the planets of the solar system, and what does this classification reveal about their origin and composition?
How does each planet contribute to our overall understanding of the solar system’s dynamics and evolution?
Why are the planets so far apart from each other?
Why do some planets have rings while others don’t?
Why don’t planets crash into each other if they’re all moving?
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