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Explore the solar system in real time in 3D. Observe the planets, their positions and orbits. Navigate freely in the solar system by clicking on the keys to move forward or backward in time and observe the movement of the planets. Zoom in, rotate the view, move with the mouse or keyboard, select a planet and track its trajectory over time. The 'measure' feature displays in real time the exact distance between two planets, materialized by clear and precise lines. The 'telescope' mode displays a rectangular area to observe distant objects and analyze the details of planets and satellites.

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Real-time exploration of the solar system

Observe, explore and navigate the solar system freely.

Composition of the solar system

The solar system is the planetary system of the sun, it is composed of 8 planets that orbit it with their moons.
Four of these planets (Mercury, Venus, the Earth and Mars) are telluric (rocky) and the other four (Jupiter, Saturn, Uranus, Neptune) are gaseous.
The sun alone contains 99.85% of the total mass of the solar system and dominates it gravitationally.
Between Mars and Jupiter, there is the asteroid belt (the main belt) composed of billions of asteroids not aggregated into planets. Beyond Neptune lies the Kuiper belt which, like the asteroid belt, is composed of remnants of the solar system's formation.

The Sun: a giant star

The Sun is a star, that is to say a very hot ball of gas, composed mainly of hydrogen and helium. It is located at the center of the solar system and exerts a force of gravity that keeps the planets in their orbits. The Sun is also our main source of light and heat, without which life on Earth would not be possible.

Position of the planets in real time

The planets gravitate around the Sun in the same direction as its rotation, which is counterclockwise from above the north pole.
Click on a planet to observe its position in real time or visit our page ephemeris

You can also move forward or backward in time (-3 years in the past and +3 years in the future) and measure the distance between two planets. For this, use the arrows and commands placed on the dashboard.

Heliocentric planetary positions

EclipticCartesian
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The coordinates are given in the barycentric heliocentric reference frame, expressed in astronomical units (AU).

Inclination, rotation and revolution of the planets

In addition to revolving around the Sun, the planets also rotate on themselves. They rotate for the most part in the same direction as around the Sun except for some like Venus which turns in the opposite direction of its revolution.

Observe the real-time rotation of the Earth in our exploration and visualize which areas are illuminated by the Sun and which areas are in the night.

Mercure
Inclination of the planet : 0.0352° | Inclination of the orbit : | Rotation period : 58,6458 jours | Revolution period : 87.969
Vénus
Inclination of the planet : 177.36° | Inclination of the orbit : 3.39471° | Rotation period : -243,023 jours | Revolution period : 224.667
Terre
Inclination of the planet : 23.4366907752° | Inclination of the orbit : | Rotation period : 23h 56min 4s | Revolution period : 365.256363
Mars
Inclination of the planet : 25.19° | Inclination of the orbit : 1.85° | Rotation period : 24,622962 h | Revolution period : 686.885
Jupiter
Inclination of the planet : 3.12° | Inclination of the orbit : 1.304° | Rotation period : 9h 55min 27,3s | Revolution period : 4332.01
Saturne
Inclination of the planet : 26.73° | Inclination of the orbit : 2.486° | Rotation period : 10h 33min | Revolution period : 10754
Uranus
Inclination of the planet : 97.8° | Inclination of the orbit : 0.77323° | Rotation period : -17,23992 h | Revolution period : 30698
Neptune
Inclination of the planet : 28.32° | Inclination of the orbit : 1.77° | Rotation period : 16h 6,6min | Revolution period : 60216.8

The other bodies of the solar system

The solar system does not consist only of planets. There are also other objects that revolve around the Sun. Among them, we find natural satellites, like the Moon, which accompany certain planets by orbiting around them.
We can also observe many asteroids, which are small rocky blocks; the majority of them are in a region called the asteroid belt, located between Mars and Jupiter.

Further still, beyond the planet Neptune, lies a distant and icy region called the Kuiper belt.
This area contains dwarf planets like Pluto, as well as countless small objects made of ice, rock or both. It's a bit like a second belt, but much larger and more distant than that of the asteroids.
These different zones show that the solar system is much larger and more complex than we imagines: from distant small icy bodies to enormous gaseous planets, everything revolves around the Sun.