☀ Our Cosmic Neighbourhood

Our Solar System

One star, eight planets, hundreds of moons, and billions of smaller bodies — all bound together by gravity in a 4.6 billion year old family stretching billions of kilometres from the Sun to the edge of the Oort Cloud.

8 Planets
400+ Known Moons
4.6bn Years Old
1 Star (Sol)
🚀 Launch Interactive Explorer

Our Star

The Sun contains 99.86% of all mass in the Solar System. Everything else — every planet, moon, comet, and asteroid — orbits this single G-type yellow dwarf star.

Planets of the Solar System

From the scorched rock of Mercury to the frozen blue giant Neptune — each planet is a world unto itself, with its own geology, atmosphere, moons, and mysteries. Where a planet sits relative to Earth's orbit also changes how it looks in a telescope: it's why Venus and Mercury show phases but Mars doesn't.

Browse all planet guides for size comparisons, facts and 2026 viewing dates, including the Moon and Pluto.

Mercury

Terrestrial 0.39 AU
1st Planet · Innermost World

The smallest planet and the fastest, completing an orbit in just 88 days. With virtually no atmosphere, surface temperatures swing from −180°C at night to 430°C by day — the widest range of any planet.

Diameter 4,879 km
Orbital Period 88 days

Venus

Terrestrial 0.72 AU
2nd Planet · Earth's Twin

Almost identical to Earth in size, but a vision of hell beneath — the hottest planet in the Solar System at 465°C, with a crushing CO₂ atmosphere and sulphuric acid clouds. It rotates backwards, and slower than it orbits the Sun.

Diameter 12,104 km
Surface Temp 465°C (average)

Earth

Terrestrial 1.00 AU
3rd Planet · Our Home

The only known world to harbour life — a blue marble of liquid water, oxygen-rich atmosphere, and a magnetic field that shields its surface from the worst of the Sun's radiation. Uniquely placed in the habitable zone.

Diameter 12,742 km
Surface Water 71% of surface

The Moon

Earth's Satellite 384,000 km
Our Constant Companion

The most rewarding object in the entire night sky — craters, mountains and ancient lava seas visible through any binoculars, and a south pole both NASA and China are racing to reach. Every month's full moon carries its own traditional name.

Diameter 3,474 km
Age ~4.5 billion years

Mars

Terrestrial 1.52 AU
4th Planet · The Red Planet

A frozen desert world with the Solar System's largest volcano — Olympus Mons, three times the height of Everest — and a canyon system, Valles Marineris, wide enough to span the USA. Once had liquid water flowing on its surface.

Diameter 6,779 km
Day Length 24 hrs 37 min

Jupiter

Gas Giant 5.20 AU
5th Planet · Largest in the System

More than twice as massive as all other planets combined. The Great Red Spot — a storm wider than Earth — has raged for at least 350 years. Jupiter's four Galilean moons, including ocean-harbouring Europa, are worlds in their own right.

Diameter 139,820 km
Mass 318 × Earth

Saturn

Gas Giant 9.58 AU
6th Planet · Lord of the Rings

The jewel of the Solar System, wearing a ring system of ice and rock spanning 282,000 km. Saturn is so light it would float on water. Its moon Enceladus shoots geysers of liquid water into space, and Titan has a thick nitrogen atmosphere and liquid methane lakes.

Ring Span 282,000 km
Density 0.69 g/cm³

Uranus

Ice Giant 19.2 AU
7th Planet · Tilted World

The oddest planet in the Solar System — tilted 98° on its side, so it rolls along its orbit like a spinning top on its side. Its blue-green colour comes from methane ice, and it holds the record for the coldest planetary atmosphere at −224°C.

Axial Tilt 97.77°
Min Temp −224°C

Neptune

Ice Giant 30.1 AU
8th Planet · Outermost Giant

The most distant planet, never visible to the naked eye, and host to the fastest winds in the Solar System — reaching 2,100 km/h. Its largest moon Triton orbits backwards, almost certainly a captured Kuiper Belt Object, and is slowly spiralling inward to its doom.

Wind Speed 2,100 km/h
Orbital Period 164.8 years

Dwarf Planets

The IAU defines a dwarf planet as a body that orbits the Sun and has sufficient mass for a roughly spherical shape — but has not cleared the neighbourhood around its orbit. Hundreds may exist, mostly in the Kuiper Belt.

Regions & Small Body Populations

Beyond the planets, the Solar System is shaped by vast regions of rocky and icy debris — remnants of formation that still influence planetary orbits and deliver comets and meteors to the inner system today.

How the Solar System Formed

A brief primer on the origin and structure of our cosmic neighbourhood.

The Solar System formed approximately 4.6 billion years ago from the gravitational collapse of a giant molecular cloud — a vast region of gas and dust in the Milky Way. As the cloud collapsed, it spun faster and flattened into a protoplanetary disc around the young Sun. Over millions of years, dust grains collided and stuck together, growing into planetesimals and eventually into the planets we see today. The inner planets — rocky and dense — formed where it was too hot for volatile ices to survive. The outer planets — rich in hydrogen, helium, and ice — formed beyond the frost line, where those materials could condense.

The Solar System's structure is not entirely stable over billions of years. Planetary migrations early in its history — particularly Jupiter's inward and outward movement described by the Nice Model — dramatically reshaped the orbits of other planets and may have been responsible for the Late Heavy Bombardment, a period of intense cratering on the Moon and inner planets around 4 billion years ago. Today's configuration is relatively settled, but the gravitational dance between the outer planets continues to slowly influence the Solar System's long-term future.

What to use to explore the Solar System

Five planets are naked-eye objects. With binoculars or a small telescope, you can see Jupiter's moons, Saturn's rings, and Mars's polar caps. Here's where to start.

Best first telescope

Sky-Watcher Heritage 130P

4.6Full review

Shows Jupiter's cloud bands and four moons, Saturn's rings, the crescent of Venus, and Mars's polar caps at opposition. Compact enough to grab on a clear night without a lengthy setup.

~£194
Buy at FLO
Start with binoculars

Celestron SkyMaster Pro 15×70

4.5Full review

Jupiter's Galilean moons appear as tiny dots in a line. Venus shows a clear disc. Mars glows orange. All five naked-eye planets look distinctly different from stars — no twinkling. A great entry point before committing to a telescope.

~£229
Buy at FLO

Equipment guides

Telescopes, binoculars, mounts, cameras, and accessories — honest recommendations for every budget, from first purchase to serious upgrades.

Browse all →

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Frequently Asked Questions

How many planets are in the Solar System?
Eight: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. Pluto was counted as the ninth from its discovery in 1930 until 2006, when the International Astronomical Union moved it into the new dwarf planet category alongside Eris and Ceres. The Sun holds about 99.86% of all the mass in the system.
What is the Kuiper Belt?
The Kuiper Belt is a broad ring of icy bodies orbiting beyond Neptune, roughly 30 to 50 AU from the Sun. It holds several dwarf planets, Pluto among them, alongside more than 2,000 other known objects. It is also where most short-period comets come from.
What is the Oort Cloud?
The Oort Cloud is a shell of icy bodies thought to surround the whole Solar System, from about 2,000 AU out to perhaps 100,000 AU, which is close to a third of the way to the nearest star. Nobody has observed it directly, as it is far too distant and faint. It exists as the explanation for long-period comets, which arrive from every direction on orbits lasting thousands of years.
What is the smallest planet in the Solar System?
Mercury, at 4,879km across. It is smaller than Jupiter's moon Ganymede and Saturn's moon Titan, and it orbits the Sun once every 88 days. It took the title outright in 2006, when Pluto was reclassified as a dwarf planet.
How did the Solar System form?
It formed about 4.6 billion years ago, when a giant cloud of gas and dust collapsed under its own gravity. The cloud flattened into a spinning disc around the young Sun, and over millions of years dust grains stuck together and grew into planets. The inner planets came out rocky because it was too hot near the Sun for ices to survive, while beyond the frost line the outer planets grew large and gas-rich.

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