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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
Loved and debated in equal measure. Reclassified from planet to dwarf planet by the IAU in 2006, Pluto is a complex, geologically active world with a nitrogen-ice heart — Tombaugh Regio — visible in the stunning New Horizons flyby images of 2015.
More massive than Pluto and the trigger for the 2006 IAU planet debate, Eris orbits in the scattered disc on a highly elliptical path taking 559 years to complete one revolution.
The only dwarf planet in the inner Solar System, residing in the main asteroid belt between Mars and Jupiter. Visited by the Dawn spacecraft, which found mysterious bright spots of sodium carbonate in its craters.
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.
A region of rocky and metallic bodies — the largest of which is Ceres — occupying the gap between the rocky inner planets and the gas giants. Far less dense than Hollywood would have you believe.
A vast disc of icy bodies beyond Neptune — the home of Pluto, Eris, Makemake, and Haumea, and the source of short-period comets. The New Horizons probe is currently travelling through this region.
A theorised spherical shell of icy bodies surrounding the Solar System at enormous distance — the source of long-period comets. Its outer edge, about 1–2 light-years away, marks the true gravitational boundary of our solar neighbourhood.
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.