Nine Worlds, One Star, No Two Alike

A field guide to the solar system, built in three dimensions

Rotate a planet. Read what makes it strange. Come back when you're curious about a different one.

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1
Star
8
Planets
5
Dwarf Planets
1
Moon, So Far

00The Star

1 OBJECT
The Sun
Yellow Dwarf Star

The Sun is a G2V yellow dwarf star holding 99.8% of the solar system's total mass. Its core fuses roughly 600 million tons of hydrogen into helium every second, and the resulting light takes about 8 minutes and 20 seconds to reach Earth.

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01The Inner and Outer Planets

9 OBJECTS
Mercury
Terrestrial Planet

Mercury is the smallest and innermost planet in the solar system, a cratered, airless world that swings from 430°C in direct daylight to -180°C at night. Despite being closest to the Sun, it is not the hottest planet — that title belongs to Venus.

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Venus
Terrestrial Planet

Venus is a runaway-greenhouse world wrapped in thick sulfuric acid clouds. Surface pressure is equivalent to being 900 meters underwater on Earth, and the surface itself is hot enough to melt lead — hotter than Mercury despite being farther from the Sun.

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Earth
Terrestrial Planet

Earth is the only known world with liquid water oceans on its surface, a breathable oxygen-nitrogen atmosphere, and life. Its magnetic field, generated by a molten iron core, shields the surface from most solar and cosmic radiation.

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The Moon
Natural Satellite

The Moon formed roughly 4.5 billion years ago from debris after a Mars-sized body, sometimes called Theia, struck early Earth. It is gravitationally locked, always showing the same face to Earth, and drifts about 3.8 centimeters farther away each year.

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Mars
Terrestrial Planet

Mars is a cold, iron-oxide desert world home to Olympus Mons, the largest volcano in the solar system at nearly three times the height of Mount Everest, and dry riverbeds suggesting liquid water once flowed across its surface.

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Jupiter
Gas Giant

Jupiter is the largest planet in the solar system, a gas giant more massive than all other planets combined. Its Great Red Spot is a storm wider than Earth that has been raging for at least 190 years, possibly for centuries longer.

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Saturn
Gas Giant

Saturn is best known for its dramatic ring system, made almost entirely of ice particles ranging from dust-sized grains to house-sized chunks, held in place by a handful of small shepherd moons.

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Uranus
Ice Giant

Uranus is tipped over almost completely on its side, likely from an ancient collision, so it essentially rolls around the Sun rather than spinning upright like the other planets. It is classified as an ice giant, built from water, ammonia, and methane ice.

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Neptune
Ice Giant

Neptune is the windiest place known in the solar system, with supersonic gusts exceeding 2,000 km/h tearing across an atmosphere fourteen times Earth's mass. It is the outermost recognized planet, orbiting the Sun once every 165 years.

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02Recognized Dwarf Planets

5 OBJECTS
Ceres
Dwarf Planet

Ceres is the largest object in the asteroid belt and the closest dwarf planet to the Sun. It contains substantial water ice beneath its surface and features mysterious bright spots inside its craters, later identified as salt deposits.

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Haumea
Dwarf Planet

Haumea spins so fast, once every four hours, that it has been stretched into an elongated oval shape like a rugby ball. It orbits beyond Neptune and even has its own faint ring system and two known moons.

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Makemake
Dwarf Planet

Makemake is named after a Rapa Nui creation deity and is a reddish, frozen world coated in methane and ethane ice, orbiting in the Kuiper Belt far beyond Neptune.

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Eris
Dwarf Planet

Eris is one of the most massive known dwarf planets, covered in highly reflective frozen methane. Its discovery in 2005 directly triggered Pluto's reclassification, since Eris is nearly as large and forced astronomers to define 'planet' more precisely.

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Pluto
Dwarf Planet

Pluto was the ninth planet from 1930 until 2006, when the discovery of the similarly sized Eris led the IAU to formally define 'planet' and reclassify Pluto as a dwarf planet. It has a large, heart-shaped nitrogen-ice plain called Sputnik Planitia and five known moons.

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Why the planets don't look alike

The short version: heat and leftovers. When the solar system formed about 4.6 billion years ago, the young Sun burned off the lighter gases from anything orbiting close by. What survived near the center were dense, rocky worlds — Mercury, Venus, Earth, and Mars — built from the heavier material that could withstand the heat.

Farther out, the Sun's heat couldn't reach as effectively, so Jupiter and Saturn held onto enormous envelopes of hydrogen and helium, becoming gas giants. Uranus and Neptune, colder still, are built more from water, ammonia, and methane ice — which is why they're often called ice giants instead, even though they're mostly fluid beneath the clouds.

The dwarf planets — Ceres, Pluto, Haumea, Makemake, and Eris — didn't gather enough surrounding material to "clear their orbital neighborhood," which is the specific criterion that keeps them out of the eight-planet club, even though several are large enough to be round under their own gravity.

How the formation actually happened

A slowly rotating cloud of gas and dust — the solar nebula — began to collapse under its own gravity. Most of it fell inward and ignited into the Sun. What was left formed a flattened disk, and inside that disk, dust grains collided and stuck together, building up from pebbles to boulders to planet-sized bodies over a few hundred million years.

That process wasn't gentle. Early Earth is thought to have been struck by a Mars-sized planet, with the debris from that impact eventually forming the Moon. The solar system you see in this catalog is really just what survived the collisions.

Questions people actually ask

How is this 3D viewer built?
It runs on WebGL through Three.js — no plugins, no download. Your browser renders the sphere, applies the texture, and handles the lighting directly on your device.
Where do the numbers on each planet page come from?
Radius, mass, distance, and rotation speed are drawn from public astronomical datasets maintained by NASA and the IAU — the same figures you'd find in a textbook, just rendered as telemetry instead of a table.
Is this free?
Yes, no account and no download. It's supported by the small ad units on the page, not a subscription.
Does it work on a phone?
Yes — the layout and the 3D viewer are both built to work with touch, on a screen of any size.