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Planet

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A planet is a large, rounded astronomical body that orbits a star, a stellar remnant, or a brown dwarf. To be classified as a planet, the object must not be a star itself. In our Solar System, the International Astronomical Union (IAU) recognizes eight planets. These are divided into the terrestrial planets and the giant planets.

Planet collage to scale
Planet collage to scale

Understanding planets helps us learn how solar systems form and where life might exist. It also helps us understand the difference between rocky worlds and massive gas giants.

Planets form through a process called accretion. This begins when an interstellar cloud of gas and dust collapses into a nebula. At the center, a young protostar forms. Surrounding this star is a rotating protoplanetary disk. Inside this disk, dust particles undergo sticky collisions to accumulate mass. These particles grow into local concentrations of mass called planetesimals.

Jupiter interior
Jupiter interior

As planetesimals grow, their gravitational attraction pulls in even more material. This accelerates the accretion process until they become dense protoplanets. Once a protoplanet reaches a mass larger than Mars, it begins to capture an extended atmosphere. This atmosphere increases the rate at which it pulls in more planetesimals through atmospheric drag.

There are several distinct types of planets in our Solar System. The terrestrial planets include Mercury, Venus, Earth, and Mars. These bodies are primarily composed of rock and metal. Earth is the largest of these terrestrial worlds. The giant planets are much more massive and fall into two groups. Jupiter and Saturn are gas giants, made mostly of hydrogen and helium.

Voyager 2 - Saturn Rings - 3085 7800 2
Voyager 2 - Saturn Rings - 3085 7800 2

Uranus and Neptune are known as ice giants. These are composed of low-boiling-point materials like water, methane, and ammonia. They also possess thick atmospheres of hydrogen and helium.

Our understanding of planets has changed significantly throughout history. The word "planet" comes from a Greek term. In antiquity, people used it to describe the Sun, the Moon, and five moving lights: Mercury, Venus, Mars, Jupiter, and Saturn. Many cultures associated these celestial bodies with their gods. For a long time, people believed in geocentrism, the idea that Earth was the center of the universe.

1660 illustration of Claudius Ptolemy's geocentric model of the Universe
1660 illustration of Claudius Ptolemy's geocentric model of the Universe

This changed during the 16th and 17th centuries with the rise of heliocentrism. The invention of the telescope later revealed many more objects, such as the moons of other planets and the ice giants.

In 2006, the IAU established a specific definition for planets. This decision was spurred by the discovery of large objects in the Kuiper belt, such as Eris. Under this definition, Ceres, Pluto, and Eris are classified as dwarf planets. Dwarf planets are gravitationally rounded but have not cleared their orbits of other bodies.

TheKuiperBelt Orbits Pluto Ecliptic
TheKuiperBelt Orbits Pluto Ecliptic

While the IAU uses a strict definition, many planetary scientists still use the term "planet" more broadly. They may include dwarf planets or large, rounded moons in their studies.

Specific measurements show the incredible variety of sizes in our system. Jupiter is the largest planet, with a mass of 318 Earth masses. In contrast, Mercury is the smallest at only 0.055 Earth masses. Saturn is a massive gas giant, but it is only one third as massive as Jupiter, at 95 Earth masses. The ice giants are much smaller, with Uranus and Neptune having masses of 14 and 17 Earth masses respectively.

Solar System true color (captions)
Solar System true color (captions)

These numbers highlight the massive scale differences between the different types of planets.

Beyond our Solar System, astronomers have discovered over 5,900 exoplanets. These are planets that orbit stars other than our Sun. Some exoplanets have very unusual features. For example, "hot Jupiters" are giant planets that orbit very close to their parent stars. Others, like HD 20782 b, have extremely eccentric orbits.

Exoplanet detections per year
Exoplanet detections per year

Scientists also look for planets in the "habitable zone." This is the region around a star where liquid water could potentially exist on a surface. While many exoplanets exist in these zones, Earth remains the only planet known to support life.

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🖼️ Images & Media (41)
File:Planet_collage_to_scale.jpg
Planet_collage_to_scale.jpg
File:Solar System true color (captions).jpg
Solar System true color (captions).jpg
File:Exoplanet detections per year.png
Exoplanet detections per year.png
File:TheKuiperBelt Orbits Pluto Ecliptic.svg
TheKuiperBelt Orbits Pluto Ecliptic.svg
File:AxialTiltObliquity.png
AxialTiltObliquity.png
File:Jupiter interior.png
Jupiter interior.png
File:Top of Atmosphere.jpg
Top of Atmosphere.jpg
File:Structure_of_the_magnetosphere_LanguageSwitch.svg
Structure_of_the_magnetosphere_LanguageSwitch.svg
File:Voyager 2 - Saturn Rings - 3085 7800 2.png
Voyager 2 - Saturn Rings - 3085 7800 2.png
File:Apparent retrograde motion of Mars in 2003.gif
Apparent retrograde motion of Mars in 2003.gif
File:1660 illustration of Claudius Ptolemy's geocentric model of the Universe.jpg
1660 illustration of Claudius Ptolemy's...
File:The_Solar_System,_with_the_orbits_of_5_remarkable_comets._LOC_2013593161.jpg
The_Solar_System,_with_the_orbits_of_5_rem...

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