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Moons of Neptune

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Neptune is a giant planet in our solar system with 16 known moons.

Neptune inner moons size comparison
Neptune inner moons size comparison

These moons are divided into two distinct categories: regular and irregular satellites. Regular moons orbit close to the planet in circular paths. They stay near Neptune's equatorial plane. Irregular moons are found much farther away. These moons often have orbits that are tilted or highly stretched. Most of these moons follow a naming convention based on Greek mythology. Because Neptune is the god of the sea, the names belong to water deities and creatures. This includes children of Poseidon, such as Triton and Proteus.

Neptunemoonsdiagram
Neptunemoonsdiagram

The moons are grouped by how they move and where they stay. The seven regular moons are Naiad, Thalassa, Despina, Galatea, Larissa, Hippocamp, and Proteus. These moons orbit in a prograde direction. This means they move in the same direction that Neptune rotates. Some of these moons, like Naiad and Thalassa, orbit between the planet's rings. Galatea is a special moon that acts as a shepherd. Its gravity helps keep the narrow Adams ring in place. The irregular moons include Triton and eight other satellites. These include Nereid, Halimede, and the distant S/2021 N 1.

Triton is the most unique moon in the entire Neptune system. It is the largest moon and is an irregular satellite. Unlike the other moons, Triton has a retrograde orbit. This means it orbits in the opposite direction of Neptune's rotation. Its orbit is also inclined, or tilted, relative to the planet's equator. Scientists believe Triton was not formed near Neptune. Instead, they think Neptune's gravity captured it from elsewhere. This capture was likely a catastrophic event. It probably disrupted Neptune's original satellites. Those moons may have collided to form a disc of rubble. The seven regular moons were likely re-accreted from that rubble.

Triton orbit & Neptune
Triton orbit & Neptune

History shows how our knowledge of these moons has grown over time. William Lassell discovered Triton on October 10, 1846. This happened only 17 days after Neptune was discovered. In 1949, Gerard P. Kuiper found the moon Nereid. In 1981, a team of astronomers discovered Larissa. They were actually looking for rings around Neptune. They noticed a star's luminosity, or brightness, dipped for a few seconds. This dip indicated a moon was passing in front of the star. In 1989, the Voyager 2 spacecraft provided many new details. It rediscovered Larissa and found five inner moons, including Proteus and Naiad.

Larissa 1
Larissa 1

The physical properties of these moons vary greatly. The inner regular moons are dark objects. Their geometric albedo, which measures how much light they reflect, is only 7% to 10%. They are likely made of water ice mixed with dark organic compounds. Proteus is the largest regular moon, measuring about 400 km in diameter. It has a heavily cratered surface with a large crater called Pharos. Triton is very different from the other moons. It is massive enough to achieve hydrostatic equilibrium, meaning it is shaped like a sphere. It even has a thin atmosphere made of nitrogen, methane, and carbon monoxide.

Proteus (Voyager 2)
Proteus (Voyager 2)

Some moons hold records for being extreme or unusual. Triton is one of the coldest bodies in the solar system. Its surface is covered in ices like nitrogen and carbon dioxide. It also has a very high albedo, reflecting much more light than the inner moons. Nereid is another unusual moon. It has a highly eccentric orbit, which is a very stretched-out path. S/2021 N 1 is also remarkable. It orbits farther from Neptune than any other known moon. It takes about 27 Earth years to complete just one orbit.

S-2021 N 1 GeminiNorth 2023-11-03 average stack annotated
S-2021 N 1 GeminiNorth 2023-11-03 average stack annotated

Studying Neptune's moons helps scientists understand how planetary systems work. The interaction between moons and rings, like Galatea and the Adams ring, shows how gravity organizes matter. The capture of Triton shows how large planets can grab objects from space. Even the smallest moons, like Hippocamp, provide clues about the history of the system. Hippocamp was found by analyzing old Hubble Space Telescope images. This discovery shows how new technology can find things that were missed before. Each moon is a piece of a larger puzzle about how our solar system formed and changed.

Irregular moon orbits a vs. i
Irregular moon orbits a vs. i
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🖼️ Images & Media (23)
File:New Webb Images Capture Rare View of Neptune’s Rings (Labeled).png
New Webb Images Capture Rare View of...
File:Orbits of inner moons of Neptune including S 2004 N 1.jpg
Orbits of inner moons of Neptune...
File:Neptune inner moons size comparison.svg
Neptune inner moons size comparison.svg
File:Triton orbit & Neptune.png
Triton orbit & Neptune.png
File:Irregular moon orbits a vs. i.jpg
Irregular moon orbits a vs. i.jpg
File:Neptunemoonsdiagram.png
Neptunemoonsdiagram.png
File:Naiad Voyager.png
Naiad Voyager.png
File:Neptune_Trio.jpg
Neptune_Trio.jpg
File:Despina.jpg
Despina.jpg
File:Galatea moon.jpg
Galatea moon.jpg
File:Larissa 1.jpg
Larissa 1.jpg
File:Hippocamp-heic1904b.jpg
Hippocamp-heic1904b.jpg

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