Puck

Updated

Details

Puck is the largest of Uranus' lesser inner moons, discovered in Voyager 2 images ahead of the spacecraft's 1986 Uranus flyby. It orbits Uranus in less than one Earth day, giving the planet's crowded inner moon region a compact anchor between the rings and Miranda.

Puck matters because it is the largest member of Uranus' small inner moon family, not one of the five classical major moons. Voyager 2 found it during the 1986 Uranus encounter, turning what had been a nearly invisible inner region into a known collection of small satellites.

NASA describes Puck as about 150 kilometers across and as the largest of Uranus' lesser satellites. That makes it a useful boundary object: large enough to stand apart from the smallest inner moons, but still far below Miranda and the other major Uranian moons. It orbits the planet in less than one Earth day, deep inside the larger moon system.

That is why Puck belongs on this scale. It shows that Uranus is not only a set of five named icy worlds; it also has a crowded inner system where small moons and narrow rings occupy the same architectural neighborhood. Puck gives that inner region a visible body to hold onto.

65.5km
Visual creditscaleofspace.org / CC BY-NC 4.0

Key facts

Category
Moons
Object class
Small inner moon
Host
Uranus
Scale fact
150 kmdiameter
Composition
Water ice and silicate rock

Scale context

Where Puck sits on the full axis

By size on the journey, Puck sits between Cygnus X-1 and Phoebe. The band below uses nearby Moons objects for context.

Shared physical scale
303km
Deimos12 km
Phobos22 km
Puck150 km
Phoebe213 km
Nereid340 km
Mimas396 km

Together, these objects make the size change around Puck easy to compare at a glance.

Sources

References for Puck

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Between the smallest and the largest, perspective is everything.

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