Cressida

Cressida

Moon· orbits Uranus

Cressida — moon of Uranus.

Open in 3D viewSee Cressida in the live, interactive 3D map

Key facts

Mass
1.84 × 10¹⁷ kg
0.0000025 Moon masses
Radius
39.8 km
2% of our Moon's radius
Orbit around Uranus
11.1 hours
0.46 Earth days

Science

Physical

Mass
1.84 × 10¹⁷ kg · 0.0000025 Moon masses
French et al. 2024, Icarus 411, 115957 — weighed from the amplitude of the 3:2 wave it raises in the η ring (±12%, 1σ); with the HST size this implies a density of 0.70 (+0.44/−0.21) g/cm³ View source ↗
Radius (estimated)
39.8 km · 2% of our Moon's radius
Sized from brightness and an assumed reflectivity, not a resolved disk. JPL Horizons still lists 33 km; this is Karkoschka's later HST value, and the size French et al. (2024) pair with the ring-wave mass for a density of 0.70 (+0.44/−0.21) g/cm³ — the same mass against the older size would imply 1.2 g/cm³.

Orbit around Uranus

Distance from Uranus
61,770 km
From JPL orbital elements
Orbital period
11.15 hours
From JPL orbital elements
Eccentricity
0.004
From JPL orbital elements
Inclination to Uranus's Laplace plane
1.80 °
From JPL orbital elements · The Laplace plane is the one a moon's orbit precesses about: close in it is the planet's equatorial plane, the plane of the rings, and further out it tilts toward the planet's own orbit.

Radiation & temperature

Insolation
0.00265 S⊕ · 1/378 of the sunlight Earth receives
Computed from the distance to the Sun (inverse-square; Earth's sunlight = 1), before any atmosphere.

Discovery & history

By
Voyager Science Team

Cressida was discovered in 1986 by Voyager Science Team. Uranus's moons are named after characters from the plays of Shakespeare and the poetry of Alexander Pope. Beyond its discovery and naming, little more about it has been individually recorded.

Images

Images from open archives · credit shown per image