Ariel

MOONMoon of Uranus

ILLUSTRATION FROM DENSITY 1.54 G/CM³ · RADIUS 579 KM · SHADING, NOT THE PHASE

[

OVERVIEW

] MOON

Ariel is a moon of Uranus. It orbits Uranus at a mean distance of 190 929 . It has a mass of 2.09×10⁻⁴ and a mean radius of 578.9 . It was discovered in 1851.

WHAT IT IS
Moon of Uranus
HOW FAR
190 929

Its average distance from Uranus, not from Earth.

HOW BIG
578.9

Its mean radius: half the width across.

ONE ORBIT TAKES
2.52

One trip round Uranus.

[

THE MODEL

] CATALOGUED RADIUS
DRAG TO ORBIT

CALCULATED · NOT AN OBSERVATION · CATALOGUED RADIUS · DENSITY 1.54 G/CM³ · RADIUS 579 KM · LIT FROM WHERE THE SUN IS

Drawn from the catalogued radius and from the same properties the picture at the top of this page uses, at the distance a flight to it would stop. Drag it, or use the arrow keys, to look from another direction. The stars behind are the 498,631 this catalogue holds real distances for, at their real positions and drawn from where the camera actually is — so the constellations are wrong, and that is the point. This is the sky from there, not the sky from here.

[

OBSERVING

] FROM WHERE YOU ARE

What it takes to see Ariel for yourself. Everything in this part of the page is worked out for a real horizon, a real night and the equipment you say you have.

[

CATALOG DATA

] 24 FIELDS

The raw catalogue values, as the source published them, with the error bars where one was published — sorted by what each set of figures is about rather than by the order they happened to be stored in.

WHAT KIND OF THING IT IS

What the object is in itself, rather than how it happens to look from here.

Mean density
1.539 ±0.026

THE ORBIT

The shape of the path, where the object sits on it, and the instant those figures were true of. An orbit is a fit to observations and drifts away from the real one either side of its epoch.

Orbits
Uranus
Orbital period
2.520379
Eccentricity
Inclination
0
Longitude of ascending node
0
Argument of periapsis
9.6
Mean anomaly
193.5
Element epoch
2451545.0000
Elements referred to
the planet's equator
Reference plane pole (right ascension)
77.3
Reference plane pole (declination)
15.2
Apsidal precession period
28.901
Mean anomaly fitted to the ephemeris
193.56
Mean anomaly rate
142.802
Apsidal precession rate
0.0341035
Nodal precession rate
0
Agreement with the ephemeris
0.1

WHEN IT WAS FOUND

Who first saw it, from where, and by what method.

Discovered by
W. Lassell

OTHER NAMES AND NUMBERS

The identifiers other catalogues file this object under, for anyone joining this data to theirs.

Also known as
Ariel (moon), Uranus I
JPL satellite code
701
Wikidata item
Q3343
Wikipedia article
Ariel (moon)

WHERE THESE FIGURES CAME FROM

Which catalogue, paper or model each of the fields above was read from, where the source named one.

Ephemeris
URA182
[

ALSO KNOWN AS

] 1 DESIGNATIONS
  • Common name Ariel
[

CITE THIS PAGE

] DR1

This page is live and its numbers move when an upstream refreshes, so the citation names the release the rows belong to rather than the day you read them. The release itself is frozen, republished as a bundle, and is what a data-availability statement should point at.

PLAIN TEXT
SpaceCatalog. Ariel [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/ariel
BIBTEX
@misc{spacecatalog_ariel,
  author       = {{SpaceCatalog}},
  title        = {{Ariel}},
  howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
  year         = {2026},
  url          = {https://spacecatalog.org/object/ariel},
  note         = {Catalogue entry, data release DR1 (2026-08-21). Values from JPL Planetary Satellite Data.}
}

The values above were taken from JPL Planetary Satellite Data — No licence stated; citation requested. Citing this page does not replace citing that catalogue.

That catalogue asks for this acknowledgement: Solar System Dynamics. (Downloaded 2026, September 13). Planetary Satellite Mean Elements; Planetary Satellite Physical Parameters; Planetary Satellite Discovery Circumstances. https://ssd.jpl.nasa.gov

[

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