A Guide to Planetary Satellites

by the Editors of Sky & Telescope

Amalthea
Jupiter's inner moon Amalthea, discovered by E. E. Barnard in 1892 and seen at close range by NASA's Galileo spacecraft in 1999, is roughly 170 kilometers across.
Courtesy NASA/JPL.
Discovering a planetary satellite used to be a rare event. After the finding of Uranus's moon Miranda by Gerard Kuiper in 1948 and Jupiter's Ananke by Seth Nicholson in 1951, the total count of natural satellites stood at 31: Jupiter led with 12, followed by Saturn (9), Uranus (5), Neptune (2), Mars (2), and Earth (1). Telescopic observers added only a few more in the ensuing three decades — most notably Pluto's moon, Charon — as satellite discovery largely fell to NASA spacecraft. After Voyager 2's flyby of Neptune in 1989, the total had nearly doubled to 60.

However, the advent of sensitive electronic cameras has put telescopic observers back in the driver's seat, resulting in dozens of finds over the past few years. Indeed, some of the new objects are so small, only a few kilometers across, that they stretch the traditional notion of what constitutes a "moon." Sometimes faint objects appear fleetingly in images and are never seen again; others require patient follow-up observations over months or years to confirm their reality. While comets bear the surname(s) of their discoverer(s), and observers retain naming rights for asteroids, those who spot planetary moons must yield this privilege to the International Astronomical Union. By convention, the IAU does not name a satellite until its orbit is known precisely — a threshhold sometimes not reached until decades after the initial discovery.

The following is a tabulation of known planetary satellites, last updated in September 2007. As of then, the count stood at 166, distributed as follows: Earth 1, Mars 2, Jupiter 63, Saturn 60, Uranus 27, Neptune 13. The dwarf planets have 4: Pluto 3 and Eris 1.

In the table below and on the following pages, the Diameter of each satellite and the Orbital distance from its planet's center (semimajor axis) are in kilometers; Eccentricity (Ecc.) is the elongation of the satellite's orbit; and Inclination is the tilt of its orbit plane, in degrees, with respect to the planet's equatorial plane (for inner moons) or the ecliptic plane (for outer moons).

Confirmed List of Planetary Satellites
 
Satellite
Diameter
(km)
Visual
magnitude
Distance
(km)
Orbital
period (days)
 
Ecc.
Inc.
(degrees)
EARTH      
Moon3,475-12.7384,40027.30.0555.2
MARS      
Phobos2211.49,3800.30.0151.1
Deimos1212.523,4601.30.0001.8



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