Phoebe (moon) Overview Orbital Characteristics Physical

**Phoebe**

Discovery
Discovered by	W.H. Pickering
Discovered in	1898
Orbital characteristics
Semimajor axis	12,952,000 km
Eccentricity	0.163
Orbital period	550 day 11 h 31 min
Inclination	175.3 °
Is a satellite of	Saturn
Physical characteristics
Mean diameter	220 km
Mass	7.2×10¹⁸ kg
Mean density	2.3 g/cm³
Surface gravityThis article covers the physics of gravitation. See also gravity (disambiguation). Gravitation is the tendency of masses to move toward each other. The first mathematical formulation of the theory of gravitation was made by Sir Isaac Newton and proved ast	0.039 m/s²In physics, acceleration (symbol: a is defined as the rate of change (or time derivative) of velocity. It is thus a vector quantity with dimension length/ time². In SI units, this is metre/second². To accelerate an object is to change its velocity over a
Rotation periodprograde planet like the Earth, the sidereal day is shorter than the solar day. At time 1, the sun and a certain distant star are both overhead. At time 2, the planet has rotated 360° and the distant star is overhead again (1→2 one sidereal day).	9 h 30 min
Axial tiltAxial tilt is an astronomical term regarding the inclination angle of a planet's rotation axis in relation to its orbital plane. It is also called obliquity . A planet whose rotation axis were perpendicular to the orbital plane would have an axial tilt of	unknown
AlbedoNote: This article discusses the physical or planetological property of albedo. For other usage, see Albedo (disambiguation). The albedo is a measure of reflectivity of a surface or body. It is the ratio of electromagnetic radiation reflected to the amoun	0.06
Atmosphere	none

1 Overview

For more than 100 years, Phoebe was Saturn's outermost known moon, until the discovery of several smaller moons in 2000. Phoebe is almost 4 times more distant from Saturn than its nearest major neighbor ( Iapetus), and is substantially larger than any of the other moons orbiting planets at comparable distances.

2 Orbital characteristics

All of Saturn's moons up to Iapetus orbit very nearly in the plane of Saturn's equator. The outer moons can be broken down into two groups: Siarnaq's group ( Kiviuq, Ijiraq, Paaliaq, Albiorix, Erriapo, Siarnaq and Tarvos) is inclined 33.5-46.5° whilst Phoebe's group (Phoebe, Skathi, S/2003 S 1, Mundilfari, Suttungr, Thrymr and Ymir) is retrograde and inclined 134.5-175.5°. Both groups are fairly to highly eccentric, and none of their moons are expected to rotate synchronously as all the inner moons of Saturn do (except for Hyperion). The inclinations given are with respect to the solar system's ecliptic rather than Saturn's equator, as the local Laplace plane at these distances is already quite tilted with respect to Saturn's equator. This tilt reaches 15° at Iapetus' distance; at Phoebe's, it has already merged with the ecliptic (tilt of 26°).

3 Physical characteristics

Phoebe is roughly spherical and has a diameter of 220 kilometres (about 137 miles), which is equal to about one-fifteenth of the diameter of Earth's moon. Phoebe rotates on its axis every nine hours and it completes a full orbit around Saturn in about 18 months. Its surface temperature is only 75 K (-198°C).

Most of Saturn's inner moons have very bright surfaces, but Phoebe's albedo is very low (0.06), as dark as lamp black. The surface is extremely heavily scarred, with craters up to 80 kilometres across, one of which has walls 16 kilometres high.

Phoebe's dark colouring initially led to scientists surmising that it was a captured asteroid, as it resembled the common class of dark carbonaceous asteroids. These are chemically very primitive and are thought to be composed of original solids that condensed out of the solar nebula with little modification since then.

However, images from the Cassini-Huygens space probe indicate that Phoebe's craters show a considerable variation in brightness, which indicate the presence of large quantities of ice below a relatively thin blanket of dark surface deposits some 300 to 500 metres (980 to 1,600 feet) thick. In addition, quantities of carbon dioxide have been detected on the surface, a finding which has never been replicated on an asteroid. It is estimated that Phoebe is about 50% rock, as opposed to the 35% or so that typifies Saturn's inner moons. For these reasons, scientists are coming to believe that Phoebe is a captured Centaur, one of a number of icy planetoids from the Kuiper belt that orbit the Sun between Jupiter and Neptune. If this is the case, Phoebe is the first such object to be imaged as anything other than a dot.

Material displaced from Phoebe's surface by microscopic meteor impacts may be responsible for the dark surfaces of Hyperion and the leading hemisphere of Iapetus. The debris from the biggest impacts may also have been the building blocks of the other moons of Phoebe's group -all of which are less than 10 km in diameter.

4 Spacecraft flybys

The Voyager 2 spacecraft passed by Phoebe in September 1981, although the long distance (2.2 Gm) and low resolution meant that relatively little could be learned from the resulting images.

The Cassini spacecraft flew within 2,068 kilometers (about 1,285 miles) of Phoebe on June 11, 2004, returning many high-resolution images of the moon and its scarred surface.

5 See also

List of geological features on Saturn's smaller moons

6 External links

... | Ijiraq | Phoebe | Paaliaq | ...

Saturn
Janus' group \| Mimas \| Enceladus \| Tethys \| Dione \| Rhea
Titan \| Hyperion \| Iapetus \| Siarnaq's group \| Phoebe's group
(For other moons, see: Saturn's natural satellites)
see also: Cassini-Huygens

Saturn's moons

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