Proteus (moon)

Proteus (Template:IPAc-en Template:Respell), also known as Neptune VIII, is the second-largest moon of Neptune and the planet's largest inner satellite. Discovered by Voyager 2 in 1989, it is named after Proteus, the shape-shifting sea god in Greek mythology. Proteus is about Template:Convert in diameter and orbits Neptune in a nearly equatorial orbit at a distance of about 4.75 Neptune radii from the planet's center.

Proteus has a highly irregular shape that differs significantly from an ellipsoid. It resembles an irregular polyhedron with several slightly concave facets and surface relief of up to Template:Convert. Its surface is dark, nearly neutral in color, and heavily cratered. The largest crater, Pharos, is more than Template:Convert across. The surface also contains numerous cliffs, grooves, and valleys associated with large impact craters.

Proteus is unlikely to have formed alongside Neptune. Instead, it probably accreted from debris produced after the capture of Neptune's largest moon, Triton.

Discovery and naming

Voyager 2, the space probe that discovered Proteus

Proteus was discovered in images taken by the Voyager 2 spacecraft during its approach to Neptune in 1989, about two months before its closest flyby. Its discovery came 40 years after that of Neptune's moon Nereid in 1949.

Following its discovery, the moon received the provisional designation S/1989 N 1. Stephen P. Synnott and Bradford A. Smith announced the discovery on July 7, 1989, describing it as being identified in "17 frames taken over 21 days", indicating a discovery date sometime before June 16.

On September 16, 1991, S/1989 N 1 was officially named Proteus after the shape-shifting sea god of Greek mythology, following the convention of naming Neptune's moons after sea deities and mythological sea creatures.

Orbit

Template:Annotated image Proteus orbits Neptune at an average distance of approximately Template:Convert, or about 4.75 times Neptune's equatorial radius. It completes one orbit every 1.1 days. Its orbit is nearly circular, with an eccentricity of Template:Val, and is inclined by about 0.5 degrees to Neptune's equator. Proteus is tidally locked to Neptune, rotating once per orbit so that the same hemisphere always faces the planet.

Proteus may once have been in a 1:2 orbital resonance with Larissa, completing one orbit for every two made by Larissa. As Proteus gradually migrated outward because of tidal interactions with Neptune, this resonance was broken, likely several hundred million years ago.

Physical characteristics

Proteus compared to 1 Ceres and the Moon

Proteus is the second-largest moon of Neptune and the largest of its regular prograde satellites. It is about Template:Convert in diameter, making it larger than Nereid, Neptune's third-largest moon. Because it orbits so close to Neptune, Proteus remained undiscovered by Earth-based telescopes, as it is obscured by the planet's bright reflected light.

Composition

False-color Voyager 2 image of Proteus, with its large crater Pharos located at the right

Proteus has a dark surface with a geometric albedo of about 10 percent, meaning it reflects only about one-tenth of the sunlight that reaches it. Its surface is nearly neutral in color, with little change in reflectivity across visible wavelengths. In the near-infrared, at wavelengths around 2 μm, its reflectivity decreases, suggesting the presence of complex organic compounds such as hydrocarbons or cyanides. These materials may contribute to the low albedo of Neptune's inner moons. Measurements at wavelengths of 1.4, 2.1, 3.0, and 4.6 μm show that Proteus has infrared reflectance properties similar to those of other dark small bodies in the Solar System, including Template:Mpl-.

Spectroscopic observations indicate that Proteus's surface contains hydrated minerals, possibly including ammonia-bearing materials, as well as weak carbon dioxide absorption that is slightly stronger on the trailing hemisphere. These findings suggest that Proteus is primarily a rocky body. Unlike Larissa, Galatea, and Neptune's rings, Proteus appears to be relatively poor in phyllosilicates. This may indicate that impacts have dehydrated phyllosilicate minerals on its surface or that Proteus formed from material different from that of Larissa and Galatea.

Shape

Proteus is approximately spherical, with a mean radius of about Template:Convert, although its shape deviates from a true sphere by as much as Template:Convert. It is thought to be close to the maximum size a body of its density can attain without its gravity pulling it into hydrostatic equilibrium. Proteus is slightly elongated toward Neptune, but its overall shape more closely resembles an irregular polyhedron than a triaxial ellipsoid. Its surface includes several flat or slightly concave facets measuring Template:Convert across, which are thought to be degraded impact craters. Template:Clear

Surface features

Voyager 2 image of Proteus, digitally processed showing surface features

Proteus is heavily cratered and shows no evidence of significant geological resurfacing. Its largest crater, Pharos, is Template:Nowrap in diameter and about Template:Convert deep. The crater contains a central dome several kilometers high. Pharos is the only named surface feature on Proteus. It is named after the Lighthouse of Alexandria, which is associated with Proteus in Greek mythology. In addition to Pharos, the moon has several craters Template:Convert across and many smaller craters less than Template:Convert in diameter.

Proteus also has linear features, including cliffs, valleys, and grooves. The most prominent of these lies west of Pharos and runs roughly parallel to the equator. These features may have formed during the impacts that created Pharos and the other large craters or as a result of tidal stresses exerted by Neptune.

Named features

Craters on Proteus are named after water-related spirits, gods, and goddesses, excluding figures from Greek and Roman mythology. As of May 2024, only one crater on Proteus, Pharos, has been named.

Crater	Pronunciation	Diameter	Approval Year	Eponym	Ref
Pharos	Template:IPAc-en Template:Respell	255 ± 12 km	1994	Lighthouse of Alexandria (Pharos), island where Proteus reigned	Template:WGPSN

Origin

Proteus, like Neptune's other inner moons, is unlikely to have formed alongside the planet. Instead, it probably accreted from debris produced after the capture of Triton. Following its capture, Triton is thought to have occupied a highly eccentric orbit that gravitationally disrupted Neptune's original inner satellites, causing them to collide and break apart into a debris disk. After Triton's orbit became nearly circular, some of this debris re-accreted to form Neptune's present-day inner moons.

Proteus may originally have orbited about Template:Convert closer to Neptune than it does today. Over time, tidal interactions caused the moon to migrate outward. During this migration, impacts may have created its largest craters and ejected fragments into orbit around Neptune. One such impact has been proposed as the origin of Neptune's small moon Hippocamp, which orbits close to Proteus.

External links

• Proteus In Depth at NASA's Solar System Exploration site
• Proteus page at The Nine Planets
• Proteus, A Moon Of Neptune on Views of the Solar System
• Ted Stryk's Proteus Page
• Neptune's Known Satellites (by Scott S. Sheppard)