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Metis
Metis

Jupiter XVI - 1979J3

Metis [MEE-tis] is the innermost known satellite of Jupiter. It was named after a Titaness who was a consort of Zeus (Jupiter). Metis and Adrastea lie within Jupiter's main ring and may be the source of material for the ring. Very little is known about Metis.

Metis Statistics
Discovered byStephen Synnott
Date of discovery1979
Mass (kg)9.56e+16
Mass (Earth = 1)1.5997e-08
Equatorial radius (km)20
Equatorial radius (Earth = 1)3.1358e-03
Mean density (gm/cm^3)2.8
Mean distance from Jupiter (km)127,969
Rotational period (days)?
Orbital period (days)0.294779
Mean orbital velocity (km/sec)31.57
Orbital eccentricity0.0000
Orbital inclination (degrees)0.0000
Escape velocity (km/sec)0.0253
Visual geometric albedo0.05
Magnitude (Vo)17.5

Metis Galileo Image of Metis
This image of Metis was taken by Galileo's solid state imaging system between November 1996 and June 1997. Although Metis was discovered by Voyager, it was no more than a point of light on images. This Galileo image is the the first image of the small moon that shows its irregular shape. Metis orbits Jupiter in the zone between the planet's ring and the larger Galilean satellites. The longest dimension of Metis is approximately 60 kilometers (37 miles) across. (Courtesy of NASA/Cornell University)

Metis Metis
This image of Metis was taken by the Voyager 1 spacecraft on March 4, 1979. Metis is the small dark dot above the arrow. (Copyright Calvin J. Hamilton)

Metis Best images yet of Thebe, Amalthea and Metis
These images of the inner Jovian moons Thebe, Amalthea, and Metis (left to right) are the highest-resolution images ever obtained of these small, irregularly shaped satellites. The images resolve surface features as small as 2 kilometers (about 1.2 miles) across for Thebe; 2.4 kilometers (about 1.5 miles) across for Amalthea, and 3 kilometers (about 1.9 miles) across for Metis.

The moons are shown in their correct relative sizes, with sunlight coming from the right. We are viewing the side of each moon that faces permanently away from Jupiter, and north is approximately up in all cases. (Courtesy NASA/Cornell University)

Metis Jupiter Small Satellite Montage
This image is A montage of images of the small inner moons of Jupiter from the camera onboard NASA's Galileo spacecraft shows the best views obtained of these moons. The top two images show the moon Thebe. Thebe rotates by approximately 50 degrees between the time these two images were taken, so that the same prominent impact crater is seen in both views; this crater, which has been given the provisional name Zethus, is near the point on Thebe that faces permanently away from Jupiter.

The next two images show the moon Amalthea; they were taken with the Sun directly behind the observer, an alignment that emphasizes patterns of intrinsically bright or dark surface material. The third image from the top is a view of Amalthea's leading side, the side of the moon that 'leads' as Amalthea moves in its orbit around Jupiter. This image looks 'noisy' because it was obtained serendipitously during an observation of the Jovian satellite Io. The fourth image from the top emphasizes prominent 'spots' of relatively bright material that are located near the point on Amalthea that faces permanently away from Jupiter. The bottom image is a view of the tiny moon Metis. (Courtesy NASA/Cornell University)

Metis Family Portrait of the Small Inner Satellites of Jupiter
These images, taken by Galileo's solid state imaging system between November 1996 and June 1997, provide the first ever "family portrait" of the four small, irregularly shaped moons that orbit Jupiter in the zone between the planet's ring and the larger Galilean satellites. The moons are shown in their correct relative sizes, with north approximately up in all cases. From left to right, arranged in order of increasing distance from Jupiter, are Metis (longest dimension is approximately 60 kilometers or 37 miles across), Adrastea (20 kilometers or 12 miles across), Amalthea (247 kilometers or 154 miles across), and Thebe (116 kilometers or 72 miles across). While Amalthea, the largest of these four tiny moons, was imaged by NASA's two Voyager spacecraft in 1979 with a resolution comparable to what is shown here, the new Galileo observations represent the first time that Metis, Adrastea, and Thebe have been seen as more than points of light. (Courtesy of NASA/Cornell University)

Synnott, S. P. "1979J3: Discovery of a Previously Unknown Satellite of Jupiter." Science, Vol 212, 19 June 1981.

Synnott, S. P. "Orbits of the Small Inner Satellites of Jupiter." Icarus 58, 1984.

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