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9 Metis facts for kids

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For the moon of Jupiter, see Metis (moon).
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9 Metis Astronomical symbol for 9 Metis
Discovery
Discovered by A. Graham
Discovery date April 25, 1848
Designations
1974 QU2
Main belt
Orbital characteristics
Epoch July 14, 2004 (JD 2453200.5)
Aphelion 400.548 Gm (2.678 AU)
Perihelion 313.556 Gm (2.096 AU)
357.052 Gm (2.387 AU)
Eccentricity 0.122
1346.815 d (3.69 a)
19.21 km/s
274.183°
Inclination 5.576°
68.982°
5.489°
Physical characteristics
Dimensions 235×195×140 km
Mass ~9×1018 kg
Mean density
~2.7 g/cm³
~0.070 m/s²
~0.11 km/s
0.2116 d (5.078 h)
Albedo 0.243 (geometric)
Temperature ~173 K
max: 282 K (+9° C)
Spectral type
S-type
8.1 to 11.83
6.28
0.23" to 0.071"

9 Metis is one of the largest asteroids in the main asteroid belt. It is mostly made of silicate rocks and metals like nickel and iron. Scientists think it might be the leftover core of a much bigger asteroid. This larger asteroid was likely destroyed long ago in a huge space crash.

Discovery and Naming

Moon and Asteroids 1 to 10
The first 10 asteroids compared to Earth's Moon. 9 Metis is the second from the right.

The asteroid Metis was discovered by Andrew Graham. He found it on April 25, 1848. This was the only asteroid he ever discovered. It is also the only asteroid found from observations made in Ireland.

Metis is named after a figure from ancient Greek myths. Metis was a Titaness (a powerful goddess from an older generation of gods) and an Oceanid (a sea nymph). She was the daughter of Tethys and Oceanus. The name Thetis was also thought of for the asteroid but was not chosen. Another asteroid, 17 Thetis, later received that name.

What Metis is Like

We don't know which way Metis is spinning right now.

Pictures from the Hubble Space Telescope and studies of how its brightness changes show that Metis is not perfectly round. It has a stretched shape, with one end being pointy and the other wider. Radar observations also suggest it has a flat area. This matches the shape scientists have figured out from its light changes.

Scientists believe the surface of Metis is made of about 30-40% metal-rich olivine (a common green mineral) and 60-70% nickel-iron metal.

At one point, data about Metis's light suggested it might have its own moon. However, later observations did not confirm this idea. Searches using the Hubble Space Telescope in 1993 also did not find any moons around Metis.

Star Blockages

Metis has passed in front of, or "occulted," stars at least five times. When an asteroid occults a star, it means the asteroid temporarily blocks the star's light from reaching Earth. This helps scientists learn more about the asteroid's size and shape.


Images for kids

See also

Kids robot.svg In Spanish: (9) Metis para niños

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