9 Metis
|
Discovery A (http://cfa-www.harvard.edu/iau/lists/NumberedMPs.html) | |
---|---|
Discoverer | Andrew Graham |
Discovery date | April 25, 1848 |
Alternate designations | 1974 QU2 B (http://cfa-www.harvard.edu/iau/MPDes.html) |
Category | Main belt |
Orbital elements C (http://asteroid.lowell.edu/) Epoch July 14, 2004 (JD 2453200.5) | |
Eccentricity (e) | 0.122 |
Semi-major axis (a) | 357.052 Gm (2.387 AU) |
Perihelion (q) | 313.556 Gm (2.096 AU) |
Aphelion (Q) | 400.548 Gm (2.678 AU) |
Orbital period (P) | 1346.815 d (3.69 a) |
Mean orbital speed | 19.28 km/s |
Inclination (i) | 5.576° |
Longitude of the ascending node (Ω) | 68.982° |
Argument of perihelion (ω) | 5.489° |
Mean anomaly (M) | 274.183° |
Physical characteristics | |
Dimensions | 235×165 km [1] (http://web.media.mit.edu/~win/hstpub.pdf) km |
Mass | 4.6×1018 kg |
Density | 2 ? g/cm³ |
Surface gravity | 0.036 m/s² |
Escape velocity | 0.081 km/s |
Rotation period | 0.2116 d 2 (http://www.psi.edu/pds/archive/lc.html) |
Spectral class | S-type asteroid 3 (http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT) |
Absolute magnitude | 6.28 |
Albedo | 0.160 3 (http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT) |
Mean surface temperature | ~185 K |
9 Metis (mee'-tis) is one of the largest Main belt asteroids. It is composed of silicates and metallic nickel-iron.
Metis was discovered by A. Graham on April 25, 1848; his only asteroid discovery. It is also the only asteroid to have been discovered from Ireland. Its name comes from the mythological Metis, a Titaness, daughter of Tethys and Oceanus (and thus an Oceanid), who was the first wife of Zeus and the mother of Athena. Zeus devoured her lest she bear a child more powerful than he.
Light curve data on Metis led to an assumption that it could have a satellite. However, subsequent observations failed to confirm this. [2] (http://www.bdl.fr/observateur/binast/binary_ast.php) [3] (http://www.johnstonsarchive.net/astro/asteroidmoonsq.html) Metis was later observed with the Hubble Space Telescope in 1993, which was able to resolve the irregular shape of the asteroid, but no satellites were detected. [4] (http://web.media.mit.edu/~win/hstpub.pdf)
Metis has been observed occulting a star no less than 5 times.
Metis is also the name of a satellite of Jupiter.
External links
- "Notice of discovery of Metis", MNRAS 8 (1848) 146 (http://adsabs.harvard.edu//full/seri/MNRAS/0008//0000146.000.html)
- Irish Astronomical History: Markree Castle Observatory and The Discovery of the Asteroid Metis (http://www.eaas.co.uk/news/metis.html)
The minor planets |
Vulcanoids | Main belt | Groups and families | Near-Earth objects | Jupiter Trojans |
Centaurs | Trans-Neptunians | Damocloids | Comets | Kuiper belt | Oort cloud |
(For other objects and regions, see: Binary asteroids, Asteroid moons and the Solar system) |
(For a complete listing, see: List of asteroids. For pronunciation, see: Pronunciation of asteroid names.) |