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9 Metis
Discovery A |
Discoverer |
A. Graham |
Discovery date |
April 25, 1848 |
Alternate
designations |
1974 QU2 B |
Category |
Main belt |
Orbital elements C D |
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 km1 |
Mass |
4.6—1018 kg
(estimation) |
Density |
2 g/cm³
(estimation) |
Surface gravity |
0.036 m/s²
(estimation) |
Escape velocity |
0.081 km/s
(estimation) |
Rotation period |
0.2116 d 2 |
Spectral class |
S-type 3 |
Absolute magnitude |
6.28 |
Albedo |
0.160 3 |
Mean surface
temperature |
~177 K |
9 Metis (mee'-tis) is one of the largest Main belt asteroids. It is composed of silicates and metallic nickel-iron.
Size comparison: the first 10 asteroids profiled against Earth's Moon. From left to right, 1 Ceres, 2 Pallas, 3 Juno, 4 Vesta, 5 Astraea, 6 Hebe, 7 Iris, 8 Flora, 9 Metis, and 10 Hygiea. [Source]
Metis was discovered by Andrew Graham on April 25, 1848; his only asteroid discovery. It is also the only asteroid to have been discovered as a result of observations 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. [1] [2] 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. [3]
Metis has been observed occulting a star no less than 5 times.
Metis is also the name of a satellite of Jupiter.
Aspects
Stationary, retrograd |
Opposition |
distance to earth (AU) |
maximum brightness |
Stationary, prograde |
conjunction to sun |
January 19, 2006 |
March 3, 2006 |
1.35200 |
9.1 mag |
April 20, 2006 |
June 7, 2005 |
May 4, 2007 |
June 23, 2007 |
1.64582 |
9.7 mag |
August 13, 2007 |
November 5, 2006 |
September 24, 2008 |
November 5, 2008 |
1.13923 |
8.4 mag |
December 19, 2008 |
February 15, 2008 |
February 23, 2010 |
April 11, 2010 |
1.53609 |
9.5 mag |
June 3, 2010 |
August 7, 2009 |
June 11, 2011 |
July 28, 2011 |
1.53974 |
9.6 mag |
September 16, 2011 |
December 6, 2010 |
November 23, 2012 |
January 2, 2013 |
1.13905 |
8.5 mag |
February 12, 2013 |
March 30, 2012 |
March 26, 2014 |
May 15, 2014 |
1.64402 |
9.6 mag |
July 7, 2014 |
September 23, 2013 |
July 25, 2015 |
September 6, 2015 |
1.35478 |
9.2 mag |
October 25, 2015 |
January 5, 2015 |
January 11, 2017 |
February 22, 2017 |
1.31456 |
9.0 mag |
April 10, 2017 |
May 27, 2016 |
April 28, 2018 |
June 17, 2018 |
1.65468 |
9.7 mag |
August 7, 2018 |
October 30, 2017 |
September 14, 2019 |
October 27, 2019 |
1.16286 |
8.6 mag |
December 10, 2019 |
February 8, 2019 |
Links
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For other objects and regions, see: Binary asteroids, Asteroid moons and the Solar system
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