On Oct. 29, 1991, the Galileo spacecraft took a historic photograph of asteroid 951 Gaspra from a distance of 10,000 miles (16,000 kilometers) away. It was the first close-up photo ever taken of an asteroid in space.
Gaspra is an irregular, potato-shaped object about 12.5 miles (20 kilometers) by 7.5 miles (12 kilometers) by 7 miles (11.2 kilometers) in size. Its surface is covered with a layer of loose rubble and its terrain is covered with several dozen small craters.
Close-up photos of Asteroid 243 Ida taken by the Galileo spacecraft on Aug. 28, 1993, revealed that Ida had a tiny egg-shaped moon measuring 0.9 miles by 0.7 miles (1.44 by 1.12 kilometers). The moon has been named Dactyl.
NASA's Near-Earth Asteroid Rendezvous spacecraft was launched on Feb. 17, 1996. (Near-Earth asteroids come within 121 million miles [195 million kilometers] of the Sun. Their orbits come close enough that one could eventually hit Earth.) It flew within 750 miles (1,200 kilometers) of minor planet 253 Mathilde on June 27, 1997, and took spectacular images of the dark, crater-battered world. The asteroid's mean diameter was found to be 33 miles (52.8 kilometers). The NEAR spacecraft discovered that the carbon-rich Mathilde is one of the darkest objects in the solar system, only reflecting about 3% of the Sun's light, making it twice as dark as a chunk of charcoal. The asteroid is almost completely cratered, and at least five of its craters just on the lighted side are larger than 12 miles (19.2 kilometers).
The spacecraft reached asteroid 433 Eros in Dec. 1998, but aborted its mission due to engine problems. NEAR measured Eros to be 21 miles (33.6 kilometers) long by 8 miles (12.8 kilometers) wide and 8 miles (12.8 kilometers) deep. It rotates once every 5.27 hours and has no visible moons.
The spacecraft was renamed NEAR Shoemaker in honor of geologist Dr. Eugene M. Shoemaker (1928–1997), who influenced research on asteroids and comets in shaping the planets. It made a successful rendezvous with Eros on Feb. 14, 2000, and began a year-long orbit of the asteroid. NEAR Shoemaker data showed that the asteroid's ancient surface is covered with craters, ridges, boulders, and other complex features.
The First Ten Minor Planets (Asteroids)
Name | Year of discovery | Mean distance from Sun (millions of miles) | Orbital period (years) | Diameter (miles) | Magnitude | |
---|---|---|---|---|---|---|
1. Ceres | 1801 | 257.0 | 4.60 | 485 | 7.4 | |
2. Pallas | 1802 | 257.4 | 4.61 | 304 | 8.0 | |
3. Juno | 1804 | 247.8 | 4.36 | 118 | 8.7 | |
4. Vesta | 1807 | 219.3 | 3.63 | 243 | 6.5 | |
5. Astraea | 1845 | 239.3 | 4.14 | 50 | 9.9 | |
6. Hebe | 1847 | 225.2 | 3.78 | 121 | 8.5 | |
7. Iris | 1847 | 221.4 | 3.68 | 121 | 8.4 | |
8. Flora | 1847 | 204.4 | 3.27 | 56 | 8.9 | |
9. Metis | 1848 | 221.7 | 3.69 | 78 | 8.9 | |
10. Hygeia | 1849 | 222.6 | 5.59 | 40(?) | 9.5 |
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