243 Ida

From Wikipedia, the free encyclopedia
Jump to: navigation, search
243 Ida
243 ida
Galileo image of 243 Ida. The tiny dot to the right is its moon, Dactyl.
Discovery[1] and designation
Discovered by Johann Palisa
Discovery time September 29, 1884
Names
Other names A910 CD; 1988 DB1
Group Main belt (Koronis)
Orbit
Reference date October 22, 2004 (JD 2453300.5)
Longest distance from the Sun 447.843 Gm (2.994 AU)
Shortest distance from the Sun 408.207 Gm (2.729 AU)
Longest distance from the center of its orbital path
("semi-major axis")
428.025 Gm (2.861 AU)
How egg-shaped its orbit is
("eccentricity")
0.046
How long it takes to complete an orbit 1767.724 d (4.84 a)
Average speed 17.60 km/s
Mean anomaly 245.469°
Angle above the reference plane
("inclination")
1.138°
Longitude of where it comes up through the reference plane 324.218°
Angle between its shortest distance from what it orbits around and where it comes up through the reference plane
("argument of periapsis")
108.754°
Natural things which orbit around it Dactyl
Size and Other Qualities
Measures 53.6×24.0×15.2 km
Average distance from its center to its surface 15.7 km
Mass 4.2×1016 kg 1
Average density 2.6 g/cm³ 1
Gravity at its surface 0.0109 m/s²
Slowest speed able to escape into space
("escape velocity")
0.0185 km/s
How long it takes to turn around one time 0.1931 d (4 h 37 min) 2
How much light it reflects 0.2382 3
Surface temp. Min. Avg. Max.
Kelvin ~158 229
Celsius -45°
Light-band group
("spectral type")
S
True brightness
("absolute magnitude")
9.94

243 Ida is a Main belt asteroid with pictures taken by the Galileo spacecraft on August 28, 1993. It was the first binary asteroid to be found and is a member of the Koronis family of asteroids.

Discovery and name[change | edit source]

Ida was found by Johann Palisa on September 29, 1884 in Vienna. It is named after Ida, a Cretan nymph in Greek mythology who lived on a mountain that has her name (see Mount Ida, Crete).

Moon[change | edit source]

Ida has a small moon, Dactyl, which was found on February 17, 1994 by Galileo mission member Ann Harch, while examining the delayed image downloads. The moon was given the designation S/1993 (243) 1 and later named (243) Ida I Dactyl. The pictures where it was first seen were taken on 28 August 1993, hence the designation. The moon was reported on 12 March 1994.

Dactyl is only 1.4 km in diameter. Some researchers believe that Dactyl formed from debris blown off from Ida because of cratering, while others suggest that Ida and Dactyl formed as a pair a billion or more years ago when Ida's parent body was disrupted. Both of these theories present difficulties that are unresolved at this time. Since Dactyl was found, other sightings have suggested that asteroid moons are common.

Although Ida's dimensions, measured along the principal axes (based on its rotation) are 53.6×24.0×15.2 km, the best-fit ellipsoid measures 60.0×25.2×18.6 km. Since its mass is well known thanks to its little moon, one can calculate that its surface gravity can be between 0.0031 and 0.0324 m/s². The rotation axis is within one degree of the shorter dimension axis, which means the centrifugal effect can reach a value as high as 0.0042 m/s² — at the tips of its longest axes, Ida is actually under tension.

Related pages[change | edit source]

References[change | edit source]