Galileo image of 243 Ida. The tiny dot to the right is its moon, Dactyl.
|Discovery and designation|
|Discovered by||Johann Palisa|
|Discovery date||September 29, 1884|
|Alternative names||A910 CD; 1988 DB1|
|Minor planet category||Main belt (Koronis)|
|Epoch October 22, 2004 (JD 2453300.5)|
|Aphelion||447.843 Gm (2.994 AU)|
|Perihelion||408.207 Gm (2.729 AU)|
|Semi-major axis||428.025 Gm (2.861 AU)|
|Orbital period||1767.724 d (4.84 a)|
|Average orbital speed||17.60 km/s|
|Longitude of ascending node||324.218°|
|Argument of perihelion||108.754°|
|Mean radius||15.7 km|
|Mass||4.2×1016 kg 1|
|Mean density||2.6 g/cm³ 1|
|Equatorial surface gravity||0.0109 m/s²|
|Equatorial escape velocity||0.0185 km/s|
|Rotation period||0.1931 d (4 h 37 min) 2|
|Geometric albedo||0.2382 3|
|Absolute magnitude (H)||9.94|
Discovery and name[change | edit source]
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]
- P. C. Thomas, M. J. S. Belton, B. Carcich, C. R. Chapman, M. E. Davies, R. Sullivan, and J. Veverka; The shape of Ida, Icarus, Issue 1, No. 120, pp. 20–32, 1996.
- M. E. Davies, T. R. Colvin, M. J. S. Belton, P. C. Thomas, J. Veverka, The Galileo Imaging Science Team, The North Pole Direction and the Control Network of the Asteroid 243 Ida, Bulletin of the American Astronomical Society, Vol. 26, p. 1154, June 1994
- Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites, 2000
- The Asteroid Orbital Elements Database
- Minor Planet Discovery Circumstances
- IAUC 6082 announcing Dactyl's naming
|Wikimedia Commons has media related to: 243 Ida|