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99 Dike
Main-belt asteroid / From Wikipedia, the free encyclopedia
99 Dike (/ˈdaɪkiː/) is a quite large and dark main-belt asteroid. Dike was discovered by Alphonse Borrelly on May 28, 1868. It was his first asteroid discovery. This object is named after Dike, the Greek goddess of moral justice. Among the first hundred numbered minor planets, 99 Dike was considered anomalously faint for over a century. However, this was later found to be untrue.[8]
![]() Three-dimensional model of 99 Dike created based on light-curve. | |
Discovery[1] | |
---|---|
Discovered by | Alphonse Borrelly |
Discovery date | 28 May 1868 |
Designations | |
(99) Dike | |
Pronunciation | /ˈdaɪkiː/[2] |
Named after | Dike |
A915 BA; 1935 UC; 1935 YL; 1939 UT; 1948 UE; 1948 WC; 1961 XJ; 1974 VB | |
Main belt | |
Adjectives | Dikean /daɪˈkiːən/ |
Orbital characteristics[3][4] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 101.25 yr (36980 d) |
Aphelion | 3.18448 AU (476.391 Gm) |
Perihelion | 2.14561 AU (320.979 Gm) |
2.66504 AU (398.684 Gm) | |
Eccentricity | 0.19491 |
4.35 yr (1589.1 d) | |
Average orbital speed | 18.07 km/s |
18.1950° | |
0° 13m 35.551s / day | |
Inclination | 13.8487° |
41.5307° | |
195.413° | |
Earth MOID | 1.13747 AU (170.163 Gm) |
Jupiter MOID | 1.82393 AU (272.856 Gm) |
TJupiter | 3.316 |
Physical characteristics | |
Dimensions | 69.04±2.7 km |
Mass | ~3.9×1017 kg |
Mean density | 2.0? g/cm3 |
Equatorial surface gravity | ~0.0201 m/s2 |
Equatorial escape velocity | ~0.0380 km/s |
18.127 h (0.7553 d)[4][5] | |
0.0627±0.005[4] 0.058 [6] | |
Temperature | ~172 K |
C (Tholen) Xk (Bus)[7] | |
9.43 | |
This asteroid is orbiting the Sun with a period of 4.35 years and an eccentricity of 0.19. Its orbital plane is inclined by 13.8° to the plane of the ecliptic. The body spans a diameter of 69 km and it is classified as a C-type asteroid, which indicates it has a dark, carbonaceous surface. Based upon a light curve that was generated from photometric observations of this asteroid at Pulkovo Observatory, it has a rotation period of 18.127 ± 0.002 hours and varies in brightness by 0.22 ± 0.02 in magnitude.[5] However, according to Shrindan E. (2009) the rotation period is rather of 10.360 ± 0.001 h.[9]
The asteroid is located near the Juno clump of asteroids, but is most likely unrelated.[citation needed]