153 Hilda | |
Background: |
|
Minorplanet: | yes |
Mpc Name: | (153) Hilda |
Alt Names: | A875 VC; 1935 GD |
Adjective: | Hildian [1] |
Discovery Site: | Austrian Naval Obs. |
Discovered: | 2 November 1875 |
Mp Category: | Main belt (Hilda) |
Epoch: | 31 July 2016 (JD 2457600.5) |
Observation Arc: | 121.05 yr (44215 d) |
Uncertainty: | 0 |
Eccentricity: | 0.13971 |
Period: | 7.94 yr (2898.3 d) |
Inclination: | 7.8249° |
Asc Node: | 228.16° |
Arg Peri: | 38.617° |
Mean Anomaly: | 51.690° |
Mean Motion: | / day |
Jupiter Moid: | 0.569657AU |
Tisserand: | 3.023 |
Mass: | ~5.2 kg |
Escape Velocity: | ~ 6 m/s |
Abs Magnitude: | 7.48 |
Rotation: | 5.9587abbr=onNaNabbr=on |
Spectral Type: | P |
153 Hilda is a large asteroid in the outer main belt, with a diameter of 170 km. The spectrum matches that of a P-type asteroid. It was discovered by Johann Palisa on 2 November 1875, from the Austrian Naval Observatory at Pula, now Croatia. The name was chosen by the astronomer Theodor von Oppolzer, who named it after one of his daughters.[2] It is the largest member of the hilda family, a collisional family of asteroids in the Hilda region.
Hilda gives its name to an asteroid group called the Hilda group (or Hildas for short). It is not a true asteroid family, since the members are not physically related, but rather share similar orbital elements. The Hildas are locked in a 2:3 orbital resonance with Jupiter;[3] since Jupiter takes 11.9 years to orbit the Sun while Hilda takes 7.9 years, Jupiter orbits the Sun twice for every 3 orbits that Hilda completes. There are over 1,100 other objects known to be in a 2:3 resonance with Jupiter.[3] The asteroid is, however, the largest member of the ancient physically related Hilda family within the dynamical group of the same name.
The orbital plane of 153 Hilda is inclined at an angle of 7.82° to the plane of the ecliptic. It has an orbital eccentricity (ovalness) of 0.13971. Multiple light curves of the asteroid provide a consistent rotation period of approximately