69 Hesperia
A three-dimensional model of 69 Hesperia based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | G. Schiaparelli |
| Discovery date | April 29, 1861 |
| Designations | |
| (69) Hesperia | |
| Pronunciation | /hɛˈspɪəriə/ |
Named after | Hesperia |
| Main belt | |
| Adjectives | Hesperian /hɛˈspɪəriən/ |
| Orbital characteristics | |
| Epoch (absent) | |
| Aphelion | 3.471 AU (519.3 Gm) |
| Perihelion | 2.489 AU (372.3 Gm) |
| 2.980 AU (445.8 Gm) | |
| Eccentricity | 0.165 |
| 1,879 days (5.14 a) | |
| Inclination | 8.59° |
| 184.99° | |
| 288.8° | |
| Physical characteristics | |
| Dimensions | 138 km (IRAS) 110 ± 15 km |
| Mass | (5.86±1.18)×1018 kg |
Mean density | 4.38±0.99 g/cm3 |
| 5.655 h | |
| 0.140 | |
| M | |
| 7.05 | |
69 Hesperia is a large, M-type main-belt asteroid. It was discovered by the Italian astronomer Giovanni Schiaparelli on April 29, 1861 from Milan, while he was searching for the recently discovered 63 Ausonia. It was his only asteroid discovery. Schiaparelli named it Hesperia in honour of Italy (the word is a Greek term for the peninsula). The asteroid is orbiting the Sun with a period of 5.14 years, a semimajor axis of 2.980 AU, and eccentricity of 0.165. The orbital plane is inclined by an angle of 8.59° to the plane of the ecliptic.
Hesperia was observed by Arecibo radar in February 2010. Radar observations combined with lightcurve-based shape models, lead to a diameter estimate of 110 ± 15 km (68 ± 9.3 mi). The radar albedo is consistent with a high-metal M-type asteroid. In the near infrared, a weak absorption feature near a wavelength of 0.9 μm can be attributed to orthopyroxenes on the surface. A meteorite analogue of the reflectance spectra from 69 Hesperia is the Hoba ataxite.