260 Huberta
In today's world, 260 Huberta has become a topic of utmost importance and relevance in various spheres of life. Both on a personal and professional level, 260 Huberta has generated a great impact and has aroused great interest in the public. There are numerous studies, research and debates surrounding 260 Huberta, demonstrating its importance and the need to understand it in depth. In this article, we will explore different aspects related to 260 Huberta, analyzing its influence on current society and its possible evolution in the future. In addition, we will reflect on the possible implications and consequences of 260 Huberta in our daily lives, as well as in the development of various industries and sectors.
.png) A three-dimensional model of 260 Huberta based on its light curve. | |
| Discovery | |
|---|---|
| Discovered by | Johann Palisa |
| Discovery date | 3 October 1886 |
| Designations | |
| (260) Huberta | |
| Pronunciation | /hjuːˈbɜːrtə/ |
Named after | Hubertus |
| A886 TA, 1906 VH 1911 ME | |
| Main belt (Cybele) | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 109.37 yr (39947 d) |
| Aphelion | 3.84026 AU (574.495 Gm) |
| Perihelion | 3.04743 AU (455.889 Gm) |
| 3.44384 AU (515.191 Gm) | |
| Eccentricity | 0.11511 |
| 6.39 yr (2334.3 d) | |
Average orbital speed | 16.05 km/s |
| 110.638° | |
| 0° 9m 15.188s / day | |
| Inclination | 6.41599° |
| 165.393° | |
| 180.996° | |
| Physical characteristics | |
| Dimensions | 94.67±3.6 km |
| 8.29 h (0.345 d) | |
| 0.0509±0.004 | |
| CX | |
| 8.97 | |
260 Huberta is a large asteroid orbiting near the outer edge of the Main belt. It is dark and rich in carbon.
It belongs to the Cybele group of asteroids[2] and may have been trapped in a 4:7 orbital resonance with Jupiter.
It was discovered by Johann Palisa on 3 October 1886 in Vienna and was named after Saint Hubertus.
References
- ^ "260 Huberta". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
- ^ Lagerkvist, Claes-Ingvar; et al. (January 2001), "A Study of Cybele Asteroids. I. Spin Properties of Ten Asteroids", Icarus, 149 (1): 190–197, Bibcode:2001Icar..149..190L, doi:10.1006/icar.2000.6507.
- The Asteroid Orbital Elements Database
- Minor Planet Discovery Circumstances
- Asteroid Lightcurve Data File
External links
- 260 Huberta at AstDyS-2, Asteroids—Dynamic Site
- 260 Huberta at the JPL Small-Body Database
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