Asteroid 776 Berbericia Observation Details
Berbericia Daily Motion
776 Berbericia will be visible until July, 20, when it will move too close to the Sun. During this time, its proximity to the Sun will cause it to disappear from the night sky, making it unobservable for a while.
Berbericia Visibility Timetable on May 09
Berbericia Rise and Set Timetable
| Time | Elevation | |
| Berbericia rise | 14:31 | |
| Moon Rise, 87.4% illuminated | 17:00 | 26° |
| Sunset | 20:32 | 66° |
| Civil sunset | 21:04 | 71° |
| Berbericia transit | 22:05 | 76° |
| Astrosession begin | 22:21 | 75° |
| Astrosession end | 04:35 | 11° |
| Moon Set | 04:45 | 9° |
| Berbericia set | 05:38 |
Track Berbericia Position Throughout the Night
← Fri, 9 May 2025 →
| Time | |
| Altitude | |
| Azimuth |
Shift the map to change the time and observe Berbericia changing position in the night sky.
Berbericia Description
Berbericia, designated as 776 Berbericia, is a main-belt asteroid, located between Mars and Jupiter in the solar system. With a diameter of 152 km, 776 Berbericia completes its orbit around the Sun in 5 years. At the moment, 776 Berbericia is 2.804 AU (419,472,429 km) from Earth, and it is located in the constellation Leo.Current position of Berbericia in Solar System
| Date | Fri, 9 May 2025 |
| Distance from Earth to Berbericia | 2.804 AU (419,472,429km) |
| Elongation | 115° |
| Angular diameter | " |
| Magnitude | 13.26 |
Finder Chart for Berbericia
Double-click to unlock the map.
| Object name | 776 Berbericia |
| Field of view | |
| Limiting magnitude | |
| 776 Berbericia coordinates | 11.694345940508, 25.554141019309 |
| Center coordinates | 11.694345940508, 25.554141019309 |
Annual motion of Berbericia
| Date | Sat, 10 May 2025 |
| Twighlight start | 22:18 |
| Twighlight end | 04:28 |
| Twighlight duration | 6h 10m |
| Rise | 14:28 |
| Set | 05:33 |
| Elevation at transit | 75° |
| Transit time | 22:01 |
| Equatorial coordinates | RA: 11h 41m 31s", Dec: 25° 27' 00s |
| Magnitude | 13 |
| Constellation | Leo |
The graph illustrates the annual visibility pattern of a Berbericia, providing a comprehensive overview of its daily appearances and transit times throughout the year.
The graph is structured with the vertical axis showing the hours of the day, ranging from 12 AM to 12 AM the next day, while the horizontal axis spans each day of the year.
The reddish shaded area indicates the periods when the Berbericia is above the horizon, visible to observers. The white line marks the times when the celestial object reaches its highest point in the sky each day, known as the transit.
The graph is structured with the vertical axis showing the hours of the day, ranging from 12 AM to 12 AM the next day, while the horizontal axis spans each day of the year.
The reddish shaded area indicates the periods when the Berbericia is above the horizon, visible to observers. The white line marks the times when the celestial object reaches its highest point in the sky each day, known as the transit.
Acknowledgments
We acknowledge NASA's Jet Propulsion Laboratory (JPL) for providing essential data on asteroids and comets through their Small-Body Database (SBDB) and Center for Near-Earth Object Studies (CNEOS). Their continuous efforts in tracking and cataloging these celestial bodies make it possible to offer accurate and up-to-date information on their positions, orbits, and physical characteristics.