422 Berolina (Asteroid)
From South El Monte , 422 Berolina is not readily observable since it is very close to the Sun, at a separation of only 17° from it.
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Name
422 Berolina
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Object type
Asteroid
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Current position
| Computed for: | 16 December 2025 |
| Right ascension: | 18h52m [1] |
| Declination: | −26°11' [1] |
| Constellation: | Sagittarius |
| Magnitude: | 14.87 (V) [1] |
| Distance: | 2.80 AU 23.26 lightmin [1] |
Orbital elements [1]
| Semi-major axis: | 2.23 AU |
| Eccentricity: | 0.214264 |
| Inclination: | 4.99° |
| Longitude ascending node: | 9.02° |
| Argument of perihelion: | 335.27° |
| Epoch of elements: | 21 Nov 2025 |
| Mean Anomaly at epoch: | 317.05° |
| Absolute mag (H): | 10.64 [1] |
| Slope parameter (G): | 0.15 [1] |
Derived quantities
| Perihelion: | 1.75 AU |
| Aphelion: | 2.71 AU |
| Orbital period: | 3.33 years |