422 Berolina (Asteroid)
From South El Monte , 422 Berolina is not observable – it will reach its highest point in the sky during daytime and is no higher than 14° above the horizon at dusk.
Name
422 Berolina
|
Object type
Asteroid
|
Computed for: | 16 September 2025 |
Right ascension: | 15h18m [1] |
Declination: | −22°28' [1] |
Constellation: | Libra |
Magnitude: | 15.32 (V) [1] |
Distance: | 2.41 AU 20.07 lightmin [1] |
Angular motion (speed): | 14.00 arcmin/day[1] |
Angular motion (pos ang): | 289.1° |
Semi-major axis: | 2.23 AU |
Eccentricity: | 0.214393 |
Inclination: | 4.99° |
Longitude ascending node: | 9.03° |
Argument of perihelion: | 335.30° |
Epoch of elements: | 25 January 2025 |
Mean Anomaly at epoch: | 228.12° |
Absolute mag (H): | 10.66 [1] |
Slope parameter (G): | 0.15 [1] |
Perihelion: | 1.75 AU |
Aphelion: | 2.71 AU |
Orbital period: | 3.33 years |
All times shown in South El Monte local time.