151 Abundantia (Asteroid)
From South El Monte , 151 Abundantia is not readily observable since it is very close to the Sun, at a separation of only 3° from it.
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Name
151 Abundantia
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Object type
Asteroid
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| Computed for: | 05 June 2026 |
| Right ascension: | 04h57m [1] |
| Declination: | +25°32' [1] |
| Constellation: | Taurus |
| Magnitude: | 14.39 (V) [1] |
| Distance: | 3.61 AU 29.99 lightmin [1] |
| Semi-major axis: | 2.59 AU |
| Eccentricity: | 0.036140 |
| Inclination: | 6.43° |
| Longitude ascending node: | 38.72° |
| Argument of perihelion: | 131.90° |
| Epoch of elements: | 9 Jun 2026 |
| Mean Anomaly at epoch: | 271.29° |
| Absolute mag (H): | 9.32 [1] |
| Slope parameter (G): | 0.15 [1] |
| Perihelion: | 2.50 AU |
| Aphelion: | 2.69 AU |
| Orbital period: | 4.17 years |
All times shown in South El Monte local time.