487 Venetia (Asteroid)
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From South El Monte , 487 Venetia is not readily observable since it is very close to the Sun, at a separation of only 20° from it.
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Name
487 Venetia
|
Object type
Asteroid
|
Current position
| Computed for: | 01 June 2026 |
| Right ascension: | 06h02m [1] |
| Declination: | +21°19' [1] |
| Constellation: | Orion |
| Magnitude: | 13.73 (V) [1] |
| Distance: | 3.47 AU 28.88 lightmin [1] |
Orbital elements [1]
| Semi-major axis: | 2.67 AU |
| Eccentricity: | 0.086231 |
| Inclination: | 10.25° |
| Longitude ascending node: | 114.75° |
| Argument of perihelion: | 281.89° |
| Epoch of elements: | 21 Nov 2025 |
| Mean Anomaly at epoch: | 9.83° |
| Absolute mag (H): | 8.43 [1] |
| Slope parameter (G): | 0.15 [1] |
Derived quantities
| Perihelion: | 2.44 AU |
| Aphelion: | 2.90 AU |
| Orbital period: | 4.36 years |
Visibility from South El Monte
All times shown in South El Monte local time.