416 Vaticana (Asteroid)
From Cambridge , 416 Vaticana is not readily observable since it is very close to the Sun, at a separation of only 3° from it.
Name
416 Vaticana
|
Object type
Asteroid
|
Computed for: | 11 May 2024 |
Right ascension: | 03h27m [1] |
Declination: | +18°19' [1] |
Constellation: | Taurus |
Magnitude: | 13.77 (V) [1] |
Distance: | 4.35 AU 36.15 lightmin [1] |
Angular motion (speed): | 6.66 arcmin/day[1] |
Angular motion (pos ang): | 243.1° |
Semi-major axis: | 2.80 AU |
Eccentricity: | 0.217488 |
Inclination: | 12.87° |
Longitude ascending node: | 58.03° |
Argument of perihelion: | 199.06° |
Epoch of elements: | 31 March 2024 |
Mean Anomaly at epoch: | 138.46° |
Absolute mag (H): | 7.80 [1] |
Slope parameter (G): | 0.15 [1] |
Perihelion: | 2.19 AU |
Aphelion: | 3.41 AU |
Orbital period: | 4.68 years |
All times shown in Cambridge local time.