Understanding > Astronomical calculations
The central line begins in the Atlantic ocean, goes across Africa, and ends in the Pacific. The eclipse is visible from most of Africa. The maximum duration of the centrality is 3m 5.6 s.
Ephemeris used to calculate positions of the Sun and Earth are the ephemeris Newcomb/ILE. For this calculation the value of TE-TU was exceptionally forced at 73.3 sec.
Julian day : : 2457632.887517
Characteristics | Values |
---|---|
Right ascension of the Sun : | 10h 43m 43.3s. |
Declination of the Sun : | +8° 03' 38.3". |
Right ascension of the Moon : | 10h 43m 22.2s. |
Declination of the Moon : | +7° 45'51.3". |
Equatorial parallax of the Sun : | 8.7". |
Equatorial parallax of the Moon : | 55' 48.5". |
True semi-diameter of the Sun : | 15' 51.0". |
True semi-diameter of the Moon : | 15' 12.4". |
Magnitude : 0.9736
Circumstances | UT | Longitude | Latitude |
---|---|---|---|
Beginning of the general eclipse | the 1 at 6h 13m 5.4s | ||
Maximum of the eclipse | the 1 at 9h 6m 50.8s | 37°46.4'E | -10° 40.8' |
End of the general eclipse | the 1 at 12h 0m 37.4s |