Understanding > Astronomical calculations
The central line begins in the western part of ocean Atlantic and ends at the east of the African continent. It is visible from northern South America to the south of Europe. The maximum duration of the centrality isf 1m 39.6 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 70.4 sec.
Julian day : : 2456600.026923
Characteristics | Values |
---|---|
Right ascension of the Sun : | 14h 35m 19.8s. |
Declination of the Sun : | -15° 12' 22.3". |
Right ascension of the Moon : | 14h 35m 37.0s. |
Declination of the Moon : | -14° 53'29.8". |
Equatorial parallax of the Sun : | 8.9". |
Equatorial parallax of the Moon : | 59' 11.0". |
True semi-diameter of the Sun : | 16' 7.4". |
True semi-diameter of the Moon : | 16' 7.6". |
Magnitude : 1.0159
Circumstances | UT | Longitude | Latitude |
---|---|---|---|
Beginning of the general eclipse | the 3 at 10h 4m 33.7s | ||
Maximum of the eclipse | the 3 at 12h 46m 28.3s | 11 °41.5'W | +3° 30.1' |
End of the general eclipse | the 3 at 15h 28m 21.0s |