Understanding > Astronomical calculations
The eclipse is visible from Europe, the northern half of Africa, the Middle East and the Caucasus.
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 67.6 sec.
Julian day : : 2455565.885559
Characteristics | Values |
---|---|
Right ascension of the Sun : | 18h 59m 14.8s. |
Declination of the Sun : | -22° 44' 21.3". |
Right ascension of the Moon : | 18h 58m 23.7s. |
Declination of the Moon : | -21° 46' 1.0". |
Equatorial parallax of the Sun : | 8.9". |
Equatorial parallax of the Moon : | 56' 09.6". |
True semi-diameter of the Sun : | 16' 15.9". |
True semi-diameter of the Moon : | 15' 18.1". |
Magnitude : 0.8572
Circumstances | UT |
---|---|
Beginning of the general eclipse | the 4 at 6h 40m 11.1s |
Maximum of the eclipse | the 4 at 8h 50m 34.0s |
End of the general eclipse | the 4 at 11h 0m 52.2s |