Understanding > Astronomical calculations
The eclipse is visible between Africa and Antarctica.
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 68.1 sec.
Julian day : : 2455743.878852
Characteristics | Values |
---|---|
Right ascension of the Sun : | 6h 40m 1.7s. |
Declination of the Sun : | +23° 07' 6.0". |
Right ascension of the Moon : | 6h 39m 2.0s. |
Declination of the Moon : | +21° 42'6.0". |
Equatorial parallax of the Sun : | 8.6". |
Equatorial parallax of the Moon : | 57' 24.6". |
True semi-diameter of the Sun : | 15' 43.9". |
True semi-diameter of the Moon : | 15' 38.6". |
Magnitude : 0.0966
Circumstances | UT |
Beginning of the general eclipse | the 1 at 7h 53m 47.3s |
Maximum of the eclipse | the 1 at 8h 38m 24.3s |
End of the general eclipse | the 1 at 9h 22m 45.0s |