Understanding > Astronomical calculations
The central line begins in Africa, goes through the Indian Ocean, passes south of India, and ends in the Pacific Ocean. The eclipse is visible from Asia and Australia. The maximum duration of the centrality is 3m 39.5 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 76.7 sec.
Julian day : : 2458843.718364
Characteristics | Values |
---|---|
Right ascension of the Sun : | 18h 17m 56.6s. |
Declination of the Sun : | -23° 22' 19.3". |
Right ascension of the Moon : | 18h 18m 3.6s. |
Declination of the Moon : | -22° 58'50.6". |
Equatorial parallax of the Sun : | 8.9". |
Equatorial parallax of the Moon : | 57' 04.1". |
True semi-diameter of the Sun : | 16' 15.7". |
True semi-diameter of the Moon : | 15' 33.0". |
Magnitude : 0.9701
Circumstances | UT | Longitude | Latitude |
---|---|---|---|
Beginning of the general eclipse | the 26 at 2h 29m 43.5s | ||
Maximum of the eclipse | the 26 at 5h 17m 36.0s | 102°16.5'E | +1° 0.3' |
End of the general eclipse | the 26 at 8h 5m 36.1s |