Understanding > Astronomical calculations
The central line begins at the eastern Pacific Ocean, gores through Chile, Argentina, South Atlantic and ends in Africa. The eclipse is visible from southern South America and from southern Africa. The maximum duration of the centrality is 0m 44.0 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 73.8 sec.
Julian day : : 2457811.110218
Characteristics | Values |
---|---|
Right ascension of the Sun : | 22h 39m 23.1s. |
Declination of the Sun : | -8° 29' 39.2". |
Right ascension of the Moon : | 22h 39m 53.1s. |
Declination of the Moon : | -8° 55' 4.1". |
Equatorial parallax of the Sun : | 8.9". |
Equatorial parallax of the Moon : | 57' 58.7". |
True semi-diameter of the Sun : | 16' 9.1". |
True semi-diameter of the Moon : | 15' 47.9". |
Magnitude : 0.9922
Circumstances | UT | Longitude | Latitude |
---|---|---|---|
Beginning of the general eclipse | the 26 at 12h 10m 44.8s | ||
Maximum of the eclipse | the 26 at 14h 53m 21.4s | 31°10.7'W | -34° 40.9' |
End of the general eclipse | the 26 at 17h 35m 58.4s |