Understanding > Astronomical calculations
The central line begins in Africa goes through the Arabian Peninsula, Pakistan, China, Taiwan, and ends in the Pacific Ocean. The maximum duration of the centrality is 0m 38.2 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 77.2 sec.
Julian day : : 2459021.778685
Characteristics | Values |
---|---|
Right ascension of the Sun : | 6h 1m 33.0s. |
Declination of the Sun : | +23° 26' 9.7". |
Right ascension of the Moon : | 6h 1m 30.1s. |
Declination of the Moon : | +23° 32'57.2". |
Equatorial parallax of the Sun : | 8.7". |
Equatorial parallax of the Moon : | 56' 31.1". |
True semi-diameter of the Sun : | 15' 44.2". |
True semi-diameter of the Moon : | 15' 24.0". |
Magnitude : 0.9940
Circumstances | UT | Longitude | Latitude |
---|---|---|---|
Beginning of the general eclipse | the 21 at 3h 45m 53.8s | ||
Maximum of the eclipse | the 21 at 6h 39m 59,3s | 79°41.3'E | +30° 31.6' |
End of the general eclipse | the 21 at 9h 33m 57.5s |