Understanding > Astronomical calculations
The eclipse is partial, visible from China, Siberia, Japan and the north of the Pacific ocean.
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 75.7 sec.
Julian day : : 2458489.571929
Characteristics | Values |
---|---|
Right ascension of the Sun : | 19h 06m 57.3s. |
Declination of the Sun : | -22° 32' 36.8". |
Right ascension of the Moon : | 19h 06m 52.9s. |
Declination of the Moon : | -21° 30'36.9". |
Equatorial parallax of the Sun : | 8.9". |
Equatorial parallax of the Moon : | 54' 27.6". |
True semi-diameter of the Sun : | 16' 15.9". |
True semi-diameter of the Moon : | 14' 50.4". |
Magnitude : 0.7147
Circumstances | UT |
Beginning of the general eclipse | the 5 at 23h 34m 1.8s |
Maximum of the eclipse | the 6 at 1h 41m 21.7s |
End of the general eclipse | the 6 at 3h 48m 44.1s |