Understanding > Astronomical calculations
The eclipse is visible from Canada to Siberia through the north of Europe.
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 75.3 sec.
Julian day : : 2458341.888884
Characteristics | Values |
---|---|
Right ascension of the Sun : | 9h 24m 28.0s. |
Declination of the Sun : | +15° 13' 19.3". |
Right ascension of the Moon : | 9h 25m 31.3s. |
Declination of the Moon : | +16° 21'41.3". |
Equatorial parallax of the Sun : | 8.7". |
Equatorial parallax of the Moon : | 1° 1' 10.0". |
True semi-diameter of the Sun : | 15' 46.8". |
True semi-diameter of the Moon : | 16' 40.0". |
Magnitude : 0.7361
Circumstances | UT |
Beginning of the general eclipse | the 11 at 8h 2m 4.8s |
Maximum of the eclipse | the 11 at 9h 46m 15.0s |
End of the general eclipse | the 11 at 11h 30m 38.7s |