Understanding > Astronomical calculations
The eclipse is visible between Australia and Antarctica.
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 75.2 sec.
Julian day : : 2458312.631244
| Characteristics | Values |
|---|---|
| Right ascension of the Sun : | 7h 29m 31.1s. |
| Declination of the Sun : | +21° 50' 30.7". |
| Right ascension of the Moon : | 7h 29m 10.9s. |
| Declination of the Moon : | +20° 27'46.6". |
| Equatorial parallax of the Sun : | 8.7". |
| Equatorial parallax of the Moon : | 1° 1' 20.3". |
| True semi-diameter of the Sun : | 15' 44.50. |
| True semi-diameter of the Moon : | 16' 42.8". |
Magnitude : 0.3367
| Circumstances | UT |
|---|---|
| Beginning of the general eclipse | the 13 at 1h 48m 17.5s |
| Maximum of the eclipse | the 13 at 3h 1m 2.4s |
| End of the general eclipse | the 13 at 4h 13m 43.1s |
