Understanding > Astronomical calculations
The eclipse is visible from 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 70.9 sec.
Julian day : : 2456776.734600
| Characteristics | Values |
|---|---|
| Right ascension of the Sun : | 2h 25m 52.9s. |
| Declination of the Sun : | +14° 26' 54.2". |
| Right ascension of the Moon : | 2h 26m 45.9s. |
| Declination of the Moon : | +13° 31'6.5". |
| Equatorial parallax of the Sun : | 8.7". |
| Equatorial parallax of the Moon : | 54' 24.1". |
| True semi-diameter of the Sun : | 15' 52.9". |
| True semi-diameter of the Moon : | 15' 38.4". |
Magnitude : 0.9842
| Circumstances | UT | Longitude | Latitude |
|---|---|---|---|
| Beginning of the general eclipse | the 29 at 3h 52m 38.1s | ||
| Maximum of the eclipse | the 29 at 6h 3m 24.3s | 131 °18,3'E | -70° 38,7' |
| End of the general eclipse | the 29 at 8h 14m 27.7s |
