Understanding > Astronomical calculations
The eclipse is visible in Antarctica and in the south of South America.
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 74.8 sec.
Julian day : : 2458165.343776
| Characteristics | Values |
|---|---|
| Right ascension of the Sun : | 21h 57m 18.7s. |
| Declination of the Sun : | -12° 28' 7.7". |
| Right ascension of the Moon : | 21h 58m 26.8s. |
| Declination of the Moon : | -13° 32'30.6". |
| Equatorial parallax of the Sun : | 8.9". |
| Equatorial parallax of the Moon : | 55' 0.9". |
| True semi-diameter of the Sun : | 16' 11.4". |
| True semi-diameter of the Moon : | 14' 59.4". |
Magnitude : 0.5986
| Circumstances | UT |
|---|---|
| Beginning of the general eclipse | the 15 at 18h 55m 45.8s |
| Maximum of the eclipse | the 15 at 20h 51m 18.6s |
| End of the general eclipse | the 15 at 22h 47m 3.4s |
