Solar Eclipse Prime Page
Annular Solar Eclipse of 1556 Nov 02
Fred Espenak
Introduction
The Annular Solar Eclipse of 1556 Nov 02 is visible from the geographic regions shown on the map to the right. Click on the map to enlarge it. For an explanation of the features appearing in the map, see Key to Solar Eclipse Maps.
The instant of greatest eclipse takes place on 1556 Nov 02 at 07:22:12 TD (07:19:48 UT1). This is 0.2 days before the Moon reaches apogee. During the eclipse, the Sun is in the constellation Libra. The synodic month in which the eclipse takes place has a Brown Lunation Number of -4528.
The eclipse belongs to Saros 116 and is number 47 of 70 eclipses in the series. All eclipses in this series occur at the Moons descending node. The Moon moves northward with respect to the node with each succeeding eclipse in the series and gamma increases.
The solar eclipse of 1556 Nov 02 is an exceptionally long annular eclipse with a duration at greatest eclipse of 10m24s. It has an eclipse magnitude of 0.9190.
The annular solar eclipse of 1556 Nov 02 is followed two weeks later by a partial lunar eclipse on 1556 Nov 17.
These eclipses all take place during a single eclipse season.
The eclipse predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., UT1 = TD - ΔT). ΔT has a value of 144.1 seconds for this eclipse.
The following links provide maps and data for the eclipse.
- Orthographic Map: Annular Solar Eclipse of 1556 Nov 02 - global map of eclipse visibility
- Google Map: Annular Solar Eclipse of 1556 Nov 02 - interactive map of the eclipse path
- Path Table: Annular Solar Eclipse of 1556 Nov 02 - coordinates of the central line and path limits
- Circumstances Table: Annular Solar Eclipse of 1556 Nov 02 - eclipse times for hundreds of cities
- Saros 116 Table - data for all eclipses in the Saros series
The tables below contain detailed predictions and additional information on the Annular Solar Eclipse of 1556 Nov 02 .