An eclipse is a shadow. When the Sun, Earth and Moon fall into a straight line, one body's shadow lands on another β and for a few minutes the everyday sky does something astonishing.
In a solar eclipse the Moon passes between us and the Sun at New Moon, and the Moon's shadow sweeps a narrow track across the Earth. In a lunar eclipse the Earth passes between the Sun and the Moon at Full Moon, and the Moon glides through Earth's shadow, often glowing a deep copper-red.
New Moon: the Moon blocks the Sun. Its shadow is tiny where it hits Earth, so totality is only ever seen along a narrow path a few tens of km wide.
Full Moon: the Moon enters Earth's long shadow. That shadow is huge, so a lunar eclipse is visible from the entire night side of Earth at once.
So why isn't there an eclipse every month? Because the Moon's orbit is tilted about 5Β° to Earth's path around the Sun. Most months the Moon passes a little above or below the Sun or shadow and misses. Only when a New or Full Moon happens near a node β where the two orbits cross β do the three bodies line up well enough. Those alignments repeat in the famous saros cycle of about 18 years 11 days.
Solar (at New Moon):
Lunar (at Full Moon):
Pick a solar eclipse to trace the path of totality (or annularity) across the Earth. A lunar eclipse is visible from the whole night side, so its βregionβ is a hemisphere, not a line.
Eclipse dates, types, durations and paths are from NASA's Goddard Eclipse Web Site (Espenak & Meeus) and cross-checked with timeanddate.com. The world map is schematic β the path lines are approximate; for the precise track and local circumstances use the per-eclipse links, and for Singapore's exact local times see timeanddate.com/eclipse/in/singapore. This list runs to 2030 and should be reviewed before then. Countdown is computed on your device. Science Centre Observatory, Singapore.