What Causes Them?

The celestial dance between the Sun, Moon, and Earth results in a variety of astronomical phenomena that have fascinated humanity for centuries. Among these awe-inspiring events, solar eclipses captivate the attention of even the most casual stargazer. While total solar eclipses often steal the limelight, annular eclipses offer their own unique spectacle. But what causes an annular eclipse, and how does it differ from other types of solar eclipses?

What is an Annular Eclipse?

An annular eclipse occurs when the Moon passes between the Earth and the Sun but doesn't cover the Sun entirely. Unlike a total solar eclipse, where the Sun disappears for a few moments, an annular eclipse leaves a visible "ring of fire" around the Moon. The term "annular" comes from the Latin word "annulus," which means ring. This spectacular display happens when the apparent size of the Moon is smaller than that of the Sun as seen from Earth.

The Role of Orbital Mechanics

To understand why annular eclipses occur, we need to delve into the mechanics of celestial orbits. Both the Earth and Moon have elliptical orbits, which means their distances from the Sun and each other can vary. Earth's distance from the Sun ranges from about 91 million miles (147 million km) at its closest (perihelion) to approximately 94.5 million miles (152 million km) at its farthest (aphelion). Similarly, the Moon’s distance from Earth can range from around 225,623 miles (363,104 km) to about 251,966 miles (405,696 km).

The Angular Diameter: Apparent Size Matters

The concept of angular diameter plays a critical role in the occurrence of annular eclipses. Angular diameter is a measure of how large an object appears to an observer. Even though the Sun is about 400 times larger than the Moon, it is also about 400 times farther away from Earth. This coincidence means that both celestial bodies can have nearly the same angular diameter as viewed from Earth.

However, the keyword here is "nearly." Due to the elliptical orbits, the angular diameter of both the Sun and Moon varies slightly over time. When the Earth is near aphelion and the Moon is near its apogee (farthest from Earth), the Moon’s apparent size can be smaller than the Sun’s. During this specific alignment, if a new moon phase coincides, we witness an annular eclipse.

The Saros Cycle

Annular eclipses don't occur randomly but are part of an 18-year, 11-day period known as the Saros cycle. This cycle can predict eclipses and is the result of three lunar orbital periods—namely the synodic month (new moon to new moon), the draconic month (node to node), and the anomalistic month (perigee to perigee)—nearly aligning. Over time, a series of eclipses belonging to the same Saros cycle will shift between partial, total, and annular as the relative distances and angular diameters of the celestial bodies change.

Viewing an Annular Eclipse

While it’s tempting to watch an annular eclipse with the naked eye, doing so can be harmful. Unlike a total solar eclipse, where the Sun is entirely covered for a brief period, the Sun in an annular eclipse is never fully obscured. Therefore, proper eye protection, such as solar viewing glasses, should be used. Telescopes and cameras equipped with solar filters can provide a more detailed view of the "ring of fire," revealing sunspots and other solar features.


Annular eclipses offer a fascinating glimpse into the intricate ballet of celestial mechanics. These events are a reminder of the ever-changing distances and angular diameters that characterize the Earth-Moon-Sun system. Although they may not provide the complete blackout that total eclipses do, the unique "ring of fire" display during annular eclipses remains a captivating spectacle—one that invites us to ponder our place in the cosmos and the marvelous intricacies that govern it.

So, the next time an annular eclipse is due, equip yourself with a solar viewer and partake in witnessing one of nature's most mesmerizing phenomena. It's a cosmic show you won't want to miss.

Roger Sarkis