Enjoy the total lunar eclipse on March 3 because it will be the last for a long while.
Observers across East Asia, Australia, the Pacific and western North America will see March’s full moon — known as the “Worm Moon” — pass through Earth’s shadow, turning a reddish-copper color for 58 spell-binding minutes.
However, once the moon emerges from Earth’s umbra — the deepest part of Earth’s shadow — there will be no further total lunar eclipses for almost three years. A lunar lull will commence and won’t end until a neatly-timed total lunar eclipse on New Year’s Eve 2028-2029. Here’s why — and why 2029 will be a year marking not just the end of a drought, but of three spectacular “blood moon” total lunar eclipses.
Lunar eclipses: total vs. partial vs. penumbral
A lunar eclipse occurs when the full moon passes through Earth’s ever-present shadow. A cone-like shadow extending from the night side of the planet, it has two parts: a lighter outer penumbra and a darker central umbra. That’s because the sun is larger than Earth, so Earth blocks its light in different ways.
Total lunar eclipse: when the whole of the moon passes through the umbra, cutting off all direct sunlight from reaching the lunar surface. The only light that can reach it is filtered through Earth’s atmosphere, which scatters short wavelengths of light and bends longer red wavelengths inward. The result is the “blood moon.”
Partial lunar eclipse: when a portion of the moon passes through the umbra, cutting off all direct sunlight from reaching some of the lunar surface. The result is the sight of Earth’s shadow moving across the full moon, turning some of it a dull grey.
Penumbral lunar eclipse: when none of the moon passes through the umbra, just the outer penumbra, causing the moon to lose some of its brightness.
A total lunar eclipse includes all of these phases: penumbral, partial, and total, a process that can take about five hours.
March 3’s total lunar eclipse
The March 3, 2026, total lunar eclipse will see the moon spend 58 minutes and 18 seconds fully inside Earth’s umbra. It has an umbral magnitude of about 1.15, meaning the moon just passes full inside Earth’s shadow. Total lunar eclipses with magnitudes only slightly above 1 tend to appear lighter copper or reddish in tone rather than a very dark crimson, because the moon does not travel deeply through the shadow.
That’s a mere detail; this total lunar eclipse is sure to be a dramatic event, turning a night sky bleached to blue by the full “Worm Moon” to a very dark sky, with stars appearing around the full moon. The entire event, including the long partial phases before and after totality, will last five hours and 38 minutes.
After March 3, the moon won’t fully enter Earth’s umbra again until the very end of 2028.
Why will total lunar eclipses disappear for a few years?
The no-totality gap after March 2026 is not unusual. Total lunar eclipses require precise alignments, far more so than partial or penumbral events. That’s because the moon’s orbit is tilted by about five degrees relative to Earth’s orbit around the sun, which means most full moons pass above or below Earth’s shadow — the reason why there isn’t an eclipse every month. In fact, lunar eclipses can only occur during eclipse seasons, brief windows about six months apart when the sun is near one of the moon’s orbital nodes. But even then, totality is not guaranteed.
During many eclipse seasons, the moon merely skims Earth’s penumbra and umbra. Partial eclipses — when some of the full moon enters the umbra — can be striking events, but at no point does the lunar surface look reddish. Penumbral eclipses are even subtler, with the lunar surface merely dulled. Compared to a total lunar eclipse, partial and penumbral events lack the drama of totality.
What happens to lunar eclipses after March 2026?
After March 3, 2026, there will be no occasions when the moon becomes fully immersed in Earth’s umbra for 34 months. Eclipse seasons continue, and lunar eclipses still occur, but none will be total. Here’s the sequence of partial and penumbral events to expect from 2026 to 2028.
- Aug. 28, 2026 — deep partial lunar eclipse (93% of the moon enters the umbra)
- Feb. 20, 2027 — penumbral lunar eclipse
- July 18, 2027 — penumbral lunar eclipse
- Aug. 17, 2027 — penumbral lunar eclipse
- Jan. 12, 2028 — shallow partial lunar eclipse
- July 6, 2028 — partial lunar eclipse (39% of the moon enters the umbra)
When total lunar eclipses return
The drought finally ends at the close of 2028, when the slow westward drift of the moon’s orbital nodes brings full moons back into deeper alignment with Earth’s shadow. What follows will be a tetrad of three total lunar eclipses in a 12-month period.
- December 31, 2028 — total lunar eclipse (totality for 71 minutes as seen from Africa, Europe, Asia, Australia, Canada and Alaska).
- June 26, 2029 — total lunar eclipse (totality for 102 minutes as seen from the Americas, western Europe and Africa).
- December 20, 2029 — total lunar eclipse (totality for 54 minutes as seen from North and South America, Europe, Africa, the Middle East and Asia).
Total lunar eclipses are not rare, but they are episodic, appearing in clusters when the geometry lines up. Are these night-side events worth traveling the world to see? Perhaps not — particularly compared to the geographically much more limited total solar eclipses — but any one location can go many years without one. One thing’s for sure about total lunar eclipses: every skywatcher should always know when and where the next one is.
