28/08/2026
What Happened to the Moon Around Midnight?
At about 12:13 a.m. EDT on August 28, 2026, the Moon reached the maximum phase of a deep partial lunar eclipse. NASA reports that 96.3% of the Moon’s visible disk was inside Earth’s umbra—the dark central region of our planet’s shadow—while only a thin portion remained in direct sunlight. This explains the extraordinary appearance seen around midnight: a brilliant white cap above a much darker copper-orange lunar surface. (NASA Scientific Visualization Studio)
A lunar eclipse occurs near full Moon when the Sun, Earth and Moon align with Earth in the middle. This alignment was extremely close, but not quite perfect enough to produce a total eclipse. The event had an umbral magnitude of about 0.93, meaning roughly 93% of the Moon’s diameter extended into the umbra at maximum. Because of the geometry of the shadow, this corresponded to about 96.3% of the lunar disk by area being shadowed. (EclipseWise)
The reddish-orange color was also caused by Earth. Although our planet blocks direct sunlight from the umbra, some sunlight passes through the edges of Earth’s atmosphere. Air molecules scatter shorter blue and violet wavelengths more efficiently, while longer red and orange wavelengths pass through more readily and are refracted into Earth’s shadow. Those filtered rays then illuminate the eclipsed Moon. The physics is closely related to the process that produces red sunrises and sunsets. (NASA Science)
The eclipse began with the Moon entering Earth’s faint penumbra at about 9:24 p.m. EDT on August 27. The partial phase began around 10:34 p.m., reached maximum shortly after midnight, ended around 1:52 a.m., and the penumbral phase finished near 3:02 a.m. The entire phenomenon lasted roughly 5 hours 38 minutes, while the dramatic partial phase lasted about 3 hours 19 minutes. (EclipseWise)
Unlike a solar eclipse, a lunar eclipse is safe to observe with the naked eye, binoculars or a telescope. What appeared in the sky this morning was therefore a remarkable real-time demonstration of orbital mechanics, Earth’s curved shadow, and atmospheric optics.
