Skywatchers are in for a celestial treat as a total lunar eclipse is set to take place between the late hours of March 13 and the early morning of March 14, 2025. During this event, the Moon will move into Earth’s shadow, taking on a striking red hue—an occurrence often referred to as a “Blood Moon.”
What to Expect During the Eclipse
The eclipse will unfold over several hours, with different phases visible at different times. According to the expected schedule (all times in Central Time):
- 10:57 PM – The penumbral eclipse begins as the Moon enters Earth’s outer shadow. The dimming effect is subtle at this stage.
- 12:09 AM – The partial eclipse begins. The Moon starts moving into the Earth’s umbra, appearing as if a bite has been taken out of it.
- 1:26 AM – Totality begins. The Moon is now completely within Earth’s shadow and glows a deep coppery red.
- 2:31 AM – Totality ends, and the Moon gradually exits the umbra, fading back to its usual color.
- 3:47 AM – The partial eclipse concludes.
- 5:00 AM – The penumbral eclipse ends, marking the end of the event.
The entire event will be visible across the Western Hemisphere, with totality occurring at approximately 2:26 AM Eastern Time (11:26 PM Pacific Time).
How to Watch the Eclipse
Observing the lunar eclipse requires no special equipment—just a clear view of the night sky. However, using binoculars or a telescope can enhance the experience by bringing out details of the Moon’s surface. The best viewing conditions will be away from bright city lights.
Why Does the Moon Turn Red?
The Moon’s transformation into a reddish hue is caused by a phenomenon known as Rayleigh scattering—the same process that makes sunsets appear red. As sunlight passes through Earth’s atmosphere, shorter blue wavelengths scatter, allowing the longer red and orange wavelengths to reach the Moon’s surface. Essentially, during a lunar eclipse, all of Earth’s sunrises and sunsets are cast onto the Moon.
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