
On Thursday night and into Friday morning, the Earth, sun, and moon will align perfectly, casting the moon into Earth’s shadow. The result? A striking red-orange glow in the sky, a phenomenon known as a lunar eclipse, often called a ‘Blood Moon.’
Here’s everything you need to know to catch the celestial show on March 13-14:
How to see it
According to NASA, the lunar eclipse will be visible to the naked eye, though binoculars or a telescope will enhance the view. For the best experience, head to a dark area away from city lights to avoid light pollution.
Timeline
- 10:57 p.m. – Penumbral eclipse begins: The moon begins to enter Earth’s outer shadow, causing a subtle dimming.
- 12:09 a.m. – The partial eclipse begins. A dark “bite” will appear as the moon moves into Earth’s umbra (the darkest part of its shadow).
- 1:26 a.m. – The total eclipse begins. The entire moon will turn a deep, coppery red.
- 2:31 a.m. – Totality ends: The moon starts exiting Earth’s umbra, gradually returning to its normal appearance.
- 3:47 a.m. – The partial eclipse ends, leaving only a slight dimming.
- 5:00 a.m. – The eclipse is officially over.
Why does the moon turn red?
Different wavelengths of light scatter differently in the atmosphere. Blue light is scattered more easily, which is why the sky looks blue during the day. Red light, however, travels more directly through the atmosphere — giving us vibrant sunrises and sunsets.
During a lunar eclipse, the Earth blocks most of the sun’s rays, but some red light filters through our atmosphere, casting a warm, reddish glow on the moon.
What else is there to see?
The lunar eclipse isn’t the only treat in the sky! NASA reports that Jupiter and Mars will be visible throughout March, and with the moon’s light dimmed, constellations may be easier to spot than usual.
Set your alarms and get ready for a stunning night in the Big Country!
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