Earth just had a total lunar eclipse. I bundled up and sat outside with a lens watching our full moon traverse the pre-dawn western sky; it orbited entirely through the Earth’s shadow. During umbra, the shadow of the earth completely blocked direct light to the moon for about 59 minutes.
A total eclipse often paints our moon with reddish orange hues. But why is this? The colour results from how faint light gets scattered by the earth’s lower atmosphere. When sunlight takes a long trip through the earth’s lower atmosphere, blue light gets scattered more, so it’s mostly red light that penetrates through to reflect off the moon’s surface. This is much the same light we see during sunset or sunrise.
I was also keen to capture blue light at the edge of the red moon. Minutes before the moon is totally eclipsed by the earth’s shadow, the only direct light reaching the moon’s edge must travel high across the earth’s upper atmosphere. In the upper atmosphere, ozone absorbs most colours, but the blue light penetrates through to reflect off the edge of the moon. This sliver edge of blue light is visible for a relatively short time at the beginning and end of totality, so just before and after the moon is fully within the umbra.
The solar eclipse in the early hours of 3 March 2026 showing the blue light as the moon enters totality. Photo by Cynthia Fraser.

I am grateful to my father, Alistair, who alerted me to the momentary blue light which he photographed during a previous Eclipse in October 2014.



























