Conditions

Why the Moon (and City Lights) Can Ruin Your Aurora Photos

6 MIN READ · AURORA NOTES

It's the most frustrating outcome in aurora chasing: Kp is elevated, Bz has turned firmly south, the sky is completely cloud-free — and the display still looks washed-out and disappointing. Almost always, the culprit is one of two things that have nothing to do with space weather at all: the moon, or the sky glow from a town you didn't think was close enough to matter.

The aurora is usually fainter than people expect

Aurora brightness varies enormously — a strong substorm can be genuinely vivid to the naked eye, but a large share of "active" nights produce a faint, greyish glow that needs a dark, contrast-friendly sky to register as more than a smudge. Anything that raises the background brightness of the sky competes directly with that faint signal, and past a certain point, it simply wins.

How much the moon actually costs you

A full moon is dramatically brighter than most people register consciously, because your eyes adapt to it. It raises the sky's background brightness enough to wash out faint structure and mute color saturation, especially in the lower, dimmer parts of a display. A thin crescent moon, by contrast, adds only a little glow and barely affects viewing.

This is exactly why Moose's visibility score builds in a moonlight discount — trimming the estimate by up to 30% as the moon approaches full, and barely at all near new moon, rather than treating every night as equally dark.

Moon phase
Typical impact
New moon
Negligible — the darkest baseline sky you'll get
Quarter moon
Noticeable on faint displays, minor on strong ones
Full moon
Significant — can mute all but the brighter, more active displays

None of this means a full moon rules out a good night — a genuinely strong storm will still show up. It just means the same Kp value on a full-moon night needs to work harder to look as good as it would near new moon.

Light pollution is the quieter problem

Moonlight at least changes night to night, giving you a schedule to work around. Light pollution from artificial lighting barely changes at all — which makes it easy to underestimate, because you stop noticing it living with it every day.

Scientists measure this with the Light Pollution Index (LPI): the ratio between a location's artificial sky glow and a natural, pristine night sky. An LPI near 0 is a truly dark sky; a bright city center can run past 40 — meaning the sky glow alone is roughly 40 times brighter than a natural night sky, before the aurora even enters the picture.

Not the same as the Bortle scale. Bortle ratings are a subjective, whole-sky judgment made by eye. LPI, the scale Moose uses, is a modeled measurement of artificial brightness straight up (at the zenith) from satellite nighttime-lights data — more consistent from place to place, though it's measuring a related but distinct thing.

Why "the sky looks clear" isn't the same as "the sky is dark"

A clear sky over a well-lit town can still have enough sky glow to hide a moderate aurora entirely, while an equally clear sky twenty minutes outside town, away from the glow dome, shows the same display clearly. Cloud cover and light pollution are separate problems that both have to be solved — a forecast that only checks one is only half a forecast.

What actually helps

Moose checks all of it at once. Space weather, cloud cover, moon phase, and your local light-pollution zone — combined into one score.
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