astronomylabMeet the Moon
A small number. A bright star.

Stellar brightness

Compare the apparent brightness of two objects using the astronomical magnitude scale.

Stellar brightnessInteractive model
A · 1 magB · 6 magSymbol sizes compressed; compare numerical flux ratio
Flux A / Flux B100×
Magnitude difference5 mag
Brighter objectObject A

Your experiment

10^(0.4 × (6 − 1)) = 100. Object A delivers 100 times the flux of object B in the same band.

How it works

Brightness A / Brightness B = 10^(0.4 × (mB − mA))

The magnitude scale runs backward: smaller numbers mean brighter objects. It is logarithmic, so a difference of five magnitudes corresponds to a factor of one hundred in brightness.

Read the field note ↗

About this model
Both magnitudes must refer to the same photometric band. This compares received flux, not intrinsic luminosity. Symbol sizes use a compressed scale.

Keep wondering

Stellar brightness: common questions

Can a magnitude be negative?

Yes. Very bright objects have negative apparent magnitudes. Zero is a reference level, not a lower limit.

What is absolute magnitude?

It is the apparent magnitude an object would have at a distance of ten parsecs, with extinction accounted for.

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