Photometry & Magnitudes

Magnitude Difference & Brightness Ratio Workbench

Convert paired magnitudes, a signed magnitude difference or a flux ratio, with explicit A/B direction and an optional reference magnitude.

Astronomy & Space · model workbench

Follow the reversed magnitude scale without losing which source is brighter.

Private calculations in your browser · explicit inputs and model boundaries
Example preview · Five magnitudes brighterA brighter source moves toward a lower magnitude
-6-2.4-3-1.20031.262.4Entered comparison: 2, -5log10(FA / FB)mA − mB (mag)

A is brighter than B. Zero on both axes means equal flux. One horizontal unit multiplies A/B by ten and lowers A-minus-B magnitude by 2.5.

  1. 1EnterProvide the known values
  2. 2CalculateResults update automatically
  3. 3VerifyReview the details and units
Try an example

Name the passband and magnitude system, or explicitly state bolometric. Quantities being compared must share the stated convention.

Enter values in mag.

Enter values in mag.

Calculation result

Enter valid values to see the result.

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Understand the relationship

The reasoning behind the result

Lower magnitude means more flux

mA−mB=−2.5 log₁₀(FA/FB)

Magnitude is a logarithmic coordinate for brightness. The negative sign reverses the ordering: a negative A-minus-B difference means A delivers more flux. Five magnitudes lower corresponds to a hundred times the flux, independent of the starting magnitude.

The ratio is of measured flux in a compatible passband and convention. It is not automatically a ratio of total luminosity, source size or distance.

A reference anchors the difference

mA=mB+Δm

A difference determines a ratio but does not determine either absolute flux. Supplying B's magnitude locates A on the same magnitude scale. Negative magnitudes are valid and do not mean negative flux.

The reciprocal FB/FA reverses the comparison. A source with half the reference flux is about 0.752575 magnitudes fainter; saying it is half a magnitude fainter would describe a different ratio.

Fractional change keeps its sign

Percentage flux change relative to B=100(R−1)

The flux increase uses B as its denominator. A ratio of two means a 100% increase; a ratio of one-half means a 50% decrease. These changes are asymmetric when the reference is reversed.

The graph uses log10 of A/B on the horizontal axis, so equal spacing represents equal multiplicative changes. Its straight line is a logarithmic relationship, not a linear-flux brightness law.

Logarithmic magnitudes require positive flux

A zero or negative measured flux can occur after background subtraction, but it has no finite ordinary logarithmic magnitude. This converter requires a strictly positive ratio. It does not substitute a detection limit or use an asinh magnitude convention.

Extremely large differences can still be represented logarithmically while their ratios exceed numerical range. Those derived ratios are labelled explicitly; the signed difference and log ratio remain available.

Follow the numbers

Half the flux of a magnitude-10 reference

  1. Enter FA/FB=0.5 and mB=10.
  2. Δm=−2.5 log10(0.5)=0.752574989 mag, so mA=10.752574989 mag.
  3. The reciprocal ratio is 2 and the flux change relative to B is 100(0.5−1)=−50%.

A is fainter even though its numerical magnitude is larger.

Quick guide

How to use this calculator

  1. State the shared band and magnitude convention.
  2. Choose a pair, a signed A-minus-B difference or a positive A/B flux ratio.
  3. If B’s magnitude is known, enable the reference anchor to infer A. Otherwise retain the ratio and difference alone.
  4. Read the direction statement and reciprocal ratio before using the comparison.

Calculation method

Calculation and interpretation

Follow the reversed magnitude scale without losing which source is brighter.

Δm=mA−mB=−2.5 log₁₀(FA/FB); R=FA/FB=10^(−0.4Δm); mA=mB+Δm.

Worked example

Half the flux of a magnitude-10 reference

A is fainter even though its numerical magnitude is larger.

Δm=mA−mB=−2.5 log₁₀(FA/FB); R=FA/FB=10^(−0.4Δm); mA=mB+Δm.

Supported inputs

Precision and limits

Matched photometry

Different bands, zero points, extinction corrections or magnitude conventions must be reconciled before interpreting the ratio.

No absolute power inference

A relative flux ratio does not determine luminosity or source distance, and no uncertainty is inferred from the entered digits.

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