Intensity Ratio for Apparent Magnitude
The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth.
The ratio of celestial intensities equals ten taken to the power of the two-fifths of the difference in apparent magnitudes.
Formula
![Copy to Clipboard QuantityVariable[Subscript["I", "1"]/Subscript["I", "2"], "Unitless"] == 10^((2*(-QuantityVariable[Subscript["m", "1"], "Unitless"] + QuantityVariable[Subscript["m", "2"], "Unitless"]))/5)](https://www.wolframcloud.com/objects/resourcesystem/marketplacestorage/resources/6e0/6e01c23a-6093-4d03-bb41-e4b0c3e3709d/Webpage/FormulaImage.png)
| symbol | description | physical quantity |
|---|---|---|
| I1/I2 | intensity ratio |
"Unitless" |
| m1 | apparent magnitude 1 | "Unitless" |
| m2 | apparent magnitude 2 | "Unitless" |
Forms
Examples
Get the resource:
| In[1]:= |
| Out[1]= | ![]() |
Get the formula:
| In[2]:= |
| Out[2]= |
Use some values:
| In[3]:= |
| Out[3]= |
