11-3 Absolute Magnitudes and Luminosities Flashcards
absolute magnitude (M)
a measure of the total energy emitted by a star, independent of distance to us.
how to calculate absolute magnitude
it is necessary to know the distance of the star and apparent brightness. apparent brightness m decreases inversely with the square of the distance between the source and the observer. M is the apparent brightness corrected by the distance. is the brightness a star would have if it were at a distance of 10 pc from us
the inverse-square law
the same amount of radiation from a light source must illuminate an ever-increasing area as the distance from the light source increases. the decrease in brightness follows the inverse-square law. for example, tripling the distance decreases the brightness by a factor between 3^2=9
the distance-magnitude relationship
M = m - 5log (d/10)
m - M = 5logd - 5