When describing stars, apparent brightness is denoted by b.
(1) State what is meant by apparent brightness, b.
(2) Show that the apparent brightness b⊙ of the Sun, of luminosity L⊙=3.83×1026W, is 1.4×103W m−2 when the Sun is 1.5×1011m from Earth. State the usual name of this quantity.
(3) Calculate the apparent brightness of a star with luminosity 5.0×1028W at a distance of four light-years.