Apparent magnitude measures how bright a star appears from Earth, using a logarithmic scale where 0 is the brightest and 6 is the limit for the naked eye. The term "system of 3 stars" likely refers to comparing an unknown star's brightness with three known stars, possibly related to the delta Cephei experiment. The scale is not linear; for example, three stars of magnitude 3 together appear as bright as one star of magnitude 1.8. To calculate combined brightness, individual magnitudes must be converted to luminosity, summed, and then converted back to magnitude. Apparent magnitude reflects observed brightness, which varies with distance from the observer.