A. For the Mass of 1 X the Sun, place your curser on the dot, and record the beginning temperature and brightness in the table below. B. Run the simulation. Keep an eye on the stage. Pause the simulation when it reaches the next stage. In complete sentences, record how long the star stayed in the Main Sequence stage and the star's next stage (giant, supergiant, white dwarf...). C. Play the simulation again. Record what happens to the size, brightness, and temperature of the star. D. Once the simulation is done, record the highest temperature and brightness. . To find the highest temperature, trace your mouse along the path of the star's life until you have the highest x value. . To find the highest brightness, trace your mouse along the path of the star's life until you have the highest y value. 8 points Star Beginning Highest Beginning Highest Summary Mass Temperature Temperature Brightness Brightness 1 X Sun 5924 604871 0.96 4367 The star changed from the Main Sequence to a Red Giant at 5468 degrees. Temperature rises when brightness rises and temperature