Only Hubble Space Telescope has the required sensitivity and resolution to detect these "cosmic milepost" type stars out to great distances from Earth, according to astronomers. Typically, Cepheids in a crowded region of a distant galaxy are too faint and the resolution too poor, as seen from ground-based telescopes, to be detected clearly. Hubble was used to make twelve one-hour exposures, timed carefully in a two-month observing window, to discover 20 Cepheid variable stars in the M100 galaxy. Though M100 is the most distant galaxy in which Cepheid variables have been discovered, HST must find Cepheids in even more distant galaxies before accurate distances can be used to calculate a definitive size and age for the universe.
The Hubble Space Telescope image was taken with the Wide Field Planetary Camera 2 (WFPC 2). This black and white picture was taken at visible light wavelengths.
M100 (100th object in the Messier catalog of non-stellar objects) is a member of the huge Virgo cluster of an estimated 2,500 galaxies. The galaxy can be seen by amateur astronomers as a faint, pinwheel-shaped object in the spring constellation Coma Berenices.