The Sun has a life span of approximately ten billion years and is viewed by scientists as belonging to the class of stars known as "main sequence stars." Extensive research indicates that the Sun has long been a middle-age star and will at some time in the foreseeable future commence development into a red giant star before cooling down into a white dwarf. Since the Sun is of megaton proportions making it proportionately more difficult to extract viable laboratory specimens, it seems reasonable to think that the effects of solar aging will be observed sooner and more readily on a planetary level, i.e., on a systemic order of magnitude. Some solar oriented scientists detect signs displayed by the Sun of a transitional phase during which hydrogen burning ceases and helium burning commences, which is an indicator of a need for reclassification, i.e., stellar identification of Earth's Sun as transitioning into a red giant which is leaving main sequence middle age and heading, figuratively and literally, into its "sunset years" before senescence as a white dwarf star joining its peers in the Milky Way galaxy.