Final answer:
The basic evolutionary sequence of a low-mass star like our Sun is: main sequence, red giant, planetary nebula, white dwarf, protostar.
Step-by-step explanation:
The basic evolutionary sequence of a low-mass star like our Sun is: c. Main sequence, red giant, planetary nebula, white dwarf, protostar.
A star with a mass like that of the Sun evolves from the main sequence phase to become a red giant. After the red giant phase, it will expel its outer layers to form a planetary nebula. The remaining core of the star then becomes a white dwarf, which slowly cools over billions of years.