Low-mass stars are stars with a mass less than about 2 solar masses. Despite being the most common type of star in the universe, low-mass stars have characteristics and behaviors that differ significantly from their higher-mass counterparts. Low-mass stars typically have longer lifespans than higher-mass stars, as they burn fuel at a slower rate and undergo nuclear fusion in their cores at a much slower pace. This gives low-mass stars the ability to remain stable on the main sequence for billions or even trillions of years. Research on low-mass stars includes studying their formation, evolution, and behavior. This includes understanding how low-mass stars form from molecular clouds, how they evolve over time, and how their properties change as they age. Additionally, low-mass stars are of particular interest in the search for exoplanets, as they are more likely to host habitable planets due to their longer lifespans and stable environments. Studying low-mass stars can provide valuable insights into the potential habitability of planets orbiting them. Overall, research on low-mass stars is crucial for understanding the evolution and behavior of stars, as well as for exploring the possibility of life beyond our solar system.