α Tuc - The brightest star of the constellation has an apparent magnitude of 2.91 and an orange hue. It is located 62 light-years away from Earth.

β Tuc - not only an optical, but also a physical binary star. Two almost equally bright components with magnitudes of 4.4 and 4.5 are separated by 27.1", so we can distinguish them well in a good binocular. Both are further doubled, which we can only perceive in a telescope. Additionally, at a distance of 9.3' to the southeast, we can observe a third component with a magnitude of 5.1, which is actually also a close binary star.

δ Tuc - An easily distinguishable double star. The primary component has a brightness of 4.8 magnitude and is separated by 7 arcseconds from a companion with a brightness of 9 magnitude, which can be separated by at least a 100 mm telescope.

κ Tuc - A binary star composed of stars with magnitudes 5 and 8, which can be resolved with a small telescope.