Zubenelschemali (β Lib) - "The Northern Tap" is slightly brighter (2.61 mag) and has a peculiar greenish tint, which is somewhat unusual. The star is approximately 100 times more luminous than the Sun.

Zubenelgenubi (α Lib) - The name means "southern clapper" and refers to the origin of the constellation. It is a very easily distinguishable binary star that can be observed with a small telescope. The primary component has a magnitude of 2.75 and is separated by 231" from the companion with a magnitude of 5.8. In terms of classification, it is a bright wide pair consisting of a white and yellow component. Since both stars exhibit the same proper motion, they are likely a physical binary. Its distance from Earth is 75 light-years.

τ Lib - The pair of stars with magnitudes 4.7 and 9.7 is separated by 8.5", so we can distinguish them with a telescope of at least 6 cm. The system is located 367 light-years away from Earth.

ι Lib - A complex multiple star, which appears as a single star with a brightness of 4.2 mag when observed with the naked eye. The finder will show its companion labeled as 25 Librae. A telescope with an objective diameter over 80 mm will reveal that the primary star has a faint companion of 9 mag at a separation of 58". With a larger telescope and appropriate magnification, it should eventually be proven that it itself is a close binary star. Its faint companion of 11 mag is located at a separation of 1.9" from it.

δ Lib - An eclipsing variable star similar to Algol has a period of 2.32 days and its brightness ranges from 4.92 to 5.9 magnitude. The entire cycle of brightness changes can be observed with the naked eye. The change from maximum to minimum occurs in about 6 hours, which can be noticed in a single spring night. Among the main minima, there is one insignificant secondary minimum, which only reaches a tenth of the stellar magnitude, making it difficult to perceive. The system is located nearly 300 light-years away from Earth.

μ Lib - In a good 100 mm refractor, we will see the binary star as a close pair of white stars, like two disks in contact (1.8 "). We will be able to distinguish them completely under calm atmospheric conditions. The components have magnitudes of 5.8 and 6.7.