Al Rischa (α Psc) - From an astronomical point of view, Al Risch is a close binary star (total magnitude 4), with its pale blue components of magnitude 4.3 and 5.2 orbiting each other with a period of 933 years. Currently, they are separated by 1.5" in the sky, requiring a telescope with a 300 mm objective diameter to resolve them. Even at 200x magnification, they appear in close contact. However, due to their orbit, the separation decreases gradually each year, reaching its lowest value of 1" in 2060. The system is located at a distance of 130 light-years and both components are also a spectroscopic binary.

ζ Psc - A nice optical double star with components of 5.6mag and 6.5mag, separated by 23.6". However, in reality, one is located at a distance of 150 light years and the other at 195 light years. The primary component appears white, while the companion has a yellow color. During a good night, it can be easily observed with binoculars, and a small telescope will also work without any problems.

TX Psc - A very interesting irregular variable star, also known as 19 Piscium. The range of its magnitude is from 6.9 to 7.7 and it seems to have no hint of periodicity. TX Psc, with a spectral class of N, is one of the reddest stars within reach of a telescope. In the same field of view, there are ι Psc (4.1 mag) and λ Psc (4.5 mag).

ψ Psc - Wide double star visible in a hand lens. It consists of two components with magnitudes of 5.5 and 5.8, separated by 30". Both have a light blue color and are located 230 light-years away.

55 Psc - A nice double star, in which the primary component has a brightness of 5.6 mag and the companion 8.8 mag. Since they are separated by 6.6", we need a telescope with an objective diameter of at least 6 cm to resolve them. The contrast is intense, with one component having a yellow-orange color and the other a blue color.

42 Psc - This binary star can be easily distinguished with a telescope with a 100 mm objective diameter. It consists of an orange primary component with a brightness of 6.2 magnitude and a companion located 28.5" away with a magnitude of 10.

Van Maanenova hviezda - Wolf 28, a rare example of a relatively well-visible white dwarf, which requires a 200 mm telescope at its brightness of 12.3 mag. This one of the first discovered white dwarfs can be found near the star δ Psc. It is located in close proximity to our Sun, at a distance of 13.8 ly.

38 Psc - Multiple star, attractive pair of yellow stars in a cluster of faint stars. The AB pair is indistinguishable and is perceived as a 7.9 magnitude object, but at a separation of 4.3", we can see a 7.8 magnitude companion. Another, this time of 12th magnitude, lies 63" southeast.