β Cam - The brightest star of the constellation has an apparent magnitude of 4.22. This yellow supergiant of spectral class G0 is located 870 light-years away and shines 1,600 times brighter than our Sun. The surface temperature reaches 30,000 Kelvin.

α Cam - In the sky, it appears as a 4.3 magnitude star. However, in reality, this blue supergiant of spectral class O is 620,000 times brighter than the Sun. It is located approximately 6,000 thousand light-years away from us.

VZ Cam - A semi-regular variable star of type M, when observed through a telescope, appears noticeably red. It exhibits small, irregular changes in magnitude, ranging from 4.8mag to 5.2mag with an average period of about 24 days. Due to its proximity to the celestial pole, it can be observed throughout the year from more northern latitudes.

29 Cam - A binary star suitable for a 100mm telescope. That it is a binary star is evident at 100x magnification. It appears as an unequal (6.5mag, 9.5mag) and contrasting pair of yellow and pale blue components. Their mutual distance is 25.1".

Z Cam - A cataclysmic variable star, which jumps every two to three weeks from a minimum around 13mag to a maximum with a magnitude of 9.6mag. However, its similarity to other variable stars of this type ends there. Its magnitude can actually stop decreasing and remain at a medium brightness level for a very long time. It stays like this for several months before its magnitude starts increasing again - the star is therefore weakening.