Hamal (α Aries) - The brightest star of the constellation, otherwise unremarkable. This red giant of spectral class K2 has a magnitude of 2 and shines at a distance of 66 light years. Sometimes the star is also referred to as El Nath.

ε Arietis - Binary star, white components with nearly the same brightness (5.2 mag and 5.5 mag) at a separation of 1.5". We can sufficiently separate them with a magnification of 150x using a 200 mm telescope during good seeing.

Mesarthim (γ Arietis) - A charming double star, composed of blue-white components with magnitudes 4.7 and 4.8, separated by 7.8", which can be resolved with a 5 cm telescope. Mesarthim is visible to the naked eye as a star with magnitude 3.9. Historically, it is interesting because it was one of the first double stars discovered by a telescope, observed by the English naturalist Robert Hooke in 1664 while observing a comet. It is located 204 light-years away.

λ Arietis - Double star easily distinguishable in a 10 cm telescope. The yellow-white star (4.9 mag) is located 37.4" away from the pale blue component (7.7 mag).

Musca Borealis (Severná mucha) - The now non-existent constellations, which once consisted of three stars of the constellation Aries - 35, 39, 41 Arietis, representing buzzing sea flies settling on the ram's tail.