The first binary star, for which the orbital path of its components was calculated, took place 60 years ago. It was achieved in 1828 by the French astronomer Felix Savary. It consists of golden components with a brightness of 4.3 mag and 4.8 mag, separated by 3 billion kilometers. Around 1970, they had a mutual separation of 3", and could easily be distinguished even with small telescopes. Then their mutual separation decreased, reaching its minimum in 1992 - 0.8". Today, this value is around 2", so a telescope with an 8 cm objective diameter is sufficient for their resolution.