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Les vitesses spatiales de 1273 étoiles autour du Soleil fournissent d'abord le mouvement solaire par rapport a ce groupe. Successivement un groupe mineur représentatif de 274 étoiles est choisi et par l'examen des vitesses spatiales residues (c'est-à-dire corrigées par le mouvement solaire) on trouve qu'il y a une remarquable tendance vers le centre galactique. L'ensemble des binaires visuelles qui se trouvent entre le même groupe autour du Soleil montre la même caractéristique.
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