[2] Bredichina is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.
[1] This minor planet was named after Fyodor Bredikhin (1831–1904), also known as Theodor or Feodor Alexandrovich Bredichin, a Russian astronomer and director of the Pulkovo Observatory.
[5] In March 2015, a rotational lightcurve of Bredichina was obtained from photometric observations by Spanish astronomers Alfonso Carreño (J08), Amadeo Aznar (Z95), Enrique Arce (J67), Pedro Brines (Z98), and Juan Lozano (I57).
[11] Previously, in August 2008, Argentine astronomer Ricardo Gil-Hutton derived period of 18.61±0.02 hours with an amplitude of 0.60±0.03 magnitude (U=2).
[14] Tentative measurements were also made by Italian Nicola Cornero and Federico Manzini at the Sozzago Astronomical Station (A12) in May 2010, which gave a period of 27.88 hours with an amplitude of 0.049 magnitude (U=2−).