INVESTIGATION OF NEO ASTEROIDS 2006 VB14 AND 1986 DA

I. Eglitis

doi:10.18524/1810-4215.2019.32.181826

INVESTIGATION OF NEO ASTEROIDS 2006 VB14 AND 1986 DA

Автор(и)

I. Eglitis Institute of Astronomy, University of Latvia, Latvia

DOI:

https://doi.org/10.18524/1810-4215.2019.32.181826

Ключові слова:

NEO, asteroids, rotation periods

Анотація

566 positions and photometric observa-
tions of NEO objects 2006 VB14 = Y5705 = 345705 and
1986 DA were obtained with Baldone Schmidt telescope
in 2018 and 2019, to detecting rotation period and other
physical characteristics. A Fourier transform was applied
to determine the rotation period for asteroid 1986
DA=6178. Value 3.12 ± 0.02h was obtained. Observations
confirm the previously obtained rotation period P = 3.25h
for 2006 VB14.