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

INVESTIGATION OF NEO ASTEROIDS 2006 VB14 AND 1986 DA

I. Eglitis

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.


Ключові слова


NEO;asteroids; rotation periods

Повний текст:

PDF (English)

Посилання


Brown P.G. et al.: 2013, Nature, http://dx.doi.org/10.1038/nature12741.

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Milani A. et al.: 2012, Minor Planet Bull., http://belissima.aob.rs/Conf2012/Milani_2012.pdf

Skiff B.A. et al.: 2012, Minor Planet Bull., 39, 111.

Warner, B.D.: 2011, MPO Canopus software v10.2.1.0,

http://www.minorplanetobserver.com/




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