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In page 23436 Alekfursenko:
"In November 2010, a rotational lightcurve of Alekfursenko was obtained from photometric observations made by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 3.6277 hours with a brightness variation of 0.42 magnitude (U=2).[1] A modeled lightcurve using photometric data from the Lowell Photometric Database and from the Wide-field Infrared Survey Explorer (WISE) was published in 2018. It gave a concurring sidereal period of 3.627672 hours, as well as a spin axis at (−1.0°, 54.0°) in ecliptic coordinates (λ, β).[2]
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