In the latest issue of Minor Planet Bulletin (VOLUME 48, NUMBER 2, A.D. 2021 APRIL-JUNE), our work on determining the rotation period of asteroid 2020 UQ6 was published. This asteroid is a Near-Earth object belonging to the Apollo group discovered at Tokyo-Kiso Observatory (MPC code 381) on 2020 October 27.
You can read here our paper titled "ROTATIONAL PERIOD AND LIGHTCURVE DETERMINATION OF 2020 UQ6: A SUPER FAST ROTATOR"
CCD photometric observation of 2020 UQ6 were carried out in 2×2 binned format during the night between 2020 October 28 and 29 by using the main telescope of the Osservatorio Salvatore di Giacomo, Agerola (MPC code L07). It is a 0.50-m Ritchey-Chretien operating at f/8 equipped with an unfiltered FLI-PL4240 CCD camera (2048×2048array of 13.5-micron pixels).
The software Tycho by D. Parrott,
that now offers the ability to construct lightcurves and determine
rotation periods, was used during the observing session to extract the
light curve of this interesting asteroid almost in real time.
In order to take in account both the high speed of the object (ranging from 21.48 arcec/min to 17.46 arcsec/min during the measurements) exposure times were kept to 4 s for all sessions. Eight observation sessions collected 1373 data points for lightcurve analysis. This led to a bimodal lightcurve with a period of 0.04521 h (162.76 s), or a frequency of 530.84 rev/d, and an amplitude of 0.57 magnitudes. This finding identifies this object as a super-fast rotator asteroid (P << 2 h).
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Credit: Guido et al.; MPB |
From the absolute magnitude value of H = 22.6 and assuming the asteroid to be a spherical object with a uniform surface and albedo ranging from 0.05 and 0.30, one can gets an estimated diameter ranging from 80 and 180 m. From this, it is possible to add the average value of the estimated diameter, D = 130 m, to the frequency vs diameter plot from LCDB. As it can be observed, 2020 UQ6 is located in an uncrowded region of the graph (identified by a yellow point), making this object particularly noteworthy. (click on the image below for a bigger version)
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Credit: Guido et al.; MPB
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by Ernesto Guido, Antonio Catapano, Alfonso Noschese, Antonio Vecchione