Long-lasting activity of asteroid (248370) 2005 QN<SUB>173</SUB>
We present the results of observations of asteroid (248370) QN 173 obtained during July 2021-January 2022 with three telescopes. Our analysis revealed the presence of the dust tail for about half of a year. The direct images of the asteroid were obtained with broad-band filters. No emissions were revealed in the spectra, and the spectrum of the
Ivanova, Oleksandra et al.
Fecha de publicación:
10
2023