we present a shape and spin axis model for main-belt asteroid 374 Burgundia. The model was achieved with the lightcurve inverson process, using combined dense photometric data acquired from four apparitions beetween 2000-2021 and sparse data from USNO Flagstaff. Analysis of the resulting data found a sidereal period P = 6.96397 ± 0.00002 hours and two mirrored pole solutions at (lambda = 9°, beta = 38°) and (lambda = 178°, beta = 28°) with an uncertainty of ± 10 degrees.
Spin-Shape Model for 374 Burgundia
Aceti, P.;
2021-01-01
Abstract
we present a shape and spin axis model for main-belt asteroid 374 Burgundia. The model was achieved with the lightcurve inverson process, using combined dense photometric data acquired from four apparitions beetween 2000-2021 and sparse data from USNO Flagstaff. Analysis of the resulting data found a sidereal period P = 6.96397 ± 0.00002 hours and two mirrored pole solutions at (lambda = 9°, beta = 38°) and (lambda = 178°, beta = 28°) with an uncertainty of ± 10 degrees.File in questo prodotto:
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