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Updated: Dec 20, 2025

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
LIGHTCURVE ANALYSIS OF THE NEAR-EARTH ASTEROID 2015 CN13
1Center for Solar System Studies-Palmer Divide Station, 446 Sycamore Ave., Eaton, CO 80615 USA.
Abstract:
The near-Earth asteroid 2015 CN13 made a fly-by of Earth in late 2015 February. We observed the asteroid on Feb 25, 26, and 28. Analysis of the data set found two possible periods, the most likely being P = 22.7 ± 0.3 h. Given the estimated diameter of 70 meters and long period, this puts 2015 CN13 in a small group of NEAs with D ≤ 140 meters and periods well below the spin barrier, i.e., approximately P ≥ 2.2 hours.
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