THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 45, NUMBER 3, A.D. 2018 JULY-SEPTEMBER 215. LIGHTCURVE ANALYSIS FOR TWO NEAR-EARTH 320ʺ/min during the close approach. The eclipse was observed, ASTEROIDS ECLIPSED BY EARTH’S SHADOW within minutes of the original prediction. Preliminary rotational and eclipse lightcurves were made available soon after the close Peter Birtwhistle approach (Birtwhistle, 2012; Birtwhistle, 2013; Miles, 2013) but it Great Shefford Observatory should be noted that a possible low amplitude 8.7 h period (Miles, Phlox Cottage, Wantage Road 2013) has been discounted in this analysis. Great Shefford, Berkshire, RG17 7DA United Kingdom Several other near-Earth asteroids are known to have been
[email protected] eclipsed by the Earth’s shadow, e.g. 2008 TC3 and 2014 AA (both before impacting Earth), 2012 KT42, and 2016 VA (this paper) (Received 2018 March18) but internet searches have not found any eclipse lightcurves. The asteroid lightcurve database (LCDB; Warner et al., 2009) lists a Photometry was obtained from Great Shefford reference to an unpublished result for 2012 XE54 by Pollock Observatory of near-Earth asteroids 2012 XE54 in 2012 (2013) without lightcurve details, but these have been provided on and 2016 VA in 2016 during close approaches. A request and give the rotation period as 0.02780 ± 0.00002 h, superfast rotation period has been determined for 2012 amplitude 0.33 mag derived from 101 points over a period of 30 XE54 and H-G magnitude system coefficients have been minutes for epoch 2012 Dec 10.2 UT at phase angle 19.5°, estimated for 2016 VA.