163 Erigone

It was discovered by French astronomer Henri Joseph Perrotin on April 26, 1876, and named after one of the two Erigones in Greek mythology.

This asteroid is orbiting the Sun at a distance of 2.37 AU with a period of 3.643 years and an eccentricity (ovalness) of 0.19.

[3] Photometric measurements taken in 2014 were used to construct a lightcurve that demonstrated a rotation period of 16.136±0.001 h with an amplitude of 0.32±0.02 in magnitude.

[7] In the early morning hours of March 20, 2014, Erigone occulted the first-magnitude star Regulus,[8] as first predicted by Aldo Vitagliano in 2004 using the SOLEX software.

[8][10] However, thick clouds and rain blocked the view for most if not all people on the shadow path.

Path of occultation from New York to Ontario