4217 Engelhardt
4217 Engelhardt, provisional designation, is a stony Phocean asteroid and a potentially binary system from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 24 January 1988, by American astronomer Carolyn Shoemaker at Palomar Observatory in California, and later named after German mineralogist Wolf von Engelhardt.
Classification and orbit
Engelhardt is a stony S-type asteroid and a member of the Phocaea family. It orbits the Sun in the inner main-belt at a distance of 1.8–2.8 AU once every 3 years and 6 months. Its orbit has an eccentricity of 0.21 and an inclination of 23° with respect to the ecliptic.It was first identified as at Turku Observatory in 1944, extending the body's observation arc by 44 years prior to its official discovery observation at Palomar. It will pass about from Earth threatening asteroid in 2736.
Physical characteristics
Lightcurves
In November 2004, a rotational lightcurve of Engelhardt was obtained from photometric observations by American astronomer Brian Warner at this Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation period of 3.066 hours with a brightness amplitude of 0.16 magnitude.In December 2011, a follow-up observation by Warner gave a period of 3.0661 hours with 0.18 amplitude. Due to a couple of supposed occultation and eclipsing events, Warner also suspects that Engelhardt might by a binary system with a minor-planet moon orbiting it every 36.03 hours. The result, however, is far from conclusive.