Hermes was discovered by German astronomer Karl Reinmuth in images taken at Heidelberg Observatory on 28 October 1937. Only four days of observations could be made before it became too faint to be seen in the telescopes of the day. This was not enough to calculate an orbit, and Hermes became a lost asteroid. It thus did not receive a number, but Reinmuth nevertheless named it after the Greek god Hermes. It was the third unnumbered but named asteroid, having only the provisional designation. The two others long lost were Apollo, discovered in 1932 and numbered 1973, and Adonis, discovered in 1936 and numbered 1977. On 15 October 2003, Brian A. Skiff of the LONEOS project made an asteroid observation that, when the orbit was calculated backwards in time, turned out to be a rediscovery of Hermes. It has been assigned sequential number 69230. Additional precovery observations were published by the Minor Planet Center, the earliest being found by an amateur astronomer on images taken serendipitously by the on 16 September 2000.
Naming
This minor planet was named after the Greek god Hermes, who is the messenger of the gods and son of Zeus and Maia . Recovered and numbered in autumn 2003, Hermes was originally named by the Astronomical Calculation Institute as early as 1937. The official naming citation was published by the Minor Planet Center on 9 November 2003.
Orbit and classification
Hermes is an Apollo asteroid, a subgroup of near-Earth asteroids that cross the orbit of Earth. It orbits the Sun at a distance of 0.6–2.7 AU once every 2 years and 2 months. Its orbit has an eccentricity of 0.62 and an inclination of 6° with respect to the ecliptic. Due to its eccentricity, Hermes is also a Mars- and Venus-crosser. Frequent close approaches to both Earth and Venus make it unusually challenging to forecast its orbit more than a century in advance, though there is no known impact risk within that timeframe.
Close approaches
The asteroid has an Earth minimum orbital intersection distance of which translates into 1.6 LD. On 30 October 1937, Hermes passed from Earth, and on 26 April 1942, from Earth. In retrospect it turned out that Hermes came even closer to the Earth in 1942 than in 1937, within 1.7 lunar distances; the second pass was unobserved at the height of the Second World War. For decades, Hermes was known to have made the closest known approach of an asteroid to the Earth. Not until 1989 was a closer approach observed. At closest approach, Hermes was moving 5° per hour across the sky and reached 8th magnitude.
Three rotational lightcurves of Hermes were obtained from photometric observations in October 2003. Lightcurve analysis gave a well-defined rotation period between 13.892 and 13.894 hours with a brightness variation between and 0.06 and 0.08 magnitude, which indicates that the body has a nearly spherical shape.
Satellite
Radar observations led by Jean-Luc Margot at Arecibo Observatory and Goldstone in October and November 2003 showed Hermes to be a binary asteroid. The primary and secondary components have nearly identical radii of and, respectively, and their orbital separation is only 1,200 metres, much smaller than the Hill radius of 35 km. The two components are in double synchronous rotation. Hermes is one of only four systems of that kind known in the near-Earth object population. The other three are,, and.
