Discovered by C. Kowal Alternative names 1976 UA Discovered 22 October 1976 Discoverer Charles T. Kowal | Discovery date 22 October 1976 Pronunciation ˈhæθ ɔr, -ər (HATH-er) Minor planet category Aten · NEO · PHA Orbits Sun | |
Similar 3362 Khufu, Sun, 5381 Sekhmet, 2101 Adonis, 2201 Oljato | ||
2340 Hathor (HATH-awr; HATH-er), provisional designation 1976 UA, is an eccentric stony asteroid, classified as near-Earth object and potentially hazardous asteroid. It belongs to the Aten group of asteroids and measures approximately 210 meters in diameter. It was discovered on 22 October 1976, by American astronomer Charles Kowal at Palomar Observatory, California, United States. It was independently discovered by Eleanor Helin and is named for the ancient Egyptian deity Hathor.
Description
Being a member of the Aten asteroids, Hathor orbits the Sun at a distance of 0.5–1.2 AU once every 9 months (283 days). Its orbit has an eccentricity of 0.45 and an inclination of 6° with respect to the ecliptic. Its observation arc begins 3 days after its official discovery at Palomar, with no precoveries taken and no prior identifications made. Its orbital solution includes non-gravitational forces.
When it was discovered in 1976, Hathor had one of its closest approaches to Earth at 0.007752 AU (1,160,000 km). On 21 October 2014, when it passed Earth at 0.048 AU, or 18.8 lunar distances, it was observed 22 times by the Goldstone Deep Space Network using radar astronomy over a period of 21 days from 10 to 31 October. Hathor will pass Earth again at 0.00658 AU (984,000 km) on 21 October 2069.
On 25 October 1976, Hathor was independently discovered by Eleanor Helin during the Palomar Planet-Crossing Asteroid Survey (PCAS), and by William Lawrence Sebok, who photographed the same field almost simultaneously using Palomars 1.22-meter Schmidt telescope. On the same day, the official discoverer Charles Kowal found that Hathor had already been imaged three days earlier by Palomars 0.46-meter telescope (the same instrument used by PCAS). A forth independent discovery was made several days later by Nikolai Chernykh at CrAO on the Crimean peninsula. The multiple discoveries were probably due to its very close approach distance to Earth. After 2062 Aten, Hathor was the second discovery of an Aten asteroid. In 1978, the third Aten, 2100 Ra-Shalom was discovered. The Aten 1954 XA was already identified at Palomar in 1954, but its discovery date was later assigned to a 2003-observation at Lincoln Laboratory ETS, and is now known as (363505) 2003 UC20.
In the Tholen and SMASS taxonomy, Hathor has a CSU and Sq spectral type, respectively. In the 1990s, Dutch–American astronomer Tom Gehrels estimated Hathor's diameter to measure approximately 300 meters, assuming an albedo of 0.15. During its close approach to Earth in October 2014, a team of astronomer published a revised estimate of 7002210000000000000♠210±30 meters for its diameter. The Collaborative Asteroid Lightcurve Link adopts this diameter and derives an albedo of 0.3331 using an absolute magnitude of 20.2.
In November 2014, American astronomer Brian D. Warner obtained a rotational light-curve of Hathor from photometric observations taken at the Palmer Divide Station in Colorado (also see § External links). Light-curve analysis gave a well-defined rotation period of 3.350 hours with a brightness variation of 0.11 magnitude (U=3).
In accordance with the custom to name all members of the Aten group after Ancient Egyptian deities, this minor planet is named for Hathor, sky-goddess and daughter of Ra, who personified the principles of joy, feminine love, and motherhood. The Ancient Greeks sometimes identified Hathor with the goddess Aphrodite. Naming was proposed by Eleanor Helin who also participated in the 1981-recovery. The minor planet 161 Athor is also named for Hathor. Naming citation was published on 1 June 1981 (M.P.C. 6060).