Raymond Scott Hudson (born 1959) is a professor of electrical engineering and computer science at Washington State University. Hudson was educated at Caltech, where he received his bachelor's degree in engineering and applied science in 1985, his master's degree in electrical engineering in 1986, and his PhD in electrical engineering in 1990. His research interests include radar imaging, optical signal processing, and radar astronomy. [1]
From August 19 to 22 of 1989, Hudson and Steven Ostro observed 4769 Castalia from the Arecibo Observatory, producing the first direct image of an asteroid.
The main-belt asteroid 5723 Hudson, discovered by Edward Bowell at Lowell Observatory in 1986, was named in his honour. [1] The official naming citation was published on 9 September 1995 ( M.P.C. 25654). [2]
1620 Geographos, provisional designation 1951 RA, is a highly elongated, stony asteroid, near-Earth object and potentially hazardous asteroid of the Apollo group, with a mean-diameter of approximately 2.5 km (1.6 mi). It was discovered on 14 September 1951, by astronomers Albert George Wilson and Rudolph Minkowski at the Palomar Observatory in California, United States. The asteroid was named in honor of the National Geographic Society.
2063 Bacchus, provisional designation 1977 HB, is a stony asteroid and near-Earth object of the Apollo group, approximately 1 kilometer in diameter. The contact binary was discovered on 24 April 1977, by American astronomer Charles Kowal at the Palomar Observatory in California, United States. It was named after Bacchus from Roman mythology.
1566 Icarus is a large near-Earth object of the Apollo group and the lowest numbered potentially hazardous asteroid. It has an extremely eccentric orbit (0.83) and measures approximately 1.4 km (0.87 mi) in diameter. In 1968, it became the first asteroid ever observed by radar. Its orbit brings it closer to the Sun than Mercury and further out than the orbit of Mars, which also makes it a Mercury-, Venus-, and Mars-crossing asteroid. This stony asteroid and relatively fast rotator with a period of 2.27 hours was discovered on 27 June 1949, by German astronomer Walter Baade at the Palomar Observatory in California. It was named after the mythological Icarus.
4486 Mithra, is an eccentric asteroid and suspected contact-binary, classified as near-Earth object and potentially hazardous asteroid, approximately 2 kilometers in diameter. It belongs to the Apollo group of asteroids and is a relatively slow rotator.
69230 Hermes is a sub-kilometer sized asteroid and binary system on an eccentric orbit, classified as a potentially hazardous asteroid and near-Earth object of the Apollo group, that passed Earth at approximately twice the distance of the Moon on 30 October 1937. The asteroid was named after Hermes from Greek mythology. It is noted for having been the last remaining named lost asteroid, rediscovered in 2003. The S-type asteroid has a rotation period of 13.9 hours. Its synchronous companion was discovered in 2003. The primary and secondary are similar in size; they measure approximately 810 meters (2,700 ft) and 540 meters (1,800 ft) in diameter, respectively.
Carl Gustav Witt was a German astronomer and discoverer of two asteroids who worked at the Berlin Urania Observatory, a popular observatory of the Urania astronomical association of Berlin.
Tsutomu Seki is a Japanese amateur astronomer and discoverer of minor planets and comets, born in Kōchi, Japan.
Shigeru Inoda was a Japanese ophthalmologist, surgeon and amateur astronomer.
Makio Akiyama is a Japanese astronomer affiliated with the Susono Observatory (886). He is a discoverer of minor planets, credited by the Minor Planet Center with the discovery of 16 numbered minor planets during 1989–1999.
Vincenzo Silvano Casulli, usually known as Silvano Casulli was an Italian amateur astronomer and a discoverer of minor planets at his Vallemare di Borbona Observatory in Lazio.
Pierre Antonini is a retired French mathematics professor and amateur astronomer who has discovered several minor planets and two supernovae at his private Observatoire de Bédoin located at Bédoin, southeastern France. For many of his discoveries he used a 16-cm telescope or a 30-cm telescope.
Giuseppe Forti was an Italian astronomer and a discoverer of asteroids.
Antonio Vagnozzi is an amateur Italian astronomer and a discoverer of asteroids.
Masayuki Yanai is a Japanese astronomer. He is a prolific co-discoverer of minor planets. One of his co-discoveries is the dark, inner main-belt asteroid 3915 Fukushima. He retired from docent for astronomy at Sapporo Science Center.
Marco Cavagna was an Italian amateur astronomer.
The Santa Lucia Stroncone Astronomical Observatory is an astronomical observatory located at 350 metres (1,150 ft) altitude in Stroncone, near the city of Terni, in Umbria, north central Italy.
Giovanni de Sanctis is an Italian astronomer and discoverer of minor planets at the Osservatorio Astronomico di Torino in Turin, Italy. His name is sometimes spelt DeSanctis, particularly in the Minor Planet Circulars. The Minor Planet Center credits him with the discovery of 42 numbered minor planets, most of which he discovered at ESO's La Silla site in northern Chile in the early 1980s.
The Starkenburg Observatory is an astronomical observatory in Heppenheim, Germany. It was founded in 1970, and currently has about 150 members.
3752 Camillo is an inclined contact-binary asteroid, classified as near-Earth object of the Apollo group, approximately 2.3 kilometers in diameter. It was discovered on 15 August 1985, by astronomers Eleanor Helin and Maria Barucci using a 0.9-metre (35 in) telescope at the CERGA Observatory in Caussols, France. Lightcurve studies by Petr Pravec in 1998 suggest that the assumed S-type asteroid has an elongated shape and a longer-than average rotation period of 38 hours.
Paul Herget was an American astronomer and director of the Cincinnati Observatory, who established the Minor Planet Center after World War II.