Discovery [1] | |
---|---|
Discovered by | Farra d'Isonzo Obs. |
Discovery site | Farra d'Isonzo Obs. |
Discovery date | 23 November 1995 |
Designations | |
(7675) Gorizia | |
Named after | Gorizia (Italian town) [2] |
1995 WT5 ·1976 UT19 1993 FD52 | |
main-belt ·(inner) background | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 39.64 yr (14,479 days) |
Aphelion | 2.6402 AU |
Perihelion | 2.1896 AU |
2.4149 AU | |
Eccentricity | 0.0933 |
3.75 yr (1,371 days) | |
206.26° | |
0° 15m 45.36s / day | |
Inclination | 4.7499° |
28.333° | |
127.73° | |
Physical characteristics | |
Dimensions | 3 km (est. at 0.22) [3] |
14.4 [1] | |
7675 Gorizia, provisional designation 1995 WT5, is a background asteroid from the inner regions of the asteroid belt, approximately 3 kilometers in diameter. It was discovered on 23 November 1995, by the staff at Farra d'Isonzo Observatory in northeastern Italy. [4] It is named for the Italian town of Gorizia. [2]
Gorizia orbits the Sun in the inner main-belt at a distance of 2.2–2.6 AU once every 3 years and 9 months (1,371 days). Its orbit has an eccentricity of 0.09 and an inclination of 5° with respect to the ecliptic. [1] In 1976, it was first identified as 1976 UT19 at the Japanese Kiso Observatory, extending the body's observation arc by 19 years prior to its official discovery observation. [4]
As of 2017, Gorizia's effective size and composition, as well as its rotation period and shape remain unknown. [5] No estimates about Gorizia's diameter and albedo have been published by any of the space-based surveys such as the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, or NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission. It has an absolute magnitude of 14.4. [1]
Based on a generic magnitude-to-diameter conversion, Gorizia measures between 3 and 7 kilometers for an albedo in the range of 0.05 to 0.25. [3] Since asteroids in the inner main-belt are often of a silicaceous rather than of a carbonaceous composition, with higher albedos, typically around 0.20, Gorizia's diameter might be on the lower end of NASA's published conversion table, as the higher the body's reflectivity (albedo), the smaller its diameter, for a given absolute magnitude (brightness). [3]
This minor planet was named for the northeastern Italian town of Gorizia, on the occasion of the 1000th anniversary celebrating its first documented mentioning. The discovering observatory, after which the asteroid 7501 Farra was named, is located not far from Gorizia. [2] The official naming citation was published by the Minor Planet Center on 2 February 1999 ( M.P.C. 33789). [6]
15017 Cuppy, provisional designation 1998 SS25, is a Florian asteroid from the inner regions of the asteroid belt, approximately 2 kilometers in diameter. It was discovered on 22 September 1998, by the Lowell Observatory Near-Earth-Object Search (LONEOS) at its Anderson Mesa Station, Arizona, United States. The asteroid was named for American humorist Will Cuppy.
19367 Pink Floyd, provisional designation 1997 XW3, is a dark background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 3 December 1997, by European astronomers of the ODAS survey at the CERGA Observatory near Caussols, France. The asteroid was named after the English rock band Pink Floyd.
100268 Rosenthal, provisional designation 1994 TL16, is a background asteroid from the inner region of the asteroid belt, approximately 3 kilometers (2 miles) in diameter. It was discovered on 5 October 1994, by German astronomer Freimut Börngen at the Karl Schwarzschild Observatory in Tautenburg, eastern Germany. The asteroid was later named for German radio and TV host Hans Rosenthal.
1997 Leverrier is a stony Flora asteroid from the inner regions of the asteroid belt. It was discovered on 14 September 1963, by the Indiana Asteroid Program at Goethe Link Observatory near Brooklyn, Indiana, United States, and named after French mathematician Urbain Le Verrier. The asteroid has a rotation period of 6.8 hours and measures approximately 7 kilometers in diameter
8549 Alcide, provisional designation 1994 FS, is a stony Nysa asteroid from the inner regions of the asteroid belt, approximately 4.2 kilometers in diameter. It was discovered on 30 March 1994, by a group of amateur astronomers at the Farra d'Isonzo Observatory, Italy, near the border to Slovenia. It was named for Alcide Bittesini, father of co-discoverer Luciano Bittesini.
1905 Ambartsumian, provisional designation 1972 JZ, is an asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 14 May 1972, by Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory, Nauchnyj, on the Crimean peninsula. The asteroid was named after theoretical astrophysicist Victor Ambartsumian.
2839 Annette is a bright Flora asteroid from the inner regions of the asteroid belt. It was discovered on 5 October 1929, by American astronomer Clyde Tombaugh at Lowell Observatory during his search for Pluto. The presumed S-type asteroid has a rotation period of 10.5 hours and measures approximately 5 kilometers in diameter. It was named after the discoverer's daughter.
2033 Basilea, provisional designation 1973 CA, is a stony asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 6 February 1973, by astronomer Paul Wild at the Zimmerwald Observatory near Bern, Switzerland. The asteroid was named for the Swiss city of Basel.
151997 Bauhinia, provisional designation 2004 JL1, is a sub-kilometer background asteroid from the inner regions of the asteroid belt, approximately 900 meters in diameter. It was discovered on 11 May 2004, by Canadian astronomer William Yeung at the Desert Eagle Observatory, Arizona, United States. It was named after the flowering plant Bauhinia blakeana also known as the "Hong Kong Orchid Tree".
1818 Brahms, provisional designation 1939 PE, is an asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 15 August 1939, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. The asteroid was named after composer Johannes Brahms.
6141 Durda, provisional designation 1992 YC3 is a stony Hungaria asteroid, classified as slow rotator and Mars-crosser from the innermost region of the asteroid belt, approximately 3.2 kilometers in diameter. It was discovered on 26 December 1992, by Spacewatch at Kitt Peak National Observatory in Arizona, United States.
27270 Guidotti, provisional designation 2000 AY4, is a carbonaceous background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 2 January 2000, by Italian astronomers Luciano Tesi and Alfredo Caronia at the Pistoia Mountains Astronomical Observatory in San Marcello Pistoiese, Italy. The asteroid was named after amateur astronomer Guido Guidotti.
3040 Kozai, provisional designation 1979 BA, is a stony asteroid and Mars-crosser on a tilted orbit from the innermost regions of the asteroid belt, approximately 4 kilometers in diameters.
7387 Malbil (prov. designation: 1982 BS1) is an elongated background asteroid from the inner regions of the asteroid belt. It was discovered on 30 January 1982, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Arizona, United States. The asteroid has a rotation period of 7.5 hours and measures approximately 6 kilometers (4 miles) in diameter. It is named for American pianist Malcolm Bilson.
1990 Pilcher, provisional designation 1956 EE, is a stony background asteroid from the Florian region of the inner asteroid belt, approximately 7 kilometers in diameter. It was discovered on 9 March 1956, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in Heidelberg, Germany. In 1982, it was named by the MPC for American physicist and photometrist Frederick Pilcher. The S-type asteroid has a short rotation period of 2.8 hours.
1530 Rantaseppä, provisional designation 1938 SG, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. Discovered by Yrjö Väisälä at Turku Observatory in 1938, it was later named after Finnish astronomer Hilkka Rantaseppä-Helenius.
1779 Paraná, provisional designation 1950 LZ, is an asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter.
37432 Piszkéstető, provisional designation 2002 AE11, is an Erigonian asteroid from the inner regions of the asteroid belt, approximately 4.6 kilometers (2.9 miles) in diameter. It was discovered on 11 January 2002, by the Hungarian astronomers Krisztián Sárneczky and Zsuzsanna Heiner at the Konkoly Observatory's Piszkéstető Station northeast of Budapest, Hungary. The asteroid was later named for the discovering observatory.
116903 Jeromeapt – provisional designation 2004 GW – is an asteroid of the Massalia family from the inner regions of the asteroid belt, approximately 1.1 kilometers in diameter. It was discovered on 11 April 2004, by American astronomer Jim Young at the Table Mountain Observatory near Wrightwood, California, in the United States. The asteroid was named for American astronaut Jerome Apt.
185638 Erwinschwab, provisional designation 2008 EU7, is a potentially sub-kilometer Nysian asteroid from the inner regions of the asteroid belt. It was discovered on 1 March 2008, by OAM-astronomers at the La Sagra Observatory in southern Spain. The asteroid is estimated to measure between 950 meters and 1.8 kilometers in diameter and was named after German astronomer Erwin Schwab in 2009.