Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 22 September 1919 |
Designations | |
(2623) Zech | |
Named after | Gert Zech (ARI astronomer) [2] |
A919 SA ·1963 RE | |
main-belt ·(inner) [3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 97.70 yr (35,684 days) |
Aphelion | 2.7846 AU |
Perihelion | 1.7243 AU |
2.2545 AU | |
Eccentricity | 0.2352 |
3.39 yr (1,236 days) | |
324.18° | |
0° 17m 28.32s / day | |
Inclination | 4.0548° |
349.11° | |
22.883° | |
Known satellites | 1 [3] [4] [5] |
Physical characteristics | |
Dimensions | 6.50 km (calculated) [3] 7.61 km (estimate) [5] |
2.7401±0.0002 h [4] | |
0.20 (assumed) [3] | |
S [3] [6] | |
13.13±0.59 [6] ·13.3 [1] [3] | |
2623 Zech, provisional designation A919 SA, is a stony binary [4] asteroid from the inner regions of the asteroid belt, approximately 6.5 kilometers in diameter. It was discovered on 22 September 1919, by German astronomer Karl Reinmuth at Heidelberg Observatory in southwest Germany. [7] It was named after German ARI astronomer Gert Zech. [2]
Zech is a stony S-type asteroid that orbits the Sun in the inner main-belt at a distance of 1.7–2.8 AU once every 3 years and 5 months (1,236 days). Its orbit has an eccentricity of 0.24 and an inclination of 4° with respect to the ecliptic. [1] The body's observation arc begins with its official discovery observation, as no precoveries were taken, and no prior identifications were made. [7] On 8 June 2002, Zech passed 0.036 AU (5,400,000 km) from the major asteroid 3 Juno. [1]
While "Johnston's Archive" estimates a diameter of 7.61 kilometers for Zech, [5] the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.5 kilometers based on an absolute magnitude of 13.3. [3] No observational results have been published by the space-based IRAS, Akari, and WISE/NEOWISE surveys. [1] [3]
In October 2004, a rotational lightcurve of Zech was obtained from photometric observations by American astronomer Donald P. Pray at Sugarloaf Mountain Observatory, Massachusetts, in a collaboration with other American and European astronomers from France, the Czech Republic, Serbia, Georgia and Ukraine. Lightcurve analysis gave a rotation period of 2.7401 hours with a brightness variation of 0.22 magnitude ( U=n.a. ). [4] While not being a fast rotator, it has a relatively fast spin rate for its size, as most minor planets rotate between 2.2 and 20 hours.
During Pray's photometric observations, it was revealed that Zech (primary) is in fact an asynchronous binary asteroid with a minor planet moon orbiting it. The moon has an orbital period of 117.2 hours and a spin rate of 18.718 hours with an amplitude 0.08 magnitude. [4] Based on Pray's secondary-to-primary mean diameter ratio (Ds/p) of more than 0.29, the Johnston's Archive estimates a diameter of at least 2.21 kilometers for Zech's companion. [5]
This minor planet was named after German astronomer Gert Zech (born 1941) at ARI in Heidelberg. He was editor of Astronomy and Astrophysics Abstracts and is known for his publications on the observational determination of the length of the astronomical unit and the mass of the Earth–Moon system using the dynamical method by observing the near-Earth object 433 Eros. Naming citation was prepared by Lutz D. Schmadel who also proposed the name. [2] The citation was published on 18 February 1992 ( M.P.C. 19692). [8]
1798 Watts, provisional designation 1949 GC, is a stony asteroid and binary system from the inner regions of the asteroid belt, approximately 7 kilometers in diameter.
1016 Anitra, provisional designation 1924 QG, is a stony Florian asteroid and suspected asynchronous binary system from the inner regions of the asteroid belt, approximately 10 kilometers in diameter.
2006 Polonskaya (provisional designation: 1973 SB3) is a stony Flora asteroid and asynchronous binary system from the inner regions of the asteroid belt, approximately 5 kilometers (3.1 miles) in diameter. It was discovered on 22 September 1973, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula, and later named after Ukrainian astronomer Elena Kazimirtchak-Polonskaïa. Its one-kilometer-sized satellite was discovered by an international collaboration of astronomers in November 2005.
1052 Belgica, provisional designation 1925 VD, is a binary Florian asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 15 November 1925, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium. It was the first minor planet discovered at Uccle Observatory, after which the minor planet 1276 Ucclia was named.
4029 Bridges, provisional designation 1982 KC1, is a stony asteroid and binary system from the middle regions of the asteroid belt, approximately 8 kilometers in diameter.
3034 Climenhaga is a stony Florian asteroid and synchronous binary asteroid from the inner regions of the asteroid belt, approximately 7.8 kilometers in diameter. The asteroid was discovered on 24 September 1917 by German astronomer Max Wolf at Heidelberg Observatory in southwest Germany and assigned provisional designation A917 SE. It was later named after Canadian astrophysicist John Climenhaga. Its minor-planet moon has a period of nearly 19 hours.
3905 Doppler, provisional designation 1984 QO, is a stony asteroid and binary system from the middle region of the asteroid belt, approximately 8 kilometers in diameter.
2754 Efimov, provisionally named 1966 PD, is a stony asteroid and binary system from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 13 August 1966, by Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named after Russian aviator Mikhail Efimov.
1453 Fennia, provisional designation 1938 ED1, is a stony Hungaria asteroid and synchronous binary system from the innermost regions of the asteroid belt, approximately 7 kilometers in diameter. Discovered by Yrjö Väisälä at the Turku Observatory in 1938, the asteroid was later named after the Nordic country of Finland. The system's minor-planet moon was discovered in 2007. It has a derived diameter of 1.95 kilometers and is orbiting its primary every 23.55 hours.
3073 Kursk, provisionally known as 1979 SW11, is a stony Florian asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 4.7 kilometers in diameter. It was discovered on 24 September 1979, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.
7958 Leakey, provisional designation 1994 LE3, is a Hungaria asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 3 kilometers in diameter.
1830 Pogson, provisional designation 1968 HA, is a stony Florian asteroid and an asynchronous binary system from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 17 April 1968, by Swiss astronomer Paul Wild at the Zimmerwald Observatory near Bern, Switzerland. The S-type asteroid has a rotation period 2.6 of hours. It was named for English astronomer Norman Pogson. The discovery of its 2.5-kilometer sized companion was announced in May 2007.
2691 Sersic, provisional designation 1974 KB, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered by staff members at the Felix Aguilar Observatory at El Leoncito Complex in Argentina, on 18 May 1974. The asteroid was named after Argentine astronomer José Sersic.
2121 Sevastopol, provisional designation 1971 ME, is a stony Florian asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 27 June 1971, by Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. Its minor-planet moon was discovered in 2010.
2815 Soma, provisional designation 1982 RL, is a binary Florian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 15 September 1982, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station in Flagstaff, Arizona, in the United States. It is named for the mechanical puzzle Soma cube.
4383 Suruga, provisional designation 1989 XP, is a Vestian asteroid and binary system from the inner regions of the asteroid belt, approximately 6.5 kilometers in diameter. It was discovered on 1 December 1989, by Japanese astronomer Yoshiaki Oshima at Gekko Observatory, Japan. The asteroid was named after the former Japanese Suruga Province. Its synchronous minor-planet moon, S/2013 (4383) 1, measures approximately 1.33 kilometers and has a period of 16.386 hours.
10208 Germanicus, provisional designation 1997 QN1, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter.
15268 Wendelinefroger, provisional designation 1990 WF3, is a stony, spheroidal, and binary Nysian asteroid from the inner regions of the asteroid belt, approximately 3.4 kilometers in diameter.
32008 Adriángalád, provisional designation: 2000 HM53, is a background asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 29 April 2000, by astronomers with the LINEAR program at Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. The V-type asteroid has a rotation period of 3.0 hours. It was named for Slovak astronomer Adrián Galád. Its 1.6-kilometer sized minor-planet moon was discovered in August 2007.
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