Discovery [1] | |
---|---|
Discovered by | H. van Gent |
Discovery site | Johannesburg Obs. (Leiden Southern Station) |
Discovery date | 29 September 1934 |
Designations | |
(1694) Kaiser | |
Named after | Frederik Kaiser (astronomer) [2] |
1934 SB ·1960 SD | |
main-belt ·(inner) [3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 82.60 yr (30,168 days) |
Aphelion | 3.0137 AU |
Perihelion | 1.7759 AU |
2.3948 AU | |
Eccentricity | 0.2584 |
3.71 yr (1,354 days) | |
125.25° | |
0° 15m 57.24s / day | |
Inclination | 11.103° |
13.421° | |
356.15° | |
Physical characteristics | |
Dimensions | 13.84±1.27 km [4] 15.678±0.175 km [5] [6] 28.42 km (calculated) [3] |
9 h [lower-alpha 1] 13.02±0.01 h [7] 13.23±0.02 h [8] | |
0.057 (assumed) [3] 0.1659±0.0088 [5] 0.166±0.009 [6] 0.241±0.046 [4] | |
B–V = 0.735 [1] U–B = 0.415 [1] Tholen = GC [1] · C [3] | |
11.46 [1] [3] [4] [5] | |
1694 Kaiser (prov. designation: 1934 SB) is a carbonaceous background asteroid from the inner regions of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 29 September 1934, by Dutch astronomer Hendrik van Gent at Leiden Southern Station, annex to the Johannesburg Observatory in South Africa. [9] It is named for Dutch astronomer Frederik Kaiser. [2]
Kaiser is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the inner main-belt at a distance of 1.8–3.0 AU once every 3 years and 9 months (1,354 days). Its orbit has an eccentricity of 0.26 and an inclination of 11° with respect to the ecliptic.of 1.8–3.0 AU once every 3.71 years (1,354 days). Its eccentric orbit of 0.26 is inclined by 11 degrees towards the plane of the ecliptic. [1] Kaiser's observation arc begins with its official discovery observation, as no precoveries were taken, and no prior identifications were made. [9]
This asteroid was named in honor of Dutch astronomer Frederik Kaiser (1808–1872), the director of the Leiden Observatory from 1837 to 1872. He founded the new Leiden Observatory and stimulated Dutch astronomical research. Frederick Kaiser is also honored by the lunar and Martian craters Kaiser. [2] Originally, the asteroid was erroneously named Kapteyn (MPC 2822), and only later it was noticed that the Duch astronomer Jacobus Kapteyn was already honored by the minor planet 818 Kapteynia. The official naming citation was published by the Minor Planet Center on 15 July 1968 ( M.P.C. 2883). [10]
On the Tholen taxonomy, the carbonaceous C-type asteroid is classified as a rare GC-type, an intermediate to the G-type asteroids. [1]
According to the survey the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Kaiser measures 13.84 and 15.68 kilometers in diameter, and its surface has an albedo of 0.241 and 0.166, respectively. [4] [5] [6] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 28.42 kilometers, with an absolute magnitude of 11.46 [3]
Two rotational lightcurves for Kaiser were obtained from photometric observations by American astronomer Brian D. Warner at his Palmer Divide Observatory in Colorado (see video in § External links). The lightcurves from January 2006 and November 2012, gave a rotation period of 13.02 and 13.23 hours and a variation in brightness of 0.32 and 0.13 magnitude, respectively ( U=3/2+ ). [7] [8]
1373 Cincinnati, provisional designation 1935 QN, is an asteroid in a comet-like orbit from the Cybele region, located at the outermost rim of the asteroid belt, approximately 20 kilometers in diameter. It was the only asteroid discovery made by famous American astronomer Edwin Hubble, while observing distant galaxies at Mount Wilson Observatory in California on 30 August 1935. The rather spherical X-type asteroid has a rotation period of 5.3 hours. It was named for the Cincinnati Observatory.
2069 Hubble, provisional designation 1955 FT, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 40 kilometers in diameter. It was discovered on 29 March 1955, by the Indiana Asteroid Program at Goethe Link Observatory, United States, and named after American astronomer Edwin Hubble.
1952 Hesburgh, provisional designation 1951 JC, is a rare-type carbonaceous asteroid from the outer regions of the asteroid belt, approximately 37 kilometers in diameter.
2023 Asaph, provisional designation 1952 SA, is a dark asteroid from the outer regions of the asteroid belt, approximately 21 kilometers in diameter. It was discovered on 16 September 1952, by astronomers of the Indiana Asteroid Program at Goethe Link Observatory in Indiana, United States.
2065 Spicer, provisional designation 1959 RN, is a dark and eccentric asteroid from the middle region of the asteroid belt, approximately 17 kilometers in diameter.
1042 Amazone, provisional designation 1925 HA, is a dark asteroid and slow rotator in the outer asteroid belt, approximately 70 kilometers in diameter. It was discovered on 22 April 1925, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. It is named after the Amazons from Greek mythology.
9936 Al-Biruni, provisional designation 1986 PN4, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 24 kilometers in diameter. It was discovered on 8 August 1986, by Belgian and Bulgarian astronomers Eric Elst and Violeta Ivanova at the Rozhen Observatory, located in Bulgaria's Smolyan province near the border to Greece. It was named for Persian medieval scholar Al-Biruni.
3037 Alku, provisional designation 1944 BA, is a carbonaceous asteroid from the central region of the asteroid belt, approximately 20 kilometers in diameter. It was discovered on 17 January 1944, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland.
3642 Frieden, provisional designation 1953 XL1, is a carbonaceous asteroid from the middle region of the asteroid belt, approximately 35 kilometers in diameter. It was discovered by German astronomer Herta Gessner at Sonneberg Observatory on 4 December 1953. It is named after the goddess of peace, Pax.
3915 Fukushima, provisional designation 1988 PA1, is a carbonaceous asteroid from the inner regions of the asteroid belt, approximately 21 kilometers in diameter.
9298 Geake, provisional designation 1985 JM, is a Mitidika asteroid from the central regions of the asteroid belt, approximately 12 kilometers in diameter. It was discovered on 15 May 1985, by American astronomer Edward Bowell at Lowell Observatory's Anderson Mesa Station near Flagstaff, Arizona, United States. The asteroid was named for British astronomer John E. Geake.
4265 Kani is a dark background asteroid from the inner regions of the asteroid belt. It was discovered by Japanese astronomers Yoshikane Mizuno and Toshimasa Furuta at Kani Observatory on 8 October 1989. The carbonaceous C-type asteroid has a rotation period of 5.7 hours and measures approximately 14 kilometers in diameter. It was named for the Japanese city of Kani.
1987 Kaplan, provisional designation 1952 RH, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 11 September 1952, by Soviet astronomer Pelageya Shajn at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after Soviet astrophysicist Samuil Kaplan.
6255 Kuma, provisional designation 1994 XT, is a carbonaceous asteroid from the central region of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 5 December 1994, by Japanese astronomer Akimasa Nakamura at Kuma Kogen Astronomical Observatory on the Island of Shikoku, Japan. It was named after the Japanese town of Kumakōgen.
1582 Martir, provisional designation 1950 LY, is a carbonaceous background asteroid from the outer regions of the asteroid belt, approximately 37 kilometers in diameter. It was discovered on 15 June 1950, by Argentine astronomer Miguel Itzigsohn at the La Plata Astronomical Observatory in Argentina. The asteroid was named after the First Lady of Argentina, Eva Perón.
3066 McFadden, provisional designation 1984 EO, is a stony background asteroid from the central regions of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 1 March 1984, by American astronomer Edward Bowell at the Anderson Mesa Station near Tucson, Arizona. It was named for American planetary scientist Lucy-Ann McFadden. The assumed S-type asteroid has a rotation period of 13.8 hours.
For other uses, see Steel (disambiguation).
1989 Tatry, provisional designation 1955 FG, is a carbonaceous Vestian asteroid and tumbling slow rotator from the inner regions of the asteroid belt, approximately 16 kilometers in diameter.
3823 Yorii, provisional designation 1988 EC1, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 11 kilometers in diameter.
1546 Izsák, provisional designation 1941 SG1, is a background asteroid from the outer regions of the asteroid belt, approximately 27 kilometers in diameter. It was discovered on 28 September 1941, by Hungarian astronomer György Kulin at the Konkoly Observatory near Budapest, Hungary. The asteroid was named after Hungarian astronomer Imre Izsák.