Discovery [1] | |
---|---|
Discovered by | P. Jensen |
Discovery site | Brorfelde Obs. |
Discovery date | 25 September 1987 |
Designations | |
(5171) Augustesen | |
Named after | Karl Augustesen [1] (Danish astronomer) |
1987 SQ3 ·1953 RP 1953 RP1 ·1989 CH8 | |
main-belt ·(inner) background [2] · Vestian [3] | |
Orbital characteristics [4] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 64.15 yr (23,430 d) |
Aphelion | 2.7460 AU |
Perihelion | 2.1036 AU |
2.4248 AU | |
Eccentricity | 0.1325 |
3.78 yr (1,379 d) | |
14.269° | |
0° 15m 39.6s / day | |
Inclination | 7.0844° |
322.10° | |
45.866° | |
Physical characteristics | |
6.445±0.074 km [5] 6.81 km (calculated) [3] 9.02±2.21 km [6] 9.41±0.33 km [7] 9.73±2.59 km [8] | |
19.2±0.1 h (poor) [9] 480±10 h [10] [lower-alpha 1] | |
0.08±0.05 [6] 0.10±0.06 [8] 0.108±0.008 [7] 0.20 (assumed) [3] 0.245±0.034 [5] | |
X [11] · S [3] | |
13.10 [5] [8] ·13.20 [3] [7] 13.3 [4] ·13.52 [6] 13.75±0.50 [11] | |
5171 Augustesen, provisional designation 1987 SQ3, is a background asteroid and slow rotator from the inner regions of the asteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 25 September 1987, by Danish astronomer Poul Jensen at the Brorfelde Observatory in Denmark. [1] The suspected tumbler and presumed Vestian asteroid has an exceptionally slow rotation period of 480 hours and possibly an elongated shape. [3] It was named after Danish astronomer Karl Augustesen. [1]
Augustesen is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. [2] Based on osculating Keplerian orbital elements, the asteroid has also been classified as a member of the Vesta family ( 401 ), one of the main belt's largest asteroid families named after 4 Vesta, the family's parent body. [3]
It orbits the Sun in the inner main-belt at a distance of 2.1–2.7 AU once every 3 years and 9 months (1,379 days; semi-major axis of 2.42 AU). Its orbit has an eccentricity of 0.13 and an inclination of 7° with respect to the ecliptic. [4] The asteroid was first observed as 1953 RP and 1953 RP1 at Heidelberg and Goethe Link Observatory, where the body's observation arc begins in September 1953, or 34 years prior to its official discovery observation at Brorfelde. [1]
Augustesen has been characterized as an X-type asteroid by Pan-STARRS ' photometric survey. [11] It is also an assumed S-type asteroid. [3]
In October 2006, a rotational lightcurve of Augustesen was obtained from photometric observations by Slovak astronomer Adrián Galád at Modra Observatory. Lightcurve analysis gave a long rotation period of 480 hours with a high brightness amplitude of 0.8 magnitude, indicative for a non-spherical shape ( U=3 ). [10] [lower-alpha 1] The asteroid is a slow rotator with a period much longer than the typical 2 to 20 hours measured for most observed asteroids. Augustesen is also a suspected tumbler with a non-principal axis rotation, also known as "tumbling". [3]
An alternative measurement by Laurent Bernasconi gave a much shorter period based on a fragmentary (poor) lightcurve ( U=1 ). [9]
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Augustesen measures between 6.445 and 9.73 kilometers in diameter and its surface has an albedo between 0.08 and 0.245. [5] [6] [7] [8]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.81 kilometers based on an absolute magnitude of 13.2. [3]
This minor planet was named after Karl Augustesen (born 1945), a Danish astronomer and co-discoverer of minor planets. For several decades he had been an observer using the Schmidt telescope at the discovering Brorfelde Observatory in Denmark, after which the asteroid 3309 Brorfelde was named. [1]
The corrected official naming citation was published by the Minor Planet Center on 22 June 2005 ( M.P.C. 54279). [12] In its preceding publication on 23 May 2005, the MPC erroneously named asteroid (6002) 1988 RO, which was discovered by Poul Jensen on 8 September 1988, as "6002 Augustesen" ( M.P.C. 54173). As of 2018, the JPL SBDB still shows the (incorrect) discovery date of that other asteroid. [12]
2829 Bobhope is a dark asteroid of the Meliboea family, from the outer region of the asteroid belt. It was discovered on 9 August 1948, by South African astronomer Ernest Leonard Johnson at Union Observatory in Johannesburg. The asteroid was later named after comedian Bob Hope. The asteroid has a rotation period of 6.1 hours and measures approximately 37 kilometers in diameter.
4349 Tibúrcio, provisional designation 1989 LX, is a dark asteroid from the central region of the asteroid belt, approximately 29 kilometers in diameter. It was discovered on 5 June 1989, by German astronomer Werner Landgraf at ESO's La Silla Observatory in northern Chile.
1743 Schmidt, provisional designation 4109 P-L, is a dark background asteroid from the inner regions of the asteroid belt, approximately 19 kilometers in diameter. It was discovered during the Palomar–Leiden survey on 24 September 1960, by astronomers Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at Palomar Observatory in California. The C-type asteroid has a rotation period of 17.5 hours. It was named for the optician Bernhard Schmidt.
11277 Ballard (provisional designation 1988 TW2) is a Phocaea asteroid from the inner regions of the asteroid belt, approximately 6.3 kilometers (3.9 miles) in diameter. It was discovered on 8 October 1988, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California. The assumed S-type asteroid has a rotation period of at least 10 hours. It was named for American marine scientist Robert Ballard.
1991 Darwin, provisional designation 1967 JL, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter.
4282 Endate, provisional designation 1987 UQ1, is an asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 28 October 1987, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at Kushiro Observatory (399) in Japan. It was named for amateur astronomer Kin Endate.
1736 Floirac, provisional designation 1967 RA, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8.7 kilometer in diameter.
2126 Gerasimovich, provisional designation 1970 QZ, is a stony background asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 30 August 1970, by Soviet astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named after Russian astronomer Boris Gerasimovich.
6709 Hiromiyuki, provisional designation 1989 CD, is a background or Florian asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 2 February 1989, by Japanese amateur astronomers Masaru Arai and Hiroshi Mori at the Yorii Observatory in Japan. The possibly elongated S-type asteroid has a rotation period of 6.8 hours. It was named after the Hiroshi Mori's children, Hiroyuki and Miyuki.
5900 Jensen, provisional designation 1986 TL, is a dark Lixiaohua asteroid from the outer regions of the asteroid belt, approximately 19 kilometers in diameter. It was discovered on 3 October 1986, by Danish astronomer Poul Jensen at the Brorfelde Observatory in Denmark. The asteroid was named for the discoverer and his wife Bodil Jensen.
4944 Kozlovskij, provisional designation 1987 RP3, is a carbonaceous Witt asteroid from the central regions of the asteroid belt, approximately 10 kilometers (6 miles) in diameter. It was discovered on 2 September 1987, by Soviet astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean Peninsula. The asteroid was named for Russian opera singer Ivan Kozlovsky.
2173 Maresjev, provisional designation 1974 QG1, is a dark background asteroid from the outer regions of the asteroid belt, approximately 28 kilometers (17 miles) in diameter. It was discovered on 22 August 1974, by Soviet–Ukrainian astronomer Lyudmila Zhuravleva at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. It was named for Soviet war veteran Alexey Maresyev. The assumed C-type asteroid has a tentative rotation period of 11.6 hours.
2696 Magion, provisional designation 1980 HB, is a dark background asteroid and a slow rotator from the inner regions of the asteroid belt, approximately 21 kilometers in diameter. It was discovered on 16 April 1980, by Slovak astronomer Ladislav Brožek at the Kleť Observatory in former Czechoslovakia. The X-type asteroid has an ambiguous rotation period of 480 hours and is possibly a tumbler. It was named for the first Czechoslovak satellite, Magion 1, launched in 1978.
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.
15350 Naganuma, provisional designation 1994 VB2, is a stony background asteroid from the inner regions of the asteroid belt, approximately 4.3 kilometers (2.7 miles) in diameter. It was discovered on 3 November 1994, by Japanese astronomers Yoshio Kushida and Osamu Muramatsu at the Yatsugatake South Base Observatory. The likely S-type asteroid has a rotation period of 2.5 hours. It was named for the town of Naganuma in northern Japan.
1696 Nurmela, provisional designation 1939 FF, is a Baptistina asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter. It was discovered on 18 March 1939, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland, and named after Finnish academician Tauno Nurmela. The possibly elongated asteroid has a rotation period of 3.15 hours.
2043 Ortutay, provisional designation 1936 TH, is a dark asteroid from the outer regions of the asteroid belt, approximately 45 kilometers in diameter. The asteroid was discovered by Hungarian astronomer György Kulin at the Konkoly Observatory, Budapest, on 12 November 1936. It was named after Hungarian ethnographer Gyula Ortutay.
1444 Pannonia is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 29 kilometers in diameter. It was discovered on 6 January 1938, by Hungarian astronomer György Kulin at Konkoly Observatory in Budapest, Hungary. It was named after the ancient province of the Roman Empire, Pannonia.
4804 Pasteur, provisional designation 1989 XC1, is a carbonaceous background asteroid from the central regions of the asteroid belt, approximately 20 kilometers in diameter. It was discovered on 2 December 1989, by Belgian astronomer Eric Elst at the ESO's La Silla Observatory in Chile. The asteroid was named after French chemist and microbiologist Louis Pasteur.
1565 Lemaître, provisional designation 1948 WA, is a highly eccentric Phocaea asteroid and sizable Mars-crosser from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 25 November 1948, by Belgian astronomer Sylvain Arend at the Royal Observatory of Belgium in Uccle, Belgium. It was named after cosmologist and priest Georges Lemaître.