Discovery [1] | |
---|---|
Discovered by | C. Rinner |
Discovery site | Ottmarsheim Obs. |
Discovery date | 10 August 2005 |
Designations | |
(120375) Kugel | |
Named after |
François Kugel
[1] (French astronomer) |
2005 PB6 · 1998 SM108 2001 KE74 | |
main-belt
[1]
[2] · (
inner) background [3] [4] · near-Flora [5] | |
Orbital characteristics [2] | |
Epoch 1 July 2021 ( JD 2459396.5) | |
Uncertainty parameter 0 | |
Observation arc | 22.53 yr (8,228 d) |
Aphelion | 2.8289 AU |
Perihelion | 1.8077 AU |
2.3183 AU | |
Eccentricity | 0.2202 |
3.53 yr (1,289 d) | |
189.77 ° | |
0° 16m 45.12s / day | |
Inclination | 2.7591° |
229.91° | |
97.616° | |
Physical characteristics | |
Mean diameter | 1.05 km (calculated) [5] |
6.923±0.0085 h [6] | |
0.24 (assumed) [5] | |
S/ Q ( SDSS-MOC) [7] | |
16.619±0.003 (R)
[6] 16.7 [2] · 17.07 [5] | |
120375 Kugel, provisional designation: 2005 PB6, is a background asteroid from the inner regions of the asteroid belt, approximately 1 kilometer (0.6 miles) in diameter. It was discovered on 10 August 2005, by French amateur astronomer Claudine Rinner at her Ottmarsheim Observatory ( 224) in France. [1] The stony S/ Q-type asteroid in the region of the Florian clan has a tentative rotation period of 6.9 hours. [5] It was named after French astronomer François Kugel. [1]
Kugel is a non- family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. [3] [4] Based on osculating Keplerian orbital elements, the asteroid has also been considered a member of the Flora family ( 402), a giant asteroid clan and the largest family of stony asteroids in the main belt. [5]
It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,289 days; semi-major axis of 2.32 AU). Its orbit has an eccentricity of 0.22 and an inclination of 3 ° with respect to the ecliptic. [2] The body's observation arc begins with its first observation as 1998 SM108 at Lincoln Laboratory ETS in September 1998, nearly 7 years prior to its official discovery observation at Ottmarsheim. [1]
This minor planet was named after French amateur astronomer François Kugel (born 1959), an active observer of comets and a collaborator of the discoverer. He has founded the Chante-Perdrix Observatory ( A77) in 2005. [1] The official naming citation was published by the Minor Planet Center on 6 August 2009 ( M.P.C. 66728). [8]
In the SDSS-based taxonomy, Kugel has an SQ-type that transitions between the common S-type and less common Q-type asteroids. [7]
In August 2012, a rotational lightcurve of Kugel was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a tentative rotation period of 6.923±0.0085 hours with a weak brightness amplitude of 0.09 magnitude ( U=1). [6] As of 2021, no secure period has been obtained. [5]
Kugel has not been observed by any of the space-based surveys such as the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the Akari satellite or IRAS. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora the parent body of the Flora family – and calculates a diameter of 1.05 kilometers based on an absolute magnitude of 17.07. [5]
Discovery [1] | |
---|---|
Discovered by | C. Rinner |
Discovery site | Ottmarsheim Obs. |
Discovery date | 10 August 2005 |
Designations | |
(120375) Kugel | |
Named after |
François Kugel
[1] (French astronomer) |
2005 PB6 · 1998 SM108 2001 KE74 | |
main-belt
[1]
[2] · (
inner) background [3] [4] · near-Flora [5] | |
Orbital characteristics [2] | |
Epoch 1 July 2021 ( JD 2459396.5) | |
Uncertainty parameter 0 | |
Observation arc | 22.53 yr (8,228 d) |
Aphelion | 2.8289 AU |
Perihelion | 1.8077 AU |
2.3183 AU | |
Eccentricity | 0.2202 |
3.53 yr (1,289 d) | |
189.77 ° | |
0° 16m 45.12s / day | |
Inclination | 2.7591° |
229.91° | |
97.616° | |
Physical characteristics | |
Mean diameter | 1.05 km (calculated) [5] |
6.923±0.0085 h [6] | |
0.24 (assumed) [5] | |
S/ Q ( SDSS-MOC) [7] | |
16.619±0.003 (R)
[6] 16.7 [2] · 17.07 [5] | |
120375 Kugel, provisional designation: 2005 PB6, is a background asteroid from the inner regions of the asteroid belt, approximately 1 kilometer (0.6 miles) in diameter. It was discovered on 10 August 2005, by French amateur astronomer Claudine Rinner at her Ottmarsheim Observatory ( 224) in France. [1] The stony S/ Q-type asteroid in the region of the Florian clan has a tentative rotation period of 6.9 hours. [5] It was named after French astronomer François Kugel. [1]
Kugel is a non- family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. [3] [4] Based on osculating Keplerian orbital elements, the asteroid has also been considered a member of the Flora family ( 402), a giant asteroid clan and the largest family of stony asteroids in the main belt. [5]
It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,289 days; semi-major axis of 2.32 AU). Its orbit has an eccentricity of 0.22 and an inclination of 3 ° with respect to the ecliptic. [2] The body's observation arc begins with its first observation as 1998 SM108 at Lincoln Laboratory ETS in September 1998, nearly 7 years prior to its official discovery observation at Ottmarsheim. [1]
This minor planet was named after French amateur astronomer François Kugel (born 1959), an active observer of comets and a collaborator of the discoverer. He has founded the Chante-Perdrix Observatory ( A77) in 2005. [1] The official naming citation was published by the Minor Planet Center on 6 August 2009 ( M.P.C. 66728). [8]
In the SDSS-based taxonomy, Kugel has an SQ-type that transitions between the common S-type and less common Q-type asteroids. [7]
In August 2012, a rotational lightcurve of Kugel was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a tentative rotation period of 6.923±0.0085 hours with a weak brightness amplitude of 0.09 magnitude ( U=1). [6] As of 2021, no secure period has been obtained. [5]
Kugel has not been observed by any of the space-based surveys such as the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the Akari satellite or IRAS. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora the parent body of the Flora family – and calculates a diameter of 1.05 kilometers based on an absolute magnitude of 17.07. [5]