Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 26 February 1928 |
Designations | |
(1091) Spiraea | |
Pronunciation | /spaɪˈriːə/ [2] |
Named after |
Spiraea (genus of shrubs) [3] |
1928 DT · 1934 CN1 1938 UR · 1964 XH | |
main-belt · (
outer)
[1]
[4] Cybele · background [5] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 89.27 yr (32,606 days) |
Aphelion | 3.6484 AU |
Perihelion | 3.2077 AU |
3.4281 AU | |
Eccentricity | 0.0643 |
6.35 yr (2,318 days) | |
110.37 ° | |
0° 9m 19.08s / day | |
Inclination | 1.1554° |
80.790° | |
12.062° | |
Physical characteristics | |
Dimensions | 32.78 km (calculated)
[4] 35.178±0.108 km [6] 39.92±17.85 km [7] 40.280±0.455 km [8] 40.52±0.91 km [9] |
7.01±0.43 h [10] | |
0.05±0.06
[7] 0.057 (assumed) [4] 0.0627±0.0106 [8] 0.063±0.003 [9] 0.091±0.025 [6] | |
C (assumed) [4] | |
10.60 [8] [9] · 10.70±0.08 (R) [10] · 10.8 [1] · 11.00±0.14 [11] · 11.15 [4] · 11.18 [7] | |
1091 Spiraea, provisional designation 1928 DT, is a carbonaceous Cybele asteroid from the outer regions of the asteroid belt, approximately 36 kilometers in diameter. It was discovered on 26 February 1928, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. [12] The asteroid was named after Spiraea, a genus of plants. [3]
Spiraea orbits the Sun in the outer main-belt at a distance of 3.2–3.6 AU once every 6 years and 4 months (2,318 days). Its orbit has an eccentricity of 0.06 and an inclination of 1 ° with respect to the ecliptic. [1] With these orbital parameters, it belongs to the Cybele asteroids, a dynamical group near the 4:7 resonance with Jupiter and named after one of the largest asteroids, 65 Cybele. It is, however, a non- family asteroid from the main belt's background population when applying the hierarchical clustering method (Nesvorny, Novakovic, Knezevic and Milani) to its proper orbital elements. [5]
The body's observation arc begins with its identification as 1934 CN1 at Uccle Observatory in February 1934, almost six years after its official discovery observation at Heidelberg. [12]
Spiraea is an assumed carbonaceous C-type asteroid. [4]
In December 2014, a fragmentary rotational lightcurve of Spiraea was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 7.01 hours with a brightness amplitude of 0.03 magnitude ( U=1+). [10]
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Spiraea measures between 35.178 and 40.52 kilometers in diameter and its surface has an albedo between 0.05 and 0.091. [6] [7] [8] [9]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 32.78 kilometers based on an absolute magnitude of 11.15. [4]
This minor planet was named after Spiraea, a genus of shrubs of the rose family ( Rosaceae), with small white or pink flowers. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 ( H 103). [3]
Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between (1009) and (1200). This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were all named after plants, in particular flowering plants (also see list of minor planets named after animals and plants). [13]
Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 26 February 1928 |
Designations | |
(1091) Spiraea | |
Pronunciation | /spaɪˈriːə/ [2] |
Named after |
Spiraea (genus of shrubs) [3] |
1928 DT · 1934 CN1 1938 UR · 1964 XH | |
main-belt · (
outer)
[1]
[4] Cybele · background [5] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 89.27 yr (32,606 days) |
Aphelion | 3.6484 AU |
Perihelion | 3.2077 AU |
3.4281 AU | |
Eccentricity | 0.0643 |
6.35 yr (2,318 days) | |
110.37 ° | |
0° 9m 19.08s / day | |
Inclination | 1.1554° |
80.790° | |
12.062° | |
Physical characteristics | |
Dimensions | 32.78 km (calculated)
[4] 35.178±0.108 km [6] 39.92±17.85 km [7] 40.280±0.455 km [8] 40.52±0.91 km [9] |
7.01±0.43 h [10] | |
0.05±0.06
[7] 0.057 (assumed) [4] 0.0627±0.0106 [8] 0.063±0.003 [9] 0.091±0.025 [6] | |
C (assumed) [4] | |
10.60 [8] [9] · 10.70±0.08 (R) [10] · 10.8 [1] · 11.00±0.14 [11] · 11.15 [4] · 11.18 [7] | |
1091 Spiraea, provisional designation 1928 DT, is a carbonaceous Cybele asteroid from the outer regions of the asteroid belt, approximately 36 kilometers in diameter. It was discovered on 26 February 1928, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. [12] The asteroid was named after Spiraea, a genus of plants. [3]
Spiraea orbits the Sun in the outer main-belt at a distance of 3.2–3.6 AU once every 6 years and 4 months (2,318 days). Its orbit has an eccentricity of 0.06 and an inclination of 1 ° with respect to the ecliptic. [1] With these orbital parameters, it belongs to the Cybele asteroids, a dynamical group near the 4:7 resonance with Jupiter and named after one of the largest asteroids, 65 Cybele. It is, however, a non- family asteroid from the main belt's background population when applying the hierarchical clustering method (Nesvorny, Novakovic, Knezevic and Milani) to its proper orbital elements. [5]
The body's observation arc begins with its identification as 1934 CN1 at Uccle Observatory in February 1934, almost six years after its official discovery observation at Heidelberg. [12]
Spiraea is an assumed carbonaceous C-type asteroid. [4]
In December 2014, a fragmentary rotational lightcurve of Spiraea was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 7.01 hours with a brightness amplitude of 0.03 magnitude ( U=1+). [10]
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Spiraea measures between 35.178 and 40.52 kilometers in diameter and its surface has an albedo between 0.05 and 0.091. [6] [7] [8] [9]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 32.78 kilometers based on an absolute magnitude of 11.15. [4]
This minor planet was named after Spiraea, a genus of shrubs of the rose family ( Rosaceae), with small white or pink flowers. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 ( H 103). [3]
Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between (1009) and (1200). This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were all named after plants, in particular flowering plants (also see list of minor planets named after animals and plants). [13]