From Wikipedia, the free encyclopedia

1091 Spiraea
Discovery [1]
Discovered by K. Reinmuth
Discovery site Heidelberg Obs.
Discovery date26 February 1928
Designations
(1091) Spiraea
Pronunciation /spˈrə/ [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 arc89.27 yr (32,606 days)
Aphelion3.6484 AU
Perihelion3.2077 AU
3.4281 AU
Eccentricity0.0643
6.35 yr (2,318 days)
110.37 °
0° 9m 19.08s / day
Inclination1.1554°
80.790°
12.062°
Physical characteristics
Dimensions32.78 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]

Orbit and classification

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]

Physical characteristics

Spiraea is an assumed carbonaceous C-type asteroid. [4]

Rotation period

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]

Diameter and albedo

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]

Naming

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]

Reinmuth's flowers

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]

References

  1. ^ a b c d e "JPL Small-Body Database Browser: 1091 Spiraea (1928 DT)" (2017-06-04 last obs.). Jet Propulsion Laboratory. Retrieved 26 September 2017.
  2. ^ "spiræa". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  3. ^ a b c Schmadel, Lutz D. (2007). "(1091) Spiraea". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 93. doi: 10.1007/978-3-540-29925-7_1092. ISBN  978-3-540-00238-3.
  4. ^ a b c d e f g "LCDB Data for (1091) Spiraea". Asteroid Lightcurve Database (LCDB). Retrieved 26 September 2017.
  5. ^ a b "Asteroid 1091 Spiraea – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 28 October 2019.
  6. ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv: 1406.6645. Bibcode: 2014ApJ...791..121M. doi: 10.1088/0004-637X/791/2/121. S2CID  119293330. Retrieved 26 September 2017.
  7. ^ a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv: 1606.08923. Bibcode: 2016AJ....152...63N. doi: 10.3847/0004-6256/152/3/63.
  8. ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: 1109.6407. Bibcode: 2011ApJ...741...90M. doi: 10.1088/0004-637X/741/2/90. S2CID  35447010.
  9. ^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode: 2011PASJ...63.1117U. doi: 10.1093/pasj/63.5.1117. ( online, AcuA catalog p. 153)
  10. ^ a b c Chang, Chan-Kao; Lin, Hsing-Wen; Ip, Wing-Huen; Prince, Thomas A.; Kulkarni, Shrinivas R.; Levitan, David; et al. (December 2016). "Large Super-fast Rotator Hunting Using the Intermediate Palomar Transient Factory". The Astrophysical Journal Supplement Series. 227 (2): 13. arXiv: 1608.07910. Bibcode: 2016ApJS..227...20C. doi: 10.3847/0067-0049/227/2/20. S2CID  30387146.
  11. ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: 1506.00762. Bibcode: 2015Icar..261...34V. doi: 10.1016/j.icarus.2015.08.007. S2CID  53493339. Retrieved 26 September 2017.
  12. ^ a b "1091 Spiraea (1928 DT)". Minor Planet Center. Retrieved 26 September 2017.
  13. ^ Schmadel, Lutz D. (2007). "(1054) Forsytia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 90. doi: 10.1007/978-3-540-29925-7_1055. ISBN  978-3-540-00238-3.

External links

From Wikipedia, the free encyclopedia

1091 Spiraea
Discovery [1]
Discovered by K. Reinmuth
Discovery site Heidelberg Obs.
Discovery date26 February 1928
Designations
(1091) Spiraea
Pronunciation /spˈrə/ [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 arc89.27 yr (32,606 days)
Aphelion3.6484 AU
Perihelion3.2077 AU
3.4281 AU
Eccentricity0.0643
6.35 yr (2,318 days)
110.37 °
0° 9m 19.08s / day
Inclination1.1554°
80.790°
12.062°
Physical characteristics
Dimensions32.78 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]

Orbit and classification

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]

Physical characteristics

Spiraea is an assumed carbonaceous C-type asteroid. [4]

Rotation period

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]

Diameter and albedo

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]

Naming

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]

Reinmuth's flowers

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]

References

  1. ^ a b c d e "JPL Small-Body Database Browser: 1091 Spiraea (1928 DT)" (2017-06-04 last obs.). Jet Propulsion Laboratory. Retrieved 26 September 2017.
  2. ^ "spiræa". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  3. ^ a b c Schmadel, Lutz D. (2007). "(1091) Spiraea". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 93. doi: 10.1007/978-3-540-29925-7_1092. ISBN  978-3-540-00238-3.
  4. ^ a b c d e f g "LCDB Data for (1091) Spiraea". Asteroid Lightcurve Database (LCDB). Retrieved 26 September 2017.
  5. ^ a b "Asteroid 1091 Spiraea – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 28 October 2019.
  6. ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv: 1406.6645. Bibcode: 2014ApJ...791..121M. doi: 10.1088/0004-637X/791/2/121. S2CID  119293330. Retrieved 26 September 2017.
  7. ^ a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv: 1606.08923. Bibcode: 2016AJ....152...63N. doi: 10.3847/0004-6256/152/3/63.
  8. ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: 1109.6407. Bibcode: 2011ApJ...741...90M. doi: 10.1088/0004-637X/741/2/90. S2CID  35447010.
  9. ^ a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode: 2011PASJ...63.1117U. doi: 10.1093/pasj/63.5.1117. ( online, AcuA catalog p. 153)
  10. ^ a b c Chang, Chan-Kao; Lin, Hsing-Wen; Ip, Wing-Huen; Prince, Thomas A.; Kulkarni, Shrinivas R.; Levitan, David; et al. (December 2016). "Large Super-fast Rotator Hunting Using the Intermediate Palomar Transient Factory". The Astrophysical Journal Supplement Series. 227 (2): 13. arXiv: 1608.07910. Bibcode: 2016ApJS..227...20C. doi: 10.3847/0067-0049/227/2/20. S2CID  30387146.
  11. ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: 1506.00762. Bibcode: 2015Icar..261...34V. doi: 10.1016/j.icarus.2015.08.007. S2CID  53493339. Retrieved 26 September 2017.
  12. ^ a b "1091 Spiraea (1928 DT)". Minor Planet Center. Retrieved 26 September 2017.
  13. ^ Schmadel, Lutz D. (2007). "(1054) Forsytia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 90. doi: 10.1007/978-3-540-29925-7_1055. ISBN  978-3-540-00238-3.

External links


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