| Discovery [1] | |
|---|---|
| Discovered by | Y. Väisälä |
| Discovery site | Turku Obs. |
| Discovery date | 20 January 1939 |
| Designations | |
| (1929) Kollaa | |
Named after |
Kollaa River
[2] ( river in Karelia) |
| 1939 BS · 1939 CH 1943 GG · 1968 BH 1976 JF3 | |
| main-belt · Vestian [3] | |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 ( JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 48.64 yr (17,766 days) |
| Aphelion | 2.5396 AU |
| Perihelion | 2.1862 AU |
| 2.3629 AU | |
| Eccentricity | 0.0748 |
| 3.63 yr (1,327 days) | |
| 226.60 ° | |
| 0° 16m 17.04s / day | |
| Inclination | 7.7797° |
| 65.429° | |
| 71.220° | |
| Physical characteristics | |
| Dimensions | 6.06 km (calculated)
[3] 6.71±0.34 km [4] 7.772±0.147 km [5] [6] |
| 2.980±0.005 h
[a] 2.9887±0.0004 h [7] | |
| 0.3855±0.0958
[5] 0.393±0.066 [4] [6] 0.4 (assumed) [3] | |
| SMASS = V [1] · V [3] | |
| 12.2 [5] · 12.50 [4] · 12.6 [1] · 12.64±0.32 [8] · 12.7 [3] | |
1929 Kollaa, provisional designation 1939 BS, is a stony Vestian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland, on 20 January 1939. [9] The asteroid was named after the Kollaa River in what is now Russia. [2]
Orbit and classification
Kollaa is a member of the Vesta family. Vestian asteroids have a composition akin to cumulate eucrite meteorites and are thought to have originated deep within 4 Vesta's crust, possibly from the Rheasilvia crater, a large impact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision. The asteroid Vesta is the main-belt's second-most-massive body after 1 Ceres. [10]
The asteroid orbits the Sun in the inner main-belt at a distance of 2.2–2.5 AU once every 3 years and 8 months (1,327 days). Its orbit has an eccentricity of 0.07 and an inclination of 8 ° with respect to the ecliptic. [1] As no precoveries were taken, the asteroid's observation arc begins with its discovery. [9]
Physical characteristics
In the SMASS taxonomy, Kollaa is a bright V-type asteroid. [1]
Lightcurves
It has a well-defined rotation period of 2.98 hours, derived from two rotational lightcurve analysis. In March 2004, photometric observations at the U.S. Magdalena Ridge Observatory in New Mexico rendered a period of 2.980 hours with a brightness variation of 0.20 in magnitude ( U=3). [a] In 2008 a second, concurring period was obtained by French amateur astronomer Pierre Antonini at his private Observatoire de Bédoin in France ( 132). It gave a period of 2.9887 hours and an amplitude 0.22 in magnitude ( U=3). [7]
Diameter and albedo
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, the body measures 6.7 and 7.7 kilometers in diameter, respectively, and its surface has an albedo 0.39. [4] [5] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.40 and calculates a diameter of 6.4 kilometers with an absolute magnitude of 12.7. [3]
Naming
This minor planet is named after the Kollaa River in Karelia, the focal point of violent battles during the Finnish Winter War (1939–40). [2] The official naming citation was published by the Minor Planet Center on 1 August 1980 ( M.P.C. 5450). [11]
Notes
- ^ a b Ryan (2007) web: rotation period 2.980±0.005 hours with a brightness amplitude of 0.22 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (1929) Kollaa from unpublished results by W. H. Ryan and E.V. Ryan, (2007).
References
- ^ a b c d e f "JPL Small-Body Database Browser: 1929 Kollaa (1939 BS)" (2016-09-14 last obs.). Jet Propulsion Laboratory. Archived from the original on 18 September 2020. Retrieved 10 June 2017.
- ^ a b c Schmadel, Lutz D. (2007). "(1929) Kollaa". Dictionary of Minor Planet Names – (1929) Kollaa. Springer Berlin Heidelberg. p. 155. doi: 10.1007/978-3-540-29925-7_1930. ISBN 978-3-540-00238-3.
- ^ a b c d e f "LCDB Data for (1929) Kollaa". Asteroid Lightcurve Database (LCDB). Retrieved 24 July 2016.
- ^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv: 1209.5794. Bibcode: 2012ApJ...759L...8M. doi: 10.1088/2041-8205/759/1/L8. S2CID 46350317. Retrieved 24 July 2016.
- ^ 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. Retrieved 24 July 2016.
- ^ a b Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv: 1109.4096. Bibcode: 2011ApJ...741...68M. doi: 10.1088/0004-637X/741/2/68. S2CID 118745497. Retrieved 8 December 2016.
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1929) Kollaa". Geneva Observatory. Retrieved 24 July 2016.
- ^ 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 24 July 2016.
- ^ a b "1929 Kollaa (1939 BS)". Minor Planet Center. Retrieved 24 July 2016.
- ^ Kelley, Michael S.; Vilas, Faith; Gaffey, Michael J.; Abell, Paul A. (September 2003). "Quantified mineralogical evidence for a common origin of 1929 Kollaa with 4 Vesta and the HED meteorites". Icarus. 165 (1): 215–218. Bibcode: 2003Icar..165..215K. doi: 10.1016/S0019-1035(03)00149-0. Retrieved 18 January 2016.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 July 2016.
External links
- Asteroid Lightcurve Database (LCDB), query form ( info Archived 21 July 2011 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1929 Kollaa at AstDyS-2, Asteroids—Dynamic Site
- 1929 Kollaa at the JPL Small-Body Database
| Discovery [1] | |
|---|---|
| Discovered by | Y. Väisälä |
| Discovery site | Turku Obs. |
| Discovery date | 20 January 1939 |
| Designations | |
| (1929) Kollaa | |
Named after |
Kollaa River
[2] ( river in Karelia) |
| 1939 BS · 1939 CH 1943 GG · 1968 BH 1976 JF3 | |
| main-belt · Vestian [3] | |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 ( JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 48.64 yr (17,766 days) |
| Aphelion | 2.5396 AU |
| Perihelion | 2.1862 AU |
| 2.3629 AU | |
| Eccentricity | 0.0748 |
| 3.63 yr (1,327 days) | |
| 226.60 ° | |
| 0° 16m 17.04s / day | |
| Inclination | 7.7797° |
| 65.429° | |
| 71.220° | |
| Physical characteristics | |
| Dimensions | 6.06 km (calculated)
[3] 6.71±0.34 km [4] 7.772±0.147 km [5] [6] |
| 2.980±0.005 h
[a] 2.9887±0.0004 h [7] | |
| 0.3855±0.0958
[5] 0.393±0.066 [4] [6] 0.4 (assumed) [3] | |
| SMASS = V [1] · V [3] | |
| 12.2 [5] · 12.50 [4] · 12.6 [1] · 12.64±0.32 [8] · 12.7 [3] | |
1929 Kollaa, provisional designation 1939 BS, is a stony Vestian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland, on 20 January 1939. [9] The asteroid was named after the Kollaa River in what is now Russia. [2]
Orbit and classification
Kollaa is a member of the Vesta family. Vestian asteroids have a composition akin to cumulate eucrite meteorites and are thought to have originated deep within 4 Vesta's crust, possibly from the Rheasilvia crater, a large impact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision. The asteroid Vesta is the main-belt's second-most-massive body after 1 Ceres. [10]
The asteroid orbits the Sun in the inner main-belt at a distance of 2.2–2.5 AU once every 3 years and 8 months (1,327 days). Its orbit has an eccentricity of 0.07 and an inclination of 8 ° with respect to the ecliptic. [1] As no precoveries were taken, the asteroid's observation arc begins with its discovery. [9]
Physical characteristics
In the SMASS taxonomy, Kollaa is a bright V-type asteroid. [1]
Lightcurves
It has a well-defined rotation period of 2.98 hours, derived from two rotational lightcurve analysis. In March 2004, photometric observations at the U.S. Magdalena Ridge Observatory in New Mexico rendered a period of 2.980 hours with a brightness variation of 0.20 in magnitude ( U=3). [a] In 2008 a second, concurring period was obtained by French amateur astronomer Pierre Antonini at his private Observatoire de Bédoin in France ( 132). It gave a period of 2.9887 hours and an amplitude 0.22 in magnitude ( U=3). [7]
Diameter and albedo
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, the body measures 6.7 and 7.7 kilometers in diameter, respectively, and its surface has an albedo 0.39. [4] [5] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.40 and calculates a diameter of 6.4 kilometers with an absolute magnitude of 12.7. [3]
Naming
This minor planet is named after the Kollaa River in Karelia, the focal point of violent battles during the Finnish Winter War (1939–40). [2] The official naming citation was published by the Minor Planet Center on 1 August 1980 ( M.P.C. 5450). [11]
Notes
- ^ a b Ryan (2007) web: rotation period 2.980±0.005 hours with a brightness amplitude of 0.22 mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (1929) Kollaa from unpublished results by W. H. Ryan and E.V. Ryan, (2007).
References
- ^ a b c d e f "JPL Small-Body Database Browser: 1929 Kollaa (1939 BS)" (2016-09-14 last obs.). Jet Propulsion Laboratory. Archived from the original on 18 September 2020. Retrieved 10 June 2017.
- ^ a b c Schmadel, Lutz D. (2007). "(1929) Kollaa". Dictionary of Minor Planet Names – (1929) Kollaa. Springer Berlin Heidelberg. p. 155. doi: 10.1007/978-3-540-29925-7_1930. ISBN 978-3-540-00238-3.
- ^ a b c d e f "LCDB Data for (1929) Kollaa". Asteroid Lightcurve Database (LCDB). Retrieved 24 July 2016.
- ^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv: 1209.5794. Bibcode: 2012ApJ...759L...8M. doi: 10.1088/2041-8205/759/1/L8. S2CID 46350317. Retrieved 24 July 2016.
- ^ 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. Retrieved 24 July 2016.
- ^ a b Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv: 1109.4096. Bibcode: 2011ApJ...741...68M. doi: 10.1088/0004-637X/741/2/68. S2CID 118745497. Retrieved 8 December 2016.
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1929) Kollaa". Geneva Observatory. Retrieved 24 July 2016.
- ^ 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 24 July 2016.
- ^ a b "1929 Kollaa (1939 BS)". Minor Planet Center. Retrieved 24 July 2016.
- ^ Kelley, Michael S.; Vilas, Faith; Gaffey, Michael J.; Abell, Paul A. (September 2003). "Quantified mineralogical evidence for a common origin of 1929 Kollaa with 4 Vesta and the HED meteorites". Icarus. 165 (1): 215–218. Bibcode: 2003Icar..165..215K. doi: 10.1016/S0019-1035(03)00149-0. Retrieved 18 January 2016.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 July 2016.
External links
- Asteroid Lightcurve Database (LCDB), query form ( info Archived 21 July 2011 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1929 Kollaa at AstDyS-2, Asteroids—Dynamic Site
- 1929 Kollaa at the JPL Small-Body Database