| Discovery [1] | |
|---|---|
| Discovered by | L. Chernykh |
| Discovery site | Crimean Astrophysical Obs. |
| Discovery date | 3 October 1975 |
| Designations | |
| (5385) Kamenka | |
Named after | Kamianka [1] (Ukrainian town) |
| 1975 TS3 · 1975 UG 1986 TY1 | |
|
main-belt
[1]
[2] · (
outer)
[3] background [4] | |
| Orbital characteristics [2] | |
| Epoch 23 March 2018 ( JD 2458200.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 63.01 yr (23,016 d) |
| Aphelion | 3.8787 AU |
| Perihelion | 2.4352 AU |
| 3.1570 AU | |
| Eccentricity | 0.2286 |
| 5.61 yr (2,049 d) | |
| 253.72 ° | |
| 0° 10m 32.52s / day | |
| Inclination | 9.7974° |
| 41.394° | |
| 301.79° | |
| Physical characteristics | |
| 14.10±3.89
km
[5] 15.38±4.01 km [6] 16.768±0.317 km [7] [8] 20.21 km (calculated) [3] | |
| 5.93±0.04
h
[9] 6.683±0.008 h [10] | |
| 0.057 (assumed)
[3] 0.0828±0.0192 [8] 0.083±0.019 [7] 0.11±0.06 [6] 0.11±0.11 [5] | |
| C (assumed) [3] | |
| 12.20
[2]
[3]
[6]
[8] 12.24±0.11 (R) [9] 12.52 [5] 12.59±0.27 [11] | |
5385 Kamenka, provisional designation 1975 TS3, is a background asteroid from the outer regions of the asteroid belt, approximately 16 kilometers (10 miles) in diameter. It was discovered on 3 October 1975, by Soviet astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. [1] The presumed C-type asteroid has a rotation period of 6.68 hours. [3] It was named for the Ukrainian town of Kamianka. [1]
Orbit and classification
Kamenka is a non- family asteroid from the main belt's background population. [4] It orbits the Sun in the outer asteroid belt at a distance of 2.4–3.9 AU once every 5 years and 7 months (2,049 days; semi-major axis of 3.16 AU). Its orbit has an eccentricity of 0.23 and an inclination of 10 ° with respect to the ecliptic. [2] The body's observation arc begins with a precovery taken at Palomar Observatory in March 1955, twenty years prior to its official discovery observation at Nauchnij. [1]
Physical characteristics
Kamenka is an assumed carbonaceous C-type asteroid. [3]
Rotation period
Two rotational lightcurves of Kamenka have been obtained from photometric observations at the Palomar Transient Factory and at the Oakley Southern Sky and Oakley Observatory. [9] [10] Lightcurve analysis gave a rotation period of 5.93 and 6.683 hours with a brightness amplitude of 0.26 and 0.15 magnitude, respectively ( U=2/2). [3]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Kamenka measures between 14.10 and 16.768 kilometers in diameter and its surface has an albedo between 0.083 and 0.11. [5] [6] [7] [8]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 20.21 kilometers based on an absolute magnitude of 12.2. [3]
Naming
This minor planet was named after the town of Kamianka ( Ukrainian: Кам'янка; Russian: Камeнка), located in the Cherkasy Oblast region of central Ukraine. [1] The official naming citation was published by the Minor Planet Center on 24 January 2000 ( M.P.C. 38194). [12]
References
- ^ a b c d e f g "5385 Kamenka (1975 TS3)". Minor Planet Center. Retrieved 3 May 2018.
- ^ a b c d "JPL Small-Body Database Browser: 5385 Kamenka (1975 TS3)" (2018-03-27 last obs.). Jet Propulsion Laboratory. Retrieved 3 May 2018.
- ^ a b c d e f g h i "LCDB Data for (5385) Kamenka". Asteroid Lightcurve Database (LCDB). Retrieved 3 May 2018.
- ^ a b "Asteroid 5385 Kamenka – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
- ^ 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.
- ^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv: 1509.02522. Bibcode: 2015ApJ...814..117N. doi: 10.1088/0004-637X/814/2/117. S2CID 9341381.
- ^ a b c 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.
- ^ 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. ( catalog)
- ^ 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.
- ^ a b Carbo, Landy; Kragh, Katherine; Krotz, Jonathan; Meiers, Andrew; Shaffer, Nelson; Torno, Steven; et al. (July 2009). "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory and Oakley Observatory: 2008 September and October". The Minor Planet Bulletin. 36 (3): 91–94. Bibcode: 2009MPBu...36...91C. ISSN 1052-8091.
- ^ 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.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 May 2018.
External links
- Asteroid Lightcurve Database (LCDB), query form ( info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
- 5385 Kamenka at AstDyS-2, Asteroids—Dynamic Site
- 5385 Kamenka at the JPL Small-Body Database
| Discovery [1] | |
|---|---|
| Discovered by | L. Chernykh |
| Discovery site | Crimean Astrophysical Obs. |
| Discovery date | 3 October 1975 |
| Designations | |
| (5385) Kamenka | |
Named after | Kamianka [1] (Ukrainian town) |
| 1975 TS3 · 1975 UG 1986 TY1 | |
|
main-belt
[1]
[2] · (
outer)
[3] background [4] | |
| Orbital characteristics [2] | |
| Epoch 23 March 2018 ( JD 2458200.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 63.01 yr (23,016 d) |
| Aphelion | 3.8787 AU |
| Perihelion | 2.4352 AU |
| 3.1570 AU | |
| Eccentricity | 0.2286 |
| 5.61 yr (2,049 d) | |
| 253.72 ° | |
| 0° 10m 32.52s / day | |
| Inclination | 9.7974° |
| 41.394° | |
| 301.79° | |
| Physical characteristics | |
| 14.10±3.89
km
[5] 15.38±4.01 km [6] 16.768±0.317 km [7] [8] 20.21 km (calculated) [3] | |
| 5.93±0.04
h
[9] 6.683±0.008 h [10] | |
| 0.057 (assumed)
[3] 0.0828±0.0192 [8] 0.083±0.019 [7] 0.11±0.06 [6] 0.11±0.11 [5] | |
| C (assumed) [3] | |
| 12.20
[2]
[3]
[6]
[8] 12.24±0.11 (R) [9] 12.52 [5] 12.59±0.27 [11] | |
5385 Kamenka, provisional designation 1975 TS3, is a background asteroid from the outer regions of the asteroid belt, approximately 16 kilometers (10 miles) in diameter. It was discovered on 3 October 1975, by Soviet astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. [1] The presumed C-type asteroid has a rotation period of 6.68 hours. [3] It was named for the Ukrainian town of Kamianka. [1]
Orbit and classification
Kamenka is a non- family asteroid from the main belt's background population. [4] It orbits the Sun in the outer asteroid belt at a distance of 2.4–3.9 AU once every 5 years and 7 months (2,049 days; semi-major axis of 3.16 AU). Its orbit has an eccentricity of 0.23 and an inclination of 10 ° with respect to the ecliptic. [2] The body's observation arc begins with a precovery taken at Palomar Observatory in March 1955, twenty years prior to its official discovery observation at Nauchnij. [1]
Physical characteristics
Kamenka is an assumed carbonaceous C-type asteroid. [3]
Rotation period
Two rotational lightcurves of Kamenka have been obtained from photometric observations at the Palomar Transient Factory and at the Oakley Southern Sky and Oakley Observatory. [9] [10] Lightcurve analysis gave a rotation period of 5.93 and 6.683 hours with a brightness amplitude of 0.26 and 0.15 magnitude, respectively ( U=2/2). [3]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Kamenka measures between 14.10 and 16.768 kilometers in diameter and its surface has an albedo between 0.083 and 0.11. [5] [6] [7] [8]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 20.21 kilometers based on an absolute magnitude of 12.2. [3]
Naming
This minor planet was named after the town of Kamianka ( Ukrainian: Кам'янка; Russian: Камeнка), located in the Cherkasy Oblast region of central Ukraine. [1] The official naming citation was published by the Minor Planet Center on 24 January 2000 ( M.P.C. 38194). [12]
References
- ^ a b c d e f g "5385 Kamenka (1975 TS3)". Minor Planet Center. Retrieved 3 May 2018.
- ^ a b c d "JPL Small-Body Database Browser: 5385 Kamenka (1975 TS3)" (2018-03-27 last obs.). Jet Propulsion Laboratory. Retrieved 3 May 2018.
- ^ a b c d e f g h i "LCDB Data for (5385) Kamenka". Asteroid Lightcurve Database (LCDB). Retrieved 3 May 2018.
- ^ a b "Asteroid 5385 Kamenka – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
- ^ 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.
- ^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv: 1509.02522. Bibcode: 2015ApJ...814..117N. doi: 10.1088/0004-637X/814/2/117. S2CID 9341381.
- ^ a b c 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.
- ^ 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. ( catalog)
- ^ 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.
- ^ a b Carbo, Landy; Kragh, Katherine; Krotz, Jonathan; Meiers, Andrew; Shaffer, Nelson; Torno, Steven; et al. (July 2009). "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory and Oakley Observatory: 2008 September and October". The Minor Planet Bulletin. 36 (3): 91–94. Bibcode: 2009MPBu...36...91C. ISSN 1052-8091.
- ^ 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.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 May 2018.
External links
- Asteroid Lightcurve Database (LCDB), query form ( info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
- 5385 Kamenka at AstDyS-2, Asteroids—Dynamic Site
- 5385 Kamenka at the JPL Small-Body Database