| Discovery [1] | |
|---|---|
| Discovered by | Y. Väisälä |
| Discovery site | Turku Obs. |
| Discovery date | 3 April 1940 |
| Designations | |
| (3099) Hergenrother | |
Named after |
Carl Hergenrother (American astronomer) [2] |
| 1940 GF · 1969 EF1 1972 VV · 1979 KE 1980 NT · 1984 HB 1984 JG | |
| main-belt · ( outer) [3] | |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 ( JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 76.96 yr (28,111 days) |
| Aphelion | 3.4563 AU |
| Perihelion | 2.3048 AU |
| 2.8805 AU | |
| Eccentricity | 0.1999 |
| 4.89 yr (1,786 days) | |
| 309.42 ° | |
| 0° 12m 5.76s / day | |
| Inclination | 15.496° |
| 31.100° | |
| 148.52° | |
| Physical characteristics | |
| Dimensions | 14.732±0.110 km
[4]
[5] 29.21 km (calculated) [3] |
| 24.266±0.007 h [6] | |
| 0.057 (assumed)
[3] 0.224±0.016 [4] [5] | |
| C [3] | |
| 11.4 [1] [3] [4] | |
3099 Hergenrother, provisional designation 1940 GF, is an asteroid from the outer region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 3 April 1940, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland, [7] and named after American astronomer Carl Hergenrother in 1996. [2]
Orbit and classification
Hergenrother orbits the Sun in the outer main-belt at a distance of 2.3–3.5 AU once every 4 years and 11 months (1,786 days). Its orbit has an eccentricity of 0.20 and an inclination of 15 ° with respect to the ecliptic. [1] The body's observation arc begins 6 days after its official discovery observation at Turku. [7]
Physical characteristics
Rotation period
In January 2008, a rotational lightcurve of Hergenrother was obtained from photometric observations by French amateur astronomer Pierre Antonini. Lightcurve analysis gave a rotation period of 24.266 hours with a brightness variation of 0.28 magnitude ( U=2). [6]
Diameter and albedo
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Hergenrother measures 14.73 kilometers in diameter and its surface has an albedo of 0.224, [4] [5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and consequently calculates a diameter of 29.21 kilometers, as the lower the albedo, the larger the body's diameter at a certain absolute magnitude. [3]
Naming
This minor planet was named in honor of American astronomer Carl W. Hergenrother (born 1973). At Lunar and Planetary Laboratory, he has been a discoverer of minor planets with high inclinations during the Bigelow Sky Survey, precursor to the Catalina Sky Survey. The naming was proposed by MPC director Brian G. Marsden among others. [2] The official naming citation was published by the Minor Planet Center on 3 May 1996 ( M.P.C. 27124). [8]
References
- ^ a b c d "JPL Small-Body Database Browser: 3099 Hergenrother (1940 GF)" (2017-03-21 last obs.). Jet Propulsion Laboratory. Retrieved 16 June 2017.
- ^ a b c Schmadel, Lutz D. (2007). "(3099) Hergenrother". Dictionary of Minor Planet Names – (3099) Hergenrother. Springer Berlin Heidelberg. p. 255. doi: 10.1007/978-3-540-29925-7_3100. ISBN 978-3-540-00238-3.
- ^ a b c d e f "LCDB Data for (3099) Hergenrother". Asteroid Lightcurve Database (LCDB). Retrieved 8 March 2017.
- ^ 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.
- ^ 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. Retrieved 8 March 2017.
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (3099) Hergenrother". Geneva Observatory. Retrieved 8 March 2017.
- ^ a b "3099 Hergenrother (1940 GF)". Minor Planet Center. Retrieved 8 March 2017.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 8 March 2017.
External links
- Get to Know a Staff Scientist: Carl Hergenrother, Lunar & Planetary Laboratory, University of Arizona
- Asteroid Lightcurve Database (LCDB), query form ( info Archived 16 December 2017 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
- 3099 Hergenrother at AstDyS-2, Asteroids—Dynamic Site
- 3099 Hergenrother at the JPL Small-Body Database
| Discovery [1] | |
|---|---|
| Discovered by | Y. Väisälä |
| Discovery site | Turku Obs. |
| Discovery date | 3 April 1940 |
| Designations | |
| (3099) Hergenrother | |
Named after |
Carl Hergenrother (American astronomer) [2] |
| 1940 GF · 1969 EF1 1972 VV · 1979 KE 1980 NT · 1984 HB 1984 JG | |
| main-belt · ( outer) [3] | |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 ( JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 76.96 yr (28,111 days) |
| Aphelion | 3.4563 AU |
| Perihelion | 2.3048 AU |
| 2.8805 AU | |
| Eccentricity | 0.1999 |
| 4.89 yr (1,786 days) | |
| 309.42 ° | |
| 0° 12m 5.76s / day | |
| Inclination | 15.496° |
| 31.100° | |
| 148.52° | |
| Physical characteristics | |
| Dimensions | 14.732±0.110 km
[4]
[5] 29.21 km (calculated) [3] |
| 24.266±0.007 h [6] | |
| 0.057 (assumed)
[3] 0.224±0.016 [4] [5] | |
| C [3] | |
| 11.4 [1] [3] [4] | |
3099 Hergenrother, provisional designation 1940 GF, is an asteroid from the outer region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 3 April 1940, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland, [7] and named after American astronomer Carl Hergenrother in 1996. [2]
Orbit and classification
Hergenrother orbits the Sun in the outer main-belt at a distance of 2.3–3.5 AU once every 4 years and 11 months (1,786 days). Its orbit has an eccentricity of 0.20 and an inclination of 15 ° with respect to the ecliptic. [1] The body's observation arc begins 6 days after its official discovery observation at Turku. [7]
Physical characteristics
Rotation period
In January 2008, a rotational lightcurve of Hergenrother was obtained from photometric observations by French amateur astronomer Pierre Antonini. Lightcurve analysis gave a rotation period of 24.266 hours with a brightness variation of 0.28 magnitude ( U=2). [6]
Diameter and albedo
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Hergenrother measures 14.73 kilometers in diameter and its surface has an albedo of 0.224, [4] [5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and consequently calculates a diameter of 29.21 kilometers, as the lower the albedo, the larger the body's diameter at a certain absolute magnitude. [3]
Naming
This minor planet was named in honor of American astronomer Carl W. Hergenrother (born 1973). At Lunar and Planetary Laboratory, he has been a discoverer of minor planets with high inclinations during the Bigelow Sky Survey, precursor to the Catalina Sky Survey. The naming was proposed by MPC director Brian G. Marsden among others. [2] The official naming citation was published by the Minor Planet Center on 3 May 1996 ( M.P.C. 27124). [8]
References
- ^ a b c d "JPL Small-Body Database Browser: 3099 Hergenrother (1940 GF)" (2017-03-21 last obs.). Jet Propulsion Laboratory. Retrieved 16 June 2017.
- ^ a b c Schmadel, Lutz D. (2007). "(3099) Hergenrother". Dictionary of Minor Planet Names – (3099) Hergenrother. Springer Berlin Heidelberg. p. 255. doi: 10.1007/978-3-540-29925-7_3100. ISBN 978-3-540-00238-3.
- ^ a b c d e f "LCDB Data for (3099) Hergenrother". Asteroid Lightcurve Database (LCDB). Retrieved 8 March 2017.
- ^ 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.
- ^ 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. Retrieved 8 March 2017.
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (3099) Hergenrother". Geneva Observatory. Retrieved 8 March 2017.
- ^ a b "3099 Hergenrother (1940 GF)". Minor Planet Center. Retrieved 8 March 2017.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 8 March 2017.
External links
- Get to Know a Staff Scientist: Carl Hergenrother, Lunar & Planetary Laboratory, University of Arizona
- Asteroid Lightcurve Database (LCDB), query form ( info Archived 16 December 2017 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
- 3099 Hergenrother at AstDyS-2, Asteroids—Dynamic Site
- 3099 Hergenrother at the JPL Small-Body Database