11118 Modra
| Discovery [1] | |
|---|---|
| Discovered by |
A. Galád D. Kalmančok |
| Discovery site | Modra Obs. |
| Discovery date | 9 August 1996 |
| Designations | |
| MPC designation | 11118 Modra |
Named after |
Modra (town and observatory)[2] |
| 1996 PK · 1991 FL1 | |
| main-belt · Flora [3] | |
| Orbital characteristics [1] | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 25.23 yr (9,216 days) |
| Aphelion | 2.5049 AU |
| Perihelion | 2.1221 AU |
| 2.3135 AU | |
| Eccentricity | 0.0827 |
| 3.52 yr (1,285 days) | |
| 83.483° | |
| 0° 16m 48.36s / day | |
| Inclination | 3.0328° |
| 7.4695° | |
| 204.53° | |
| Physical characteristics | |
| Dimensions |
3.74 km (calculated)[3] 8.69±3.13 km[4] |
|
27.12±0.02 h[5] 27.1481±0.0409 h[6] | |
|
0.054±0.105[4] 0.24 (assumed)[3] | |
| S [3] · C [7] | |
| 14.3[1][3] · 14.211±0.005 (R)[6] · 14.17±0.36[7] · 14.10[4] | |
|
| |
11118 Modra, provisional designation 1996 PK, is a Flora asteroid of uncertain composition from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 9 August 1996, by Slovak astronomers Adrián Galád and Dušan Kalmančok at the Modra Observatory in Slovakia.[8]
It is a member of the Flora family, one of the largest orbital groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.1–2.5 AU once every 3 years and 6 months (1,285 days). Its orbit has an eccentricity of 0.08 and an inclination of 3° with respect to the ecliptic.[1] The first precovery was taken at ESO's La Silla Observatory in 1991, extending the asteroid's observation arc by 5 years prior to its discovery.[8]
In September 2010, a photometric light-curve analysis by American astronomer Brian Warner at his U.S. Palmer Divide Observatory in Colorado, rendered an unambiguous period of 27.12±0.02 hours with a brightness variation of 0.53 in magnitude (U=3).[5] A second light-curve obtained from the wide-field survey at the U.S. Palomar Transient Factory in August 2010, gave a period of 27.1481±0.0409 hours with an amplitude of 0.42 (U=2).[6]
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, the asteroid has a low albedo of 0.05.[4] In agreement, the large-scale survey by Pan-STARRS (PS1) rates it as a dark carbonaceous body.[7] However, the Collaborative Asteroid Lightcurve Link (CALL) assumes a much higher albedo of 0.24 – derived from 8 Flora, the orbital family's largest member and namesake – and groups it to the S-type asteroid.[3] The different albedos of the two spectral classes also translate into divergent estimates for the body's diameter. While CALL calculates 3.7 kilometers, NASA's space-based survey inferred a much larger diameter of 8.7 kilometers.[3][4]
The minor planet was named after both the small historical town of Modra, located in the Bratislava Region of Slovakia, and the Modra Observatory of the Institute of Astronomy at Comenius University, where this asteroid had been discovered.[2] Naming citation was published on 28 September 1999 (M.P.C. 36130).[9]
References
- 1 2 3 4 "JPL Small-Body Database Browser: 11118 Modra (1996 PK)" (2016-06-09 last obs.). Jet Propulsion Laboratory. Retrieved 4 December 2016.
- 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (11118) Modra. Springer Berlin Heidelberg. p. 753. ISBN 978-3-540-00238-3. Retrieved 25 January 2016.
- 1 2 3 4 5 6 7 "LCDB Data for (11118) Modra". Asteroid Lightcurve Database (LCDB). Retrieved 17 May 2016.
- 1 2 3 4 5 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. Retrieved 17 May 2016. - 1 2 Warner, Brian D. (April 2011). "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2010 September-December". The Minor Planet Bulletin. 38 (2): 82–86. Bibcode:2011MPBu...38...82W. ISSN 1052-8091. Retrieved 17 May 2016.
- 1 2 3 Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 17 May 2016.
- 1 2 3 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. Retrieved 17 May 2016.
- 1 2 "11118 Modra (1996 PK)". Minor Planet Center. Retrieved 25 January 2016.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 17 May 2016.
External links
- The Palmer Divide Observatory: Tour given by Brian Warner on YouTube (time 4:03 min.)
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
- 11118 Modra at the JPL Small-Body Database
