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11118 Modra

From Wikipedia, the free encyclopedia
Main-belt Flora asteroid

11118 Modra
Discovery[1]
Discovered byA. Galád
D. Kalmančok
Discovery siteModra Obs.
Discovery date9 August 1996
Designations
(11118) Modra
Named after
Modra
(town andobservatory)[2]
1996 PK · 1991 FL1
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc25.44 yr (9,291 days)
Aphelion2.5052AU
Perihelion2.1225 AU
2.3139 AU
Eccentricity0.0827
3.52yr (1,286 days)
139.39°
0° 16m 48s / day
Inclination3.0326°
7.4717°
204.63°
Physical characteristics
Dimensions3.74 km(calculated)[3]
8.69±3.13 km[4]
27.12±0.02h[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 designation1996 PK) is a Floraasteroid of uncertain composition from the inner regions of theasteroid belt, approximately 5 kilometers in diameter.

It was discovered on 9 August 1996, by Slovak astronomersAdrián Galád andDušan Kalmančok at theModra Observatory in Slovakia, and named for the townModra where the discovering observatory is located.[2][8]

Classification and orbit

[edit]

Modra is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 2.1–2.5 AU once every 3 years and 6 months (1,286 days). Its orbit has aneccentricity of 0.08 and aninclination of 3° with respect to theecliptic.[1] A firstprecovery was taken at ESO'sLa Silla Observatory in 1991, extending the asteroid'sobservation arc by 5 years prior to its discovery.[8]

Rotation period

[edit]

In September 2010, a photometriclightcurve analysis of Modra by American astronomerBrian Warner at his Palmer Divide Observatory, Colorado, rendered an unambiguousperiod of27.12±0.02 hours with a brightness variation of 0.53 inmagnitude (U=3).[5] A second lightcurve obtained during the wide-field survey at the U.S.Palomar Transient Factory in August 2010, and gave a period of27.1481±0.0409 hours with an amplitude of 0.42 (U=2).[6]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer and its subsequentNEOWISE mission, the asteroid has a lowalbedo of 0.05.[4] In agreement, the large-scale survey byPan-STARRS (PS1) rates it as a darkcarbonaceous body.[7] However, theCollaborative Asteroid Lightcurve Link (CALL) assumes a much higher albedo of 0.24 – derived from8 Flora, the orbital family's largest member and namesake – and groups it to theS-type asteroid.[3] The different albedos of the twospectral 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]

Naming

[edit]

Thisminor planet was named after both the small historical town ofModra, located in the Bratislava Region of Slovakia, and theModra Observatory of the Institute of Astronomy at Comenius University, where this asteroid had been discovered.[2] The approved naming citation was published by theMinor Planet Center on 28 September 1999 (M.P.C. 36130).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 11118 Modra (1996 PK)" (2016-08-23 last obs.).Jet Propulsion Laboratory. Retrieved5 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(11118) Modra".Dictionary of Minor Planet Names – (11118) Modra.Springer Berlin Heidelberg. p. 753.doi:10.1007/978-3-540-29925-7_8231.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (11118) Modra". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^abcdeMasiero, 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. Retrieved17 May 2016.
  5. ^abWarner, 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. Retrieved17 May 2016.
  6. ^abcWaszczak, 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. Retrieved17 May 2016.
  7. ^abcVeres, 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. Retrieved17 May 2016.
  8. ^ab"11118 Modra (1996 PK)".Minor Planet Center. Retrieved25 January 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
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