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17119 Alexisrodrz

From Wikipedia, the free encyclopedia
Main-belt asteroid

17119 Alexisrodrz
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date10 May 1999
Designations
(17119) Alexisrodrz
Named after
Alexis Rodriguez
(2003ISEF awardee)[2]
1999 JP59 · 1998 BY48
main-belt · (middle)[3]
background
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc23.68 yr (8,649 days)
Aphelion2.7912AU
Perihelion2.4851 AU
2.6381 AU
Eccentricity0.0580
4.29yr (1,565 days)
34.066°
0° 13m 48s / day
Inclination6.3433°
160.73°
150.73°
Physical characteristics
Dimensions3.917±0.732 km[4][5]
4.56 km(calculated)[3]
17.7838±0.0290h[6]
17.7935 h[3]
0.10(assumed)[3]
0.182±0.080[5]
0.1825±0.0798[4]
LS[7] · S/C[3]
14.4[1] · 14.22±0.28[7] · 14.5[4] · 14.317±0.005(R)[6] · 14.82[3]

17119 Alexisrodrz (provisional designation1999 JP59) is a stony backgroundasteroid from the central region of theasteroid belt, approximately 4 kilometers in diameter.

It was discovered on 10 May 1999, by theLINEAR team at theLincoln Laboratory's Experimental Test Site in Socorro, New Mexico, United States.[8] The asteroid was later named for Alexis Rodriguez, a 2003-awardee of theIntel International Science and Engineering Fair.[2]

Orbit and classification

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Alexisrodrz orbits the Sun in thecentral main-belt at a distance of 2.5–2.8 AU once every 4 years and 3 months (1,565 days). Its orbit has aneccentricity of 0.06 and aninclination of 6° with respect to theecliptic.[1]

The asteroid'sobservation arc begins 7 years prior to its official discovery observation, with aprecovery taken atSteward Observatory (Kitt Peak) in November 1992.[8]

Physical characteristics

[edit]

Alexisrodrz has been characterized as a LS-subtype byPan-STARRS' large-scale survey.[7] This subtype is a transitional group from the common stonyS-type to the rare and reddishL-type asteroids.

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer, Alexisrodrz measures 3.9 kilometers in diameter and its surface has analbedo of 0.18,[4] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 – a compromise value between thestony (0.20) andcarbonaceous (0.057) asteroids found in the 2.6 to 2.7 AU region of the asteroid belt – and calculates a diameter of 4.6 kilometers with anabsolute magnitude of 14.82.[3]

Rotation period

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In January 2011, and September 2013, two rotationallightcurves of Alexisrodrz were obtained from photometric observations made by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave a concurringrotation period of17.7838 and17.7935 hours with a brightness variation of 0.48 and 0.60magnitude, respectively (U=2/2).[6]

Naming

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Thisminor planet was named for the 3rd-place winner of the 2003Intel International Science and Engineering Fair, Alexis Rodriguez (born 1986). At the time, he attended the Puerto RicanAurea E. Quiles Claudio High School in Guanica.[2] The approved naming citation was published by theMinor Planet Center on 14 June 2004 (M.P.C. 52172).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 17119 Alexisrodrz (1999 JP59)" (2016-07-25 last obs.).Jet Propulsion Laboratory. Retrieved26 June 2017.
  2. ^abcSchmadel, Lutz D. (2006). "(17119) Alexisrodrz [2.64, 0.06, 6.3]".Dictionary of Minor Planet Names – (17119) Alexisrodrz, Addendum to Fifth Edition: 2003–2005.Springer Berlin Heidelberg. p. 106.doi:10.1007/978-3-540-34361-5_1129.ISBN 978-3-540-34360-8.
  3. ^abcdefg"LCDB Data for (17119) Alexisrodrz". Asteroid Lightcurve Database (LCDB). Retrieved10 May 2016.
  4. ^abcdMainzer, 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. Retrieved10 May 2016.
  5. ^abMasiero, 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. Retrieved3 December 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. Retrieved10 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. Retrieved10 May 2016.
  8. ^ab"17119 Alexisrodrz (1999 JP59)".Minor Planet Center. Retrieved10 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 May 2016.

External links

[edit]
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