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4183 Cuno

From Wikipedia, the free encyclopedia
Asteroid

4183 Cuno
Cuno, imaged by radar
Severalradar images ofCuno
Discovery [1]
Discovered byC. Hoffmeister
Discovery siteBoyden Obs.
Discovery date5 June 1959
Designations
(4183) Cuno
Named after
Cuno Hoffmeister
(astronomer)[2]
1959 LM · 1986 VT7
1987 MB
Apollo · NEO · PHA[1][3]
Mars-crosser
Venus-crosser
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc57.59 yr (21,036 days)
Aphelion3.2396AU
Perihelion0.7248 AU
1.9822 AU
Eccentricity0.6343
2.79yr (1,019 days)
338.28°
0° 21m 11.52s / day
Inclination6.7051°
294.90°
236.34°
Earth MOID0.0283 AU · 11LD
Physical characteristics
2.945±0.115 km[4]
3.73±0.15[5]
3.92 km(calculated)[6]
5.38 km[7]
5.49 km[8]
5.618±0.457 km[9]
3.558±0.002h[10]
3.5590±0.001 h[a]
3.5595 h[b]
0.097±0.025[9][11]
0.10±0.10[12]
0.10[8]
0.11[7]
0.20(assumed)[6]
0.23±0.04[4]
0.36±0.06[4]
SMASS = Sq [1]
Q[13][14][15] · S[6][16]
B–V =0.806±0.013[13]
V–R =0.457±0.008[13]
V–I =0.746±0.009[13]
14.00[16] · 14.01±0.32[15] · 14.35[5] · 14.4[1][4][6][8][9]

4183 Cuno, provisional designation1959 LM, is an eccentric, rare-typeasteroid, classified asnear-Earth object andpotentially hazardous asteroid of theApollo group, and measures approximately 4 kilometers in diameter.

It was discovered on 5 June 1959, by German astronomerCuno Hoffmeister atBoyden Observatory in Bloemfontein, South Africa, and later named in the discoverer's honor.[2][3]

Classification and orbit

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Cuno orbits the Sun at a distance of 0.7–3.2 AU once every 2 years and 9 months (1,019 days). Its orbit has aneccentricity of 0.63 and aninclination of 7° with respect to theecliptic.[1] The body'sobservation arc begins with its identification as1986 VT7, the first used observation made atPalomar Observatory in 1986, approximately 27 years after its official discovery observation at Boyden.[3]

The asteroid has an Earthminimum orbital intersection distance of 0.0283 AU (4,230,000 km), which translates into 11lunar distances.[1]Cuno approaches the Earth to within 40 million kilometers six times in the 21st century. On 20 May 2012, it made its closest Earth approach at a distance of 0.122 AU (18,000,000 km).[17] It will not make a closer approach until 2093 when it will pass Earth at 0.084 AU (13,000,000 km).[17]

Due to its eccentric orbit, it is also aMars andVenus-crosser.[1]

Physical characteristics

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Spectral type and composition

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Cuno is a stonyS-type asteroid.[16] As it has a reflective surface, composed of a mixture differentsilicates, nickel and iron, Cuno has been characterized as a rareQ-type asteroid by the 1-meterJacobus Kapteyn Telescope on La Palma,Pan-STARRS' large-scale magnitude survey, andNASA IRTF telescope.[13][14][15] On theSMASS taxonomic scheme, Cuno is a Sq-subtype, a transitional group between the S and Q types.[1]

Rotation and shape

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Several rotationallightcurves were obtained by Czech astronomerPetr Pravec and American astronomerBrian Warner between 1998 and 2014. Lightcurve analysis gave arotation period of 3.56 hours with a high brightness amplitude between 0.47 and 0.83 inmagnitude, indicating that the body has a non-spheroidal shape.[10][a][b]

In December 2000, Cuno was analysed byradar to determine its shape. The resultant images are lacking in detail, but indicate a rough sphere with some kind of concave depression 1–2 km in diameter.[citation needed]

Diameter and albedo

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Following the space-based surveys carried out by NASA'sSpitzer Space Telescope and theNEOWISE mission of theWide-field Infrared Survey Explorer,Cuno has analbedo between 0.097 and 0.36, and a diameter between 2.945 and 5.618 kilometers.[4][5][7][8][9]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for the stony asteroid of 0.20 and calculates a diameter of 3.9 kilometer with anabsolute magnitude of 14.4, as the higher the body's albedo (reflectivity), the lower its diameter at a constant absolute magnitude (brightness).[6]

Naming

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Thisminor planet was named after its discoverer,Cuno Hoffmeister, according to the established practice to name near-Earth asteroids with a four-letter masculine name.[2] The central main-belt asteroid1726 Hoffmeister, namesake of the Hofmeister family, is also named after the discoverer. The official naming citation was published on 28 May 1991 (M.P.C. 18307).[18]

Notes

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  1. ^abPravec (2000) web: rotation period of3.5590±0.001 hours with a brightness amplitude of0.83 mag. (LCDB quality code = 3). Summary figures for (4183) Cuno atCollaborative Asteroid Lightcurve Link (CALL)
  2. ^abPravec (1998) web: rotation period3.5595 hours with a brightness amplitude of0.7 in magnitude. Call assigns a quality code of 3, which denotes a secure result within the precision given and no ambiguity. Summary figures for (4183) Cuno atCollaborative Asteroid Lightcurve Link (CALL)

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 4183 Cuno (1959 LM)" (2017-01-07 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4183) Cuno".Dictionary of Minor Planet Names – (4183) Cuno.Springer Berlin Heidelberg. p. 358.doi:10.1007/978-3-540-29925-7_4154.ISBN 978-3-540-00238-3.
  3. ^abc"4183 Cuno (1959 LM)".Minor Planet Center. Retrieved1 February 2016.
  4. ^abcdeNugent, 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.
  5. ^abcNugent, 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.
  6. ^abcde"LCDB Data for (4183) Cuno". Asteroid Lightcurve Database (LCDB). Retrieved29 May 2016.
  7. ^abcHarris, A. W.; Mommert, M.; Hora, J. L.; Mueller, M.; Trilling, D. E.; Bhattacharya, B.; et al. (March 2011)."ExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object Survey".The Astronomical Journal.141 (3): 10.Bibcode:2011AJ....141...75H.doi:10.1088/0004-6256/141/3/75.S2CID 14208889.
  8. ^abcdTrilling, D. E.; Mueller, M.; Hora, J. L.; Harris, A. W.; Bhattacharya, B.; Bottke, W. F.; et al. (September 2010)."ExploreNEOs. I. Description and First Results from the Warm Spitzer Near-Earth Object Survey"(PDF).The Astronomical Journal.140 (3):770–784.Bibcode:2010AJ....140..770T.doi:10.1088/0004-6256/140/3/770.S2CID 3006566.
  9. ^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.S2CID 35447010.
  10. ^abWarner, Brian D. (April 2015)."Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2014 October-December".The Minor Planet Bulletin.42 (2):115–127.Bibcode:2015MPBu...42..115W.ISSN 1052-8091.PMC 7244186.PMID 32455352.
  11. ^Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results".The Astrophysical Journal.743 (2): 17.arXiv:1109.6400.Bibcode:2011ApJ...743..156M.doi:10.1088/0004-637X/743/2/156.S2CID 239991.
  12. ^Thomas, C. A.; Trilling, D. E.; Emery, J. P.; Mueller, M.; Hora, J. L.; Benner, L. A. M.; et al. (September 2011)."ExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid Population".The Astronomical Journal.142 (3): 12.Bibcode:2011AJ....142...85T.doi:10.1088/0004-6256/142/3/85.
  13. ^abcdeDandy, C. L.; Fitzsimmons, A.; Collander-Brown, S. J. (June 2003). "Optical colors of 56 near-Earth objects: trends with size and orbit".Icarus.163 (2):363–373.Bibcode:2003Icar..163..363D.doi:10.1016/S0019-1035(03)00087-3.
  14. ^abThomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014). "Physical characterization of Warm Spitzer-observed near-Earth objects".Icarus.228:217–246.arXiv:1310.2000.Bibcode:2014Icar..228..217T.doi:10.1016/j.icarus.2013.10.004.S2CID 119278697.
  15. ^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.S2CID 53493339.
  16. ^abcCarry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry".Icarus.268:340–354.arXiv:1601.02087.Bibcode:2016Icar..268..340C.doi:10.1016/j.icarus.2015.12.047.S2CID 119258489.
  17. ^ab"JPL Close-Approach Data: 4183 Cuno (1959 LM))". Retrieved19 June 2012.
  18. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 May 2016.

External links

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