160 Una

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160 Una
A three-dimensional model of 160 Una based on its light curve.
Discovery
Discovered byC. H. F. Peters
Discovery date20 February 1876
Designations
(160) Una
Pronunciation/ˈjnə/[1]
Minor planet categoryMain belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc118.30 yr (43209 d)
|{{{apsis}}}|helion}}2.90877 astronomical unit|AU (435.146 Gm)
|{{{apsis}}}|helion}}2.54727 AU (381.066 Gm)
2.72802 AU (408.106 Gm)
Eccentricity0.066257
Orbital period4.51 yr (1645.8 d)
Average Orbital speed18.01 km/s
Mean anomaly144.472°
Mean motion0° 13m 7.471s / day
Inclination3.82512°
Longitude of ascending node8.60989°
52.8418°
Earth MOID1.56031 AU (233.419 Gm)
Jupiter MOID2.30107 AU (344.235 Gm)
TJupiter3.349
Physical characteristics
Dimensions81.24±2.1 km
Mass5.6×1017 kg (assumed)
Mean density2.0? g/cm3
Equatorial surface gravity
0.0227 m/s2
Equatorial escape velocity
0.0429 km/s
Rotation period11.033 h (0.4597 d)[2]
0.234 d (5.61 h)[3][4]
Geometric albedo0.0625±0.003[2]
0.063[5]
Physics~170 K
C[6]
Absolute magnitude (H)9.08,[2] 8.95[7]


160 Una is a fairly large and dark, primitive main belt asteroid that was discovered by German-American astronomer C. H. F. Peters on February 20, 1876, in Clinton, New York.[8] It is named after a character in Edmund Spenser's epic poem The Faerie Queene (1590). This minor planet is orbiting the Sun at a distance of 2.73 astronomical unit|AU with an eccentricity of 0.07. The orbital plane is inclined at an angle of 3.83° to the plane of the ecliptic.[2]

In the Tholen classification system it is categorized as a CX-type, while the Bus asteroid taxonomy system lists it as an Xk asteroid.[9] Photometric observations of this asteroid made at the Torino Observatory in Italy during 1990–1991 were used to determine a synodic rotation period of 5.61 ± 0.01 hours.[3] It has an estimated diameter of about 81 km.

References

  1. Benjamin Smith (1903) The Century Dictionary and Cyclopedia
  2. 2.0 2.1 2.2 2.3 2.4 Yeomans, Donald K., "160 Una", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=160, retrieved 12 May 2016. 
  3. 3.0 3.1 di Martino, M. et al. (February 1994), "Lightcurves and rotational periods of nine main belt asteroids", Icarus 107 (2): 269–275, doi:10.1006/icar.1994.1022, Bibcode1994Icar..107..269D. 
  4. "Lightcurves and map data on numbered asteroids N° 1 to 52225". Archived on 2005-11-27. Error: If you specify |archivedate=, you must also specify |archiveurl=. http://www.astrosurf.com/aude-old/map_files/AstVarMAP01-2003.htm. Retrieved 2008-11-03. 
  5. "Infrared Astronomical Satellite (IRAS)". Archived from the original on 2005-02-24. https://web.archive.org/web/20050224095554/http://dorothy.as.arizona.edu/DSN/IRAS/index_iras.html. Retrieved 2005-02-24. 
  6. Asteroid Lightcurve Data File, Updated March 1, 2001
  7. Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin 34 (4): 113–119, Bibcode2007MPBu...34..113W. 
  8. "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), https://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html, retrieved 2013-04-07. 
  9. DeMeo, Francesca E. et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared", Icarus 202 (1): 160–180, doi:10.1016/j.icarus.2009.02.005, Bibcode2009Icar..202..160D, archived from the original on 2014-03-17, https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf, retrieved 2013-04-08.  See appendix A.





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