Astronomy:160 Una

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Short description: Main-belt asteroid
160 Una
160Una (Lightcurve Inversion).png
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]


Una (minor planet designation: 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).

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]

References

  1. Benjamin Smith (1903) The Century Dictionary and Cyclopedia
  2. 2.0 2.1 2.2 2.3 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.

External links