Astronomy:170 Maria

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Short description: S-type Main-belt asteroid
170 Maria
Asteroid Maria passing near a cluster of galaxies
Asteroid Maria passing near a cluster of galaxies as seen by a four inch telescope over a period of nearly two hours.
Discovery
Discovered byJ. Perrotin
Discovery date10 January 1877
Designations
(170) Maria
Pronunciation/məˈrə/ mə-REE
A877 AA; 1958 AC
Minor planet categoryMain belt (Maria)
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc116.69 yr (42622 d)
|{{{apsis}}}|helion}}2.7161 astronomical unit|AU (406.32 Gm)
|{{{apsis}}}|helion}}2.3923 AU (357.88 Gm)
2.5542 AU (382.10 Gm)
Eccentricity0.063388
Orbital period4.08 yr (1491.0 d)
Mean anomaly88.062°
Mean motion0° 14m 29.184s / day
Inclination14.377°
Longitude of ascending node301.34°
159.21°
Earth MOID1.4114 AU (211.14 Gm)
Jupiter MOID2.39948 AU (358.957 Gm)
TJupiter3.392
Physical characteristics
Dimensions44.30±1.0 km
Rotation period13.120 h (0.5467 d)
Geometric albedo0.1579±0.007
S[2]
Absolute magnitude (H)9.39


Maria (minor planet designation: 170 Maria) is a Main belt asteroid that was discovered by French astronomer Henri Joseph Perrotin on January 10, 1877.[3] Its orbit was computed by Antonio Abetti, and the asteroid was named after his sister, Maria. This is the namesake of the Maria asteroid family; one of the first asteroid families to be identified by Japanese astronomer Kiyotsugu Hirayama in 1918.[4]

In the Tholen classification system, this is categorized as a stony S-type asteroid.[2] Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light curve with a period of 13.120 ± 0.002 hours and a brightness range of 0.21 ± 0.02 in magnitude. Previous measurements from 2000 gave 13.14 and 5.510 hour estimates for the period.[5] Based upon its spectrum, it is classified as an S-type asteroid.

An occultation of a star by Maria was observed from Manitoba, Canada, on June 10, 1997.

References

  1. Yeomans, Donald K., "170 Maria", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=170, retrieved 12 May 2016. 
  2. 2.0 2.1 DeMeo, Francesca E. et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared", Icarus 202 (1): pp. 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.
  3. "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), archived from the original on February 13, 2012, https://web.archive.org/web/20120213005447/http://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html, retrieved 2013-04-07. 
  4. Veeder, G. J. et al. (March 1995), "Eos, Koronis, and Maria family asteroids: Infrared (JHK) photometry", Icarus 114: pp. 186–196, doi:10.1006/icar.1995.1053, Bibcode1995Icar..114..186V, https://trs.jpl.nasa.gov/bitstream/2014/29296/1/95-0212.pdf. 
  5. Warner, Brian D. (September 2007), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory", The Minor Planet Bulletin, Bibcode2007MPBu...34...72W. 

External links