Astronomy:162 Laurentia

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Short description: Main-belt asteroid
162 Laurentia
162Laurentia (Lightcurve Inversion).png
A three-dimensional model of 162 Laurentia based on its light curve.
Discovery
Discovered byPaul Henry and Prosper Henry
Discovery siteParis
Discovery date21 April 1876
Designations
(162) Laurentia
Pronunciation/lɒˈrɛnʃiə/[1]
Named afterJoseph Jean Pierre Laurent
A876 HB
Minor planet categorymain belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.88 yr (41596 d)
|{{{apsis}}}|helion}}3.5574 astronomical unit|AU (532.18 Gm)
|{{{apsis}}}|helion}}2.4779 AU (370.69 Gm)
3.0177 AU (451.44 Gm)
Eccentricity0.17887
Orbital period5.24 yr (1914.7 d)
Mean anomaly300.020°
Mean motion0° 11m 16.872s / day
Inclination6.0977°
Longitude of ascending node35.539°
116.277°
Earth MOID1.49465 AU (223.596 Gm)
Jupiter MOID1.47116 AU (220.082 Gm)
TJupiter3.214
Physical characteristics
Dimensions99.10±2.6 km
Rotation period11.8686 h (0.49453 d)[2][3]
Geometric albedo0.0529±0.003
C
Absolute magnitude (H)8.83


162 Laurentia is a large and dark main-belt asteroid that was discovered by the French brothers Paul Henry and Prosper Henry on 21 April 1876, and named after Joseph Jean Pierre Laurent, an amateur astronomer who discovered asteroid 51 Nemausa.

An occultation by Laurentia was observed from Clive, Alberta on 21 November 1999.[citation needed]

Photometric observations of this asteroid from multiple observatories during 2007 gave a light curve with a period of 11.8686 ± 0.0004 hours and a brightness variation of 0.40 ± 0.05 in magnitude. This is in agreement with previous studies in 1994 and 2007.[3]

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
    Laurentian (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Laurentian  (Subscription or UK public library membership required.)
  2. 2.0 2.1 Yeomans, Donald K., "162 Laurentia", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=162, retrieved 12 May 2016. 
  3. 3.0 3.1 Oey, Julian; Krajewski, Ric (June 2008), "Lightcurve Analysis of Asteroids from Kingsgrove and Other Collaborating Observatories in the First Half of 2007", The Minor Planet Bulletin 35 (2): pp. 47–48, Bibcode2008MPBu...35...47O. 

External links