Astronomy:119 Althaea

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Short description: Main-belt asteroid
119 Althaea
119Althaea (Lightcurve Inversion).png
A three-dimensional model of 119 Althaea based on its light curve.
Discovery
Discovered byJames Craig Watson
Discovery date3 April 1872
Designations
(119) Althaea
Pronunciation/ælˈθə/[1]
Named afterAlthaea
A872 GA; 1972 KO
Minor planet categoryMain belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc143.99 yr (52593 d)
|{{{apsis}}}|helion}}2.7896 astronomical unit|AU (417.32 Gm)
|{{{apsis}}}|helion}}2.37335 AU (355.048 Gm)
2.58147 AU (386.182 Gm)
Eccentricity0.080623
Orbital period4.15 yr (1515.0 d)
Average Orbital speed18.51 km/s
Mean anomaly114.868°
Mean motion0° 14m 15.472s / day
Inclination5.7831°
Longitude of ascending node203.674°
170.021°
Earth MOID1.37297 AU (205.393 Gm)
Jupiter MOID2.58409 AU (386.574 Gm)
TJupiter3.413
Physical characteristics
Dimensions57.30±1.1 km
Mass2.0×1017 kg
Equatorial surface gravity
0.0160 m/s2
Equatorial escape velocity
0.0303 km/s
Rotation period11.484 h (0.4785 d)[2][3]
Geometric albedo0.2306±0.010
Physics~173 K
S
Absolute magnitude (H)8.42


Althaea (minor planet designation: 119 Althaea) is a main-belt asteroid that was discovered by Canadian-American astronomer J. C. Watson on April 3, 1872,[3] and named after Althaea, the mother of Meleager in Greek mythology. Two occultations by Althaea were observed in 2002, only a month apart.

Based upon its spectrum, this is classified as an S-type asteroid.[4] Photometric observations made in 1988 at the Félix Aguilar Observatory produced a light curve with a period of 11.484 ± 0.010 hours with a brightness variation of 0.365 ± 0.010 in magnitude.[3]

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. 2.0 2.1 Yeomans, Donald K., "119 Althaea", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=119, retrieved 12 May 2016. 
  3. 3.0 3.1 3.2 Hutton, R. G. (June 1990), "V+B Photoelectric Photometry of Asteroid 119 Althaea", The Minor Planet Bulletin 17: pp. 15–17, Bibcode1990MPBu...17...15H. 
  4. 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.

External links