Astronomy:72 Feronia

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72 Feronia
A three-dimensional model of 72 Feronia based on its light curve on the top and an image of 72 Feronia on the bottom.
Discovery
Discovered byChristian Heinrich Friedrich Peters
Discovery date29 May 1861
Designations
(72) Feronia
Pronunciation/fɛˈroʊniə/[1]
Named afterFeronia
Minor planet categoryMain belt
AdjectivesFeronian
Orbital characteristics[2]
Epoch 9 June 2026 (JD 2461200.5)
Uncertainty parameter 0
|{{{apsis}}}|helion}}2.541 astronomical unit|AU (380.1 Gm)
|{{{apsis}}}|helion}}1.991 AU (297.8 Gm)
2.266 AU (339.0 Gm)
Eccentricity0.121
Orbital period1,245.87 days (3.41 a)
Mean anomaly38.122°
Inclination5.418°
Longitude of ascending node207.925°
102.678°
Jupiter MOID2.677 AU
TJupiter3.601
Physical characteristics
Dimensions83.95±4.02 km[3]
Mass(9.45 ± 3.76/1.75)×1017 kg[4]
Mean density3.045 ± 1.212/0.565 g/cm3[4]
Rotation period8.09068 h[5]
Pole ecliptic latitude287 or 102[5]
Pole ecliptic longitude−39 or −55[5]
Geometric albedo0.063[6]
TDG[7]
Absolute magnitude (H)8.94


72 Feronia is a quite large and dark main belt asteroid. It was the first asteroid discovery by C. H. F. Peters, on 29 May 1861,[8] from Hamilton College, New York State. It was initially thought that Peters had merely seen the previously discovered asteroid 66 Maja, but T.H. Safford showed that it was a new body. Safford named it after Feronia, a Roman fertility goddess.[9]

This asteroid is orbiting the Sun with a period of 3.41 years, having a semi-major axis of 2.266 astronomical unit|AU and an eccentricity of 0.121. The orbital plane is inclined by an angle of 5.4° to the plane of the ecliptic. This is a spectral type TDG asteroid with a cross-section size of 84 km. The asteroid has an estimated rotation period of 8.09 h. Hanuš et al. (2013) gives two possible solutions for the pole in ecliptic coordinates: (λ1, β1) = (287°, −39°) or (λ1, β1) = (102°, −55°).

References

  1. ↑ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ↑ 2.0 2.1 "JPL Small-Body Database Lookup: 72 Feronia". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=72. 
  3. ↑ 3.0 3.1 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode: 2012P&SS...73...98C.  See Table 1.
  4. ↑ 4.0 4.1 4.2 Fienga, A.; Avdellidou, C.; Hanuš, J. (February 2020). "Asteroid masses obtained with INPOP planetary ephemerides". Monthly Notices of the Royal Astronomical Society 492 (1). doi:10.1093/mnras/stz3407. https://academic.oup.com/mnras/article/492/1/589/5658701. 
  5. ↑ 5.0 5.1 5.2 5.3 Hanuš, J. et al. (September 2013), "Sizes of main-belt asteroids by combining shape models and Keck adaptive optics observations", Icarus 226 (1): 1045−1057, doi:10.1016/j.icarus.2013.07.023, Bibcode: 2013Icar..226.1045H. 
  6. ↑ "Asteroid Data Sets". http://www.psi.edu/pds/resource/albedo.html. 
  7. ↑ *JPL Small-Body Database Browser
  8. ↑ 8.0 8.1 Sheehan, William (1999), "Christian Heinrich Friedrich Peters", Biographical Memoirs, 76, National Academies Press, p. 289, ISBN 0309064341, https://books.google.com/books?id=4D-OIyTLoO0C&oi=fnd&pg=PA289. 
  9. ↑ Schmadel, Lutz (2003). Dictionary of minor planet names (fifth ed.). Germany: Springer. p. 22. ISBN 3-540-00238-3. https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA22. Retrieved 2008-12-31.