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72 Feronia

From Wikipedia, the free encyclopedia
Main-belt asteroid

72 Feronia
A three-dimensional model of 72 Feronia based on its light curve on the tip and an image of 72 Feronia on the bottem.
Discovery
Discovered byChristian Heinrich Friedrich Peters
Discovery dateMay 29, 1861
Designations
(72) Feronia
Pronunciation/fɛˈrniə/[1]
Named after
Feronia
Main belt
AdjectivesFeronian
Orbital characteristics
Epoch December 31, 2006 (JD 2454100.5)
Aphelion2.539 AU (379.8 Gm)
Perihelion1.993 AU (298.1 Gm)
2.266 AU (339.0 Gm)
Eccentricity0.121
1,246.123 days (3.41 a)
146.950°
Inclination5.417°
208.137°
102.608°
Physical characteristics
Dimensions83.95±4.02 km[2]
Mass(9.45 ± 3.76/1.75)×1017 kg[3]
3.045 ± 1.212/0.565 g/cm3[3]
8.09068 h[4]
−39 or −55[4]
287 or 102[4]
0.063[5]
TDG[6]
8.94

72 Feronia is a quite large and darkmain beltasteroid. It was the first asteroid discovery byC. H. F. Peters, on May 29, 1861,[7] fromHamilton College,New York State. It was initially thought that Peters had merely seen the already known asteroid66 Maja, butT.H. Safford showed that it was a new body. Safford named it afterFeronia, aRomanfertility goddess.[8]

This asteroid is orbiting theSun with aperiod of 3.41 years, having asemimajor axis of2.266 AU and aneccentricity of 0.121. Theorbital plane is inclined by an angle of 5.4° to theplane 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

[edit]
  1. ^Noah Webster (1884)A Practical Dictionary of the English Language
  2. ^Carry, B. (December 2012), "Density of asteroids",Planetary and Space Science, vol. 73, pp. 98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009. See Table 1.
  3. ^abFienga, 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.
  4. ^abcHanuš, J.; et al. (September 2013), "Sizes of main-belt asteroids by combining shape models and Keck adaptive optics observations",Icarus,226 (1): 1045−1057,arXiv:1308.0446,Bibcode:2013Icar..226.1045H,doi:10.1016/j.icarus.2013.07.023.
  5. ^"Asteroid Data Sets". Archived fromthe original on 17 December 2009. Retrieved13 January 2007.
  6. ^*JPL Small-Body Database Browser
  7. ^Sheehan, William (1999), "Christian Heinrich Friedrich Peters",Biographical Memoirs, vol. 76, National Academies Press, p. 289,ISBN 0309064341.
  8. ^Schmadel, Lutz (2003).Dictionary of minor planet names (fifth ed.). Germany: Springer. p. 22.ISBN 3-540-00238-3. Retrieved31 December 2008.

External links

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