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847 Agnia

From Wikipedia, the free encyclopedia
Main-belt asteroid

847 Agnia
A three-dimensional model of 847 Agnia based on its light curve
Discovery
Discovered byG. N. Neujmin
Discovery siteSimeis
Discovery date2 September 1915
Designations
(847) Agnia
1915 XX
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc109.53 yr (40006 d)
Aphelion3.0472 AU (455.85 Gm)
Perihelion2.5158 AU (376.36 Gm)
2.7815 AU (416.11 Gm)
Eccentricity0.095516
4.64yr (1694.4d)
208.04°
0° 12m 44.892s / day
Inclination2.4817°
270.935°
130.341°
Earth MOID1.52345 AU (227.905 Gm)
Jupiter MOID2.31009 AU (345.585 Gm)
TJupiter3.325
Physical characteristics
14.02±0.85km
14.827 h (0.6178 d)
0.1720±0.022
10.29

847 Agnia is aminor planet orbiting theSun. It is approximately 28 kilometers in diameter.[2]

The spectrum of this object indicates that it is anS-type asteroid with both low and highcalcium forms ofpyroxene on the surface, along with less than 20%olivine. The high-calcium form of pyroxene forms 40% or more of the total pyroxene present, indicating a history ofigneous rock deposits. This suggests that theasteroid underwent differentiation by melting, creating a surface ofbasalt rock.[3]

847 Agnia is the namesake of theAgnia family of asteroids that share similarorbital elements and physical properties. The members of this family, including 847 Agnia, most likely formed from the breakup of abasalt object, which in turn was spawned from a larger parent body that had previously undergoneigneous differentiation. Other members of this family include1020 Arcadia,1228 Scabiosa,2401 Aehlita, and3395 Jitka[3]

Photometric observations of this asteroid collected during 2004–2005 show arotation period of 14.827 ± 0.001 hours with a brightness variation of 0.45 ± 0.03magnitude.[4]

References

[edit]
  1. ^"847 Agnia (1915 XX)".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved4 May 2016.
  2. ^IOTA/IOTA-ES occultation update for (847) Agnia[dead link]
  3. ^abSunshine, Jessica M.; et al. (August 2004), "High-calcium pyroxene as an indicator of igneous differentiation in asteroids and meteorites",Meteoritics & Planetary Science, vol. 39, no. 8, pp. 1343–1357,Bibcode:2004M&PS...39.1343S,doi:10.1111/j.1945-5100.2004.tb00950.x.
  4. ^Pray, Donald P. (September 2005), "Lightcurve analysis of asteroids 106, 752, 847, 1057, 1630, 1670, 1927 1936, 2426, 2612, 2647, 4087, 5635, 5692, and 6235",The Minor Planet Bulletin,32 (3):48–51,Bibcode:2005MPBu...32...48P.

External links

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