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]
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]
^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.
^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.