Based uponphotometric observations taken during 2011, it has a synodicrotation period of 24.052 ± 0.001 h, with a peak-to-peak amplitude of 0.10 ± 0.01 inmagnitude. Because the rotation period nearly matches that of the Earth, it required coordinated observations from multiple observatories at widely spaced latitudes to produce a completelight curve.[4] As discovered in 2021, Pompeja alongside the main-belt asteroid269 Justitia have very red colors due totholins on its surface, similar totrans-Neptunian objects. These asteroids are therefore thought to have formed in the outer Solar System despite their current orbits within the asteroid belt.[5]
^abPilcher, Frederick; et al. (July 2012), "Rotation Period Determination for 203 Pompeja - Another Triumph of Global Collaboration",The Minor Planet Bulletin,39 (3): 99,Bibcode:2012MPBu...39...99P
^Hasegawa, Sunao; Marsset, Michaël; Demeo, Francesca E.; Bus, Schelte J.; Geem, Jooyeon; Ishiguro, Masateru; Im, Myungshin; Kuroda, Daisuke; Vernazza, Pierre (2021), "Discovery of two TNO-like bodies in the asteroid belt",The Astrophysical Journal Letters,916 (1): L6,arXiv:2106.14991,Bibcode:2021ApJ...916L...6H,doi:10.3847/2041-8213/ac0f05,S2CID235669878