P/2003 T12 is a periodic comet that revolves around the Sun once every 4.11 years. On 13 January 2012, it was observed by the satellite STEREO-B, and the most documented phase of P/2003 T12 was observed on that date. It is hypothesized to be a possible fragment of comet 169P/NEAT. It will reach perihelion in August 2028.
12 January 2012 event During its apparition on 12 January 2012, it ventured into the highest phase angle ever observed for a comet, and the forward-scattering enhancement in brightness was marked, as large as ~8.5 mag. This has given insight into Henyey-Greenstein (HG) space-dust.
References
External links P/2003 T12 at the JPL Small-Body Database
