High-resolution Search for Kuiper Belt Object Binaries from New Horizons

Using the New Horizons LOng Range Reconnaissance Imager camera, we searched for satellites near five Kuiper Belt objects (KBOs): four cold classicals (CCs: 2011 JY(31), 2014 OS393, 2014 PN70, 2011 HZ(102)) and one scattered disk (SD) object (2011 HK103). These objects were observed at distances of 0.092-0.290 au from the New Horizons spacecraft, achieving spatial resolutions of 136-430 km (resolution similar to 2 camera pixels), much higher than possible from any other facilities. Here we report that CC 2011 JY(31) is a binary system with roughly equal brightness components, CC 2014 OS393 is likely an equal-brightness binary system, while the three other KBOs did not show any evidence of binarity. The JY(31) binary has a semimajor axis of 198.6 +/- 2.9 km, an orbital inclination of 61.degrees 34 +/- 1.degrees 34, and an orbital period of 1.940 +/- 0.002 days. The OS393 binary objects have an apparent separation of similar to 150 km, making JY(31) and OS393 the tightest KBO binary systems ever resolved. Both HK103 and HZ(102) were detected with a signal-to-noise ratio (S/N) approximate to 10, and our observations rule out equal-brightness binaries with separations larger than similar to 430 km and similar to 260 km, respectively. The spatial resolution for PN70 was similar to 200 km, but this object had a S/N approximate to 2.5-3, which limited our ability to probe its binarity. The binary frequency for the CC binaries probed in our small survey (67%, not including PN70) is consistent with the high binary frequency suggested by larger surveys of CCs and recent planetesimal formation models, but we extend the results to smaller orbit semimajor axes and smaller objects than previously possible.

Automated summary

Using the New Horizons LOng Range Reconnaissance Imager camera, binary systems were discovered near two Kuiper Belt objects. These findings are significant for studying planetesimal formation models and the characteristics of small celestial bodies.