English

Col-OSSOS: The Colours of the Outer Solar System Origins Survey

Earth and Planetary Astrophysics 2019-07-17 v2

Abstract

The Colours of the Outer Solar System Origins Survey (Col-OSSOS) is acquiring near-simultaneous gg, rr, and JJ photometry of unprecedented precision with the Gemini North Telescope, targeting nearly a hundred trans-Neptunian objects (TNOs) brighter than mr=23.6m_r=23.6 mag discovered in the Outer Solar System Origins Survey. Combining the optical and near-infrared photometry with the well-characterized detection efficiency of the Col-OSSOS target sample will provide the first flux-limited compositional dynamical map of the outer Solar System. In this paper, we describe our observing strategy and detail the data reduction processes we employ, including techniques to mitigate the impact of rotational variability. We present optical and near-infrared colors for 35 TNOs. We find two taxonomic groups for the dynamically excited TNOs, the neutral and red classes, which divide at gr0.75g-r \simeq 0.75. Based on simple albedo and orbital distribution assumptions, we find that the neutral class outnumbers the red class, with a ratio of 4:1 and potentially as high as 11:1. Including in our analysis constraints from the cold classical objects, which are known to exhibit unique albedos and rzr-z colors, we find that within our measurement uncertainty, our observations are consistent with the primordial Solar System protoplanetesimal disk being neutral-class-dominated, with two major compositional divisions in grJgrJ color space.

Keywords

Cite

@article{arxiv.1809.08501,
  title  = {Col-OSSOS: The Colours of the Outer Solar System Origins Survey},
  author = {Megan E. Schwamb and Wesley C. Fraser and Michele T. Bannister and Michael Marsset and Rosemary E. Pike and J. J. Kavelaars and Susan D. Benecchi and Matthew J. Lehner and Shiang-Yu Wang and Audrey Thirouin and Audrey Delsanti and Nuno Peixinho and Kathryn Volk and Mike Alexandersen and Ying-Tung Chen and Brett Gladman and Stephen D. J. Gwyn and Jean-Marc Petit},
  journal= {arXiv preprint arXiv:1809.08501},
  year   = {2019}
}

Comments

Accepted to ApJS; on-line supplemental files will be available with the AJS published version of the paper