The Planetary Science Journal (Jan 2021)

The Sizes and Albedos of Centaurs 2014 YY49 and 2013 NL24 from Stellar Occultation Measurements by RECON

  • Ryder H. Strauss,
  • Rodrigo Leiva,
  • John M. Keller,
  • Elizabeth Wilde,
  • Marc W. Buie,
  • Robert J. Weryk,
  • JJ Kavelaars,
  • Terry Bridges,
  • Lawrence H. Wasserman,
  • David E. Trilling,
  • Deanna Ainsworth,
  • Seth Anthony,
  • Robert Baker,
  • Jerry Bardecker,
  • James K Bean Jr.,
  • Stephen Bock,
  • Stefani Chase,
  • Bryan Dean,
  • Chessa Frei,
  • Tony George,
  • Harnoorat Gill,
  • H. Wm. Gimple,
  • Rima Givot,
  • Samuel E. Hopfe,
  • Juan M. Cota Jr.,
  • Matthew Kehrli,
  • Rebekah King,
  • Sean L. Haley,
  • Charisma Lara,
  • Nels Lund,
  • Martin L. Mattes,
  • Keitha McCandless,
  • Delsie McCrystal,
  • Josh McRae,
  • Leonardo Emmanuel Rodriguez Melgarejo,
  • Paola Mendoza,
  • Alexandra Miller,
  • Ian R. Norfolk,
  • Bruce Palmquist,
  • Robert D. Reaves,
  • Megan L Rivard,
  • Michael von Schalscha,
  • Ramsey Schar,
  • Timothy J Stoffel,
  • Diana J. Swanson,
  • Doug Thompson,
  • J. A. Wise,
  • Levi Woods,
  • Yuehai Yang

DOI
https://doi.org/10.3847/PSJ/abd62a
Journal volume & issue
Vol. 2, no. 1
p. 22

Abstract

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In 2019, the Research and Education Collaborative Occultation Network (RECON) obtained multiple-chord occultation measurements of two Centaur objects: 2014 YY _49 on 2019 January 28 and 2013 NL _24 on 2019 September 4. RECON is a citizen-science telescope network designed to observe high-uncertainty occultations by outer solar system objects. Adopting circular models for the object profiles, we derive a radius $r={16}_{-1}^{+2}$ km and a geometric albedo ${p}_{V}={0.13}_{-0.024}^{+0.015}$ for 2014 YY _49 and a radius $r={66}_{-5}^{+5}$ km and a geometric albedo ${p}_{V}={0.045}_{-0.008}^{+0.006}$ for 2013 NL _24 . To the precision of these measurements, no atmosphere or rings are detected for either object. The two objects measured here are among the smallest distant objects measured with the stellar occultation technique. In addition to these geometric constraints, the occultation measurements provide astrometric constraints for these two Centaurs at a higher precision than has been feasible by direct imaging. To supplement the occultation results, we also present an analysis of color photometry from the Pan-STARRS surveys to constrain the rotational light curve amplitudes and spectral colors of these two Centaurs. We recommend that future work focus on photometry to more deliberately constrain the objects’ colors and light curve amplitudes and on follow-on occultation efforts informed by this astrometry.

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