Recent formation and likely cometary activity of near-Earth asteroid pair 2019 PR2-2019 QR6

Petr Fatka, Nicholas A. Moskovitz, Petr Pravec, Marco Micheli, Maxime Devogèle, Annika Gustafsson, Jay Kueny, Brian Skiff, Peter Kušnirák, Eric Christensen, Judit Ries, Melissa Brucker, Robert Mcmillan, Jeffrey Larsen, Ron Mastaler, Terry Bressi

Research output: Contribution to journalArticlepeer-review

Abstract

Asteroid pairs are genetically related asteroids that recently separated (<few million years), but still reside on similar heliocentric orbits. A few hundred of these systems have been identified, primarily in the asteroid main belt. Here, we studied a newly discovered pair of near-Earth objects (NEOs): 2019 PR2 and 2019 QR6. Based on broad-band photometry, we found these asteroids to be spectrally similar to D-types, a type rare amongst NEOs. We recovered astrometric observations for both asteroids from the Catalina Sky Survey from 2005, which significantly improved their fitted orbits. With these refinements we ran backwards orbital integrations to study formation and evolutionary history. We found that neither a pure gravitational model nor a model with the Yarkovsky effect could explain their current orbits. We thus implemented two models of comet-like non-gravitational forces based on water or CO sublimation. The first model assumed quasi-continuous, comet-like activity after separation, which suggested a formation time of the asteroid pair $300^{+120}_{-70}$ yr ago. The second model assumed short-term activity for up to one heliocentric orbit (∼13.9 yr) after separation, which suggested that the pair formed 272 ± 7 yr ago. Image stacks showed no activity for 2019 PR2 during its last perihelion passage. These results strongly argue for a common origin that makes these objects the youngest asteroid pair known to date. Questions remain regarding whether these objects derived from a parent comet or asteroid, and how activity may have evolved since their separation.

Original languageEnglish (US)
Pages (from-to)6033-6049
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume510
Issue number4
DOIs
StatePublished - Mar 1 2022
Externally publishedYes

Keywords

  • Celestial mechanics
  • Minor planets, asteroids: Individual

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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