Orbital Characterization of a Newly Discovered Small Satellite around Quaoar

Abstract Recent observations of a stellar occultation have revealed the presence of a previously undiscovered small satellite around Quaoar. Orbiting near Quaoar’s unusual ring system, this new satellite has the potential to provide significant insights into the formation and evolution of Quaoar and its ring system. In this Letter, we characterize the orbit of this newly discovered satellite, finding that it is likely on a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mn>3</mml:mn> <mml:mo>.</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>6</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.3</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.5</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> day orbit, plausibly placing it near a 5:3 mean motion resonance with Quaoar’s outermost known ring. Examining the possibility of observing the newly discovered satellite with further stellar occultations, we estimate that ∼hundreds of observing stations are required for recovery, since phase information about its orbit was rapidly lost after the lone detection. We also attempted to recover the satellite in JWST NIRCam imaging of Quaoar, but find no convincing detection. This nondetection is limited by the accuracy of the available NIRCam point-spread function models, as well as the satellite’s extreme faintness and close-in orbital separation. Therefore, current-generation telescopes will likely struggle to directly image this new satellite, but near-future 30 m class telescopes should prove capable of detecting it. Discovery of such a satellite provides evidence that the rings around Quaoar may have been part of an initially broad collisional disk that has evolved considerably since its formation. To further explore this hypothesis, we encourage follow-up observations of the rings and satellites with stellar occultations and direct imaging, as well as updated hydrodynamical, collisional, and tidal modeling of the system.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-11-07
DOI
https://doi.org/10.3847/2041-8213/ae1585
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

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article

Orbital Characterization of a Newly Discovered Small Satellite around Quaoar

W. M. Grundy, Charles A. Collyer, Bryan J. Holler, E. Fernández-Valenzuela et al.
The Astrophysical Journal Letters
Stellar, planetary, and galactic studies
article

Orbital Characterization of a Newly Discovered Small Satellite around Quaoar

W. M. Grundy, Charles A. Collyer, Bryan J. Holler, E. Fernández-Valenzuela, Ana Carolina Souza-Feliciano, Benjamin Proudfoot, R. Nolthenius, F. L. Rommel
article en

Abstract

Abstract Recent observations of a stellar occultation have revealed the presence of a previously undiscovered small satellite around Quaoar. Orbiting near Quaoar’s unusual ring system, this new satellite has the potential to provide significant insights into the formation and evolution of Quaoar and its ring system. In this Letter, we characterize the orbit of this newly discovered satellite, finding that it is likely on a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mn>3</mml:mn> <mml:mo>.</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>6</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.3</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.5</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> day orbit, plausibly placing it near a 5:3 mean motion resonance with Quaoar’s outermost known ring. Examining the possibility of observing the newly discovered satellite with further stellar occultations, we estimate that ∼hundreds of observing stations are required for recovery, since phase information about its orbit was rapidly lost after the lone detection. We also attempted to recover the satellite in JWST NIRCam imaging of Quaoar, but find no convincing detection. This nondetection is limited by the accuracy of the available NIRCam point-spread function models, as well as the satellite’s extreme faintness and close-in orbital separation. Therefore, current-generation telescopes will likely struggle to directly image this new satellite, but near-future 30 m class telescopes should prove capable of detecting it. Discovery of such a satellite provides evidence that the rings around Quaoar may have been part of an initially broad collisional disk that has evolved considerably since its formation. To further explore this hypothesis, we encourage follow-up observations of the rings and satellites with stellar occultations and direct imaging, as well as updated hydrodynamical, collisional, and tidal modeling of the system.

The Astrophysical Journal LettersVol. 993(2)
National Aeronautics and Space Administration, Space Telescope Science Institute
Openalex Percentile: Top 77%
Stellar, planetary, and galactic studies
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