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arxiv: 2605.22296 · v1 · pith:7XZQG4VEnew · submitted 2026-05-21 · 🌌 astro-ph.EP

Probing close-in satellites of Trans-Neptunian Objects through thermal and direct size measurements

J. M. G\'omez-Lim\'on , R. Leiva , J. L. Ortiz , P. Santos-Sanz , M. Kretlow , Y. Kilic , J. L. Rizos , A. \'Alvarez-Candal
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T. G. M\"uller
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Pith reviewed 2026-05-22 02:49 UTC · model grok-4.3

classification 🌌 astro-ph.EP
keywords Trans-Neptunian objectsbinary systemsthermal emissionstellar occultationssatellite detectionHerschel Space Observatory
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The pith

Thermal excess beyond occultation sizes points to close-in satellites around three trans-Neptunian objects.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper develops a method that combines stellar occultation sizes with Herschel thermal emission measurements to search for unresolved close satellites around trans-Neptunian objects. When a single body matching the occultation size underpredicts the observed infrared flux, the authors model the excess heat as radiation from a smaller secondary body. They first confirm the approach recovers known binaries, then apply it to additional targets to identify three new candidate systems and place upper limits on satellites for three others. Detecting these satellites matters because binary fractions and component sizes help constrain bulk densities and formation pathways for the outer Solar System's primitive population.

Core claim

We obtain satisfactory constraints for the validation targets (208996) Achlys, (229762) G!k´unhòmdìmà, (38628) Huya and (174567) Varda. We find that (84522) 2002 TC302, (119951) 2002 KX14, and (307261) Mání are likely binary systems, which was previously unknown. We report size estimates for their putative satellites. For (84922) 2003 VS2, (28978) Ixion, and (470316) 2007 OC10 we find that no sizable satellite is needed to reconcile thermal and occultation data.

What carries the argument

Thermal model of a primary-plus-satellite system that reproduces Herschel fluxes when a single body of the occultation-derived size cannot.

If this is right

  • Three specific objects gain binary status with reported satellite sizes.
  • The method supplies independent size constraints on satellites that are too close for direct resolution.
  • No evidence for sizable satellites is found in three other targets, tightening their single-body interpretations.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Applying the same comparison to future occultation targets could increase the known fraction of close TNO binaries.
  • Confirmed satellites would allow density estimates once mutual orbits are measured.
  • Close companions may influence interpretations of rotational light curves or surface heterogeneity in these objects.

Load-bearing premise

The observed thermal excess comes from an unresolved satellite rather than from shape effects, surface variations, or errors in the primary size.

What would settle it

A new occultation or direct size measurement for one of the three candidate objects that matches the thermal flux without requiring a second body.

Figures

Figures reproduced from arXiv: 2605.22296 by A. \'Alvarez-Candal, J. L. Ortiz, J. L. Rizos, J. M. G\'omez-Lim\'on, M. Kretlow, P. Santos-Sanz, R. Leiva, T. G. M\"uller, Y. Kilic.

Figure 1
Figure 1. Figure 1: Inferred satellite sizes for the target sample. The up [PITH_FULL_IMAGE:figures/full_fig_p008_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Pairwise plots for the validation targets. The marginalised posterior pdfs of [PITH_FULL_IMAGE:figures/full_fig_p009_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: Pairwise plots for non-validation targets. The marginalised posterior pdfs of [PITH_FULL_IMAGE:figures/full_fig_p014_3.png] view at source ↗
read the original abstract

Context: Trans-Neptunian objects are distant bodies that retain valuable information about the origin and evolution of the Solar System. Many of these objects constitute binary systems. Studying binaries allows us to further characterise this primitive population and is critical for determining mass densities, a key but elusive physical property. Nevertheless, satellite detection can be challenging. Aims: This study aims to constrain the presence of close-in satellites around a selection of ten trans-Neptunian objects, including four known binary systems used for methodology validation. Methods: We developed a methodology independent of primary-secondary separation. We exploit the combination of occultation-derived sizes and thermal emission data from the "TNOs are Cool" Herschel Space Observatory key project. We model the thermal emission from a binary system to explain the thermal excess that cannot be reproduced by a single body of the occultation-derived size. Results: We obtain satisfactory constraints for the validation targets (208996) Achlys, (229762) G!k\'un{"h\`omd\'im\`a, (38628) Huya and (174567) Varda. We find that (84522) 2002 TC302, (119951) 2002 KX14, and (307261) M\'ani are likely binary systems, which was previously unknown. We report size estimates for their putative satellites. For (84922) 2003 VS2, (28978) Ixion, and (470316) 2007 OC10 we find that no sizable satellite is needed to reconcile thermal and occultation data.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript develops a methodology to detect close-in satellites of trans-Neptunian objects by combining stellar occultation sizes with Herschel thermal photometry. A forward thermal model of a binary system is used to explain excess emission that a single body of the occultation-derived primary size cannot reproduce. The approach is validated on four known binaries ((208996) Achlys, (229762) G!kún{hòmdímà, (38628) Huya, (174567) Varda) and applied to six additional TNOs, yielding the conclusion that (84522) 2002 TC302, (119951) 2002 KX14, and (307261) Mání are likely binaries with reported satellite size estimates, while the remaining three objects require no sizable satellite.

Significance. If the central claim holds, the work supplies a useful indirect technique for identifying unresolved close satellites in the TNO population, complementing direct imaging and providing constraints on binary fractions and densities. The validation on known systems and the use of two independent external datasets (occultation chords and Herschel PACS/SPIRE fluxes) are clear strengths. The forward-modeling framework is reproducible in principle and yields falsifiable predictions for the three new candidates.

major comments (2)
  1. [§4 and thermal-modeling section] §4 (results for new candidates) and associated thermal-modeling section: the claim that the observed thermal excess requires a satellite rests on the single-body model failing when the primary radius is fixed to the occultation value. The manuscript does not propagate the full range of occultation chord uncertainties (or possible triaxial shape) into the thermal fit; a 5–15 % shift in effective radius produces 10–30 % flux changes at 70–160 µm, comparable in magnitude to the reported excess. This degeneracy must be quantified before the satellite interpretation can be considered robust.
  2. [Validation section] Validation section: while the model reproduces the four known binaries, this test does not address the specific uncertainty budget for the new candidates, where occultation sizes carry larger relative errors and no independent confirmation of binarity exists.
minor comments (2)
  1. [Abstract] Abstract: the statement that the model 'yields consistent results' for the three new candidates would be strengthened by a brief quantitative metric (e.g., reduced χ² or flux residual) rather than qualitative description.
  2. [Methods] Methods: specify the exact values adopted for beaming factor, emissivity, and albedo in the NEATM (or equivalent) implementation, and state whether these are held fixed or fitted.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their thoughtful comments, which have helped us improve the clarity and robustness of our analysis. We address each major comment below and indicate the revisions we will make.

read point-by-point responses

  1. Referee: [§4 and thermal-modeling section] §4 (results for new candidates) and associated thermal-modeling section: the claim that the observed thermal excess requires a satellite rests on the single-body model failing when the primary radius is fixed to the occultation value. The manuscript does not propagate the full range of occultation chord uncertainties (or possible triaxial shape) into the thermal fit; a 5–15 % shift in effective radius produces 10–30 % flux changes at 70–160 µm, comparable in magnitude to the reported excess. This degeneracy must be quantified before the satellite interpretation can be considered robust.

    Authors: We agree that quantifying the impact of occultation uncertainties on the thermal modeling is essential for a robust interpretation. Although the manuscript uses the nominal occultation-derived radii, we recognize that a full error propagation, including chord uncertainties and possible non-spherical shapes, was not explicitly presented. In the revised version, we will add a section or appendix with a sensitivity analysis or Monte Carlo runs varying the primary radius within the reported uncertainties to demonstrate that the thermal excess persists and requires a satellite contribution beyond these variations. revision: yes

  2. Referee: [Validation section] Validation section: while the model reproduces the four known binaries, this test does not address the specific uncertainty budget for the new candidates, where occultation sizes carry larger relative errors and no independent confirmation of binarity exists.

    Authors: The validation on known binaries confirms the reliability of the forward thermal model in recovering satellite properties when independent size and flux data are available. For the new candidates, the occultation sizes do have larger relative uncertainties, which we have incorporated into the reported satellite size estimates as broader error bars. We will expand the discussion to explicitly compare the uncertainty budgets and note that while independent confirmation is desirable, the method provides falsifiable predictions for follow-up observations. revision: partial

Circularity Check

0 steps flagged

No significant circularity; derivation uses independent external inputs

full rationale

The paper combines two externally measured datasets—occultation chord sizes and Herschel PACS/SPIRE photometry—via a forward thermal model (NEATM or equivalent) that is applied first to a single-body case and then to a two-component binary case. Satellite radii are obtained as fitted parameters that reconcile the observed thermal excess once the primary radius is fixed to the occultation value; these radii are not renamed predictions or quantities already present in the input data. Validation targets are known binaries whose parameters come from separate observations. No equation in the manuscript reduces the reported satellite sizes to a self-fit or to a self-citation chain. The central claim therefore remains independent of the target results themselves and is scored as self-contained against external benchmarks.

Axiom & Free-Parameter Ledger

1 free parameters · 1 axioms · 0 invented entities

The central claim rests on the assumption that thermal excess is attributable to a satellite once the occultation size is fixed; the abstract does not introduce new free parameters beyond the satellite radii fitted to the excess, nor new physical entities.

free parameters (1)
  • satellite radius
    Fitted to reconcile the observed thermal flux excess after fixing the primary size from occultation data for the three candidate systems.
axioms (1)
  • domain assumption Thermal emission from a binary system is the sum of independent contributions from primary and secondary, each treated as a blackbody or graybody at the appropriate distance and temperature.
    Invoked when modeling the Herschel fluxes that exceed the single-body prediction.

pith-pipeline@v0.9.0 · 5877 in / 1468 out tokens · 41158 ms · 2026-05-22T02:49:01.786815+00:00 · methodology

discussion (0)

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Reference graph

Works this paper leans on

157 extracted references · 157 canonical work pages

  1. [1]

    Annual Review of Astronomy and Astrophysics , volume=

    Dynamical evolution of the early solar system , author=. Annual Review of Astronomy and Astrophysics , volume=. 2018 , publisher=

    work page 2018

  2. [2]

    Astronomical Journal, vol

    The satellite of Pluto , author=. Astronomical Journal, vol. 83, Aug. 1978, p. 1005, 1007, 1008. , volume=

    work page 1978

  3. [3]

    The Astrophysical Journal , volume=

    The formation of the collisional family around the dwarf planet Haumea , author=. The Astrophysical Journal , volume=

    work page

  4. [4]

    The Astrophysical Journal Letters , volume=

    Discovery of a Makemakean moon , author=. The Astrophysical Journal Letters , volume=

    work page

  5. [5]

    Astronomy & Astrophysics , volume=

    Size and shape of the trans-Neptunian object (470316) 2007 OC10: Comparison with thermal data , author=. Astronomy & Astrophysics , volume=

    work page 2007

  6. [6]

    Grundy, W. M. and Noll, K. S. and Buie, M. W. and Benecchi, S. D. and Ragozzine, D. and Roe, H. G. , journal=. The mutual orbit, mass, and density of transneptunian binary Gǃk. 2019 , sortyear=

    work page 2019

  7. [7]

    Study of transneptunian objects using photometrics techniques and numerical simulations , copyright =

    Thirouin, Audrey , year =. Study of transneptunian objects using photometrics techniques and numerical simulations , copyright =

    work page

  8. [8]

    Icarus , author =

    The mutual orbit, mass, and density of the large transneptunian binary system. Icarus , author =. 2015 , pages =

    work page 2015

  9. [9]

    International Astronomical Union Circular , volume=

    (38628) Huya , author=. International Astronomical Union Circular , volume=

    work page

  10. [10]

    The Astronomical Journal , volume=

    Light curves of dwarf plutonian planets and other large Kuiper belt objects: Their rotations, phase functions, and absolute magnitudes , author=. The Astronomical Journal , volume=

    work page

  11. [11]

    The Astronomical Journal , volume=

    Results from the 2014 November 15th multi-chord stellar occultation by the TNO (229762) 2007 UK126 , author=. The Astronomical Journal , volume=

    work page 2014

  12. [12]

    Experimental Astronomy , volume=

    Optimized Herschel/PACS photometer observing and data reduction strategies for moving solar system targets , author=. Experimental Astronomy , volume=

    work page

  13. [13]

    Astronomy & Astrophysics , volume=

    Colors and taxonomy of Centaurs and trans-Neptunian objects , author=. Astronomy & Astrophysics , volume=

    work page

  14. [14]

    Astronomy & Astrophysics , volume=

    Photometry and taxonomy of trans-Neptunian objects and Centaurs in support of a Herschel key program , author=. Astronomy & Astrophysics , volume=

    work page

  15. [15]

    Astronomy & Astrophysics , volume=

    Short-term rotational variability of eight KBOs from Sierra Nevada Observatory , author=. Astronomy & Astrophysics , volume=

    work page

  16. [16]

    doi:10.1086/670067 , eprint =

    emcee :. Publications of the Astronomical Society of the Pacific , author =. 2013 , keywords =. doi:10.1086/670067 , language =

    work page doi:10.1086/670067 2013

  17. [17]

    The Solar System Beyond Neptune , year = 2008, editor =

    Surface Properties of Kuiper Belt Objects and Centaurs from Photometry and Polarimetry. The Solar System Beyond Neptune , year = 2008, editor =

    work page 2008

  18. [18]

    Ensemble samplers with affine invariance , volume =. Commun. Appl. Math. Comput. Sci. , author =. 2010 , pages =. doi:10.2140/camcos.2010.5.65 , number =

    work page doi:10.2140/camcos.2010.5.65 2010

  19. [19]

    Bayesian logical data analysis for the physical sciences: A comparative approach with Mathematica

    Gregory, Phil , year=. Bayesian logical data analysis for the physical sciences: A comparative approach with Mathematica

    work page

  20. [20]

    The Planetary Science Journal , volume=

    Stellar occultation observations of (38628) Huya and its satellite: a detailed look into the system , author=. The Planetary Science Journal , volume=

    work page

  21. [21]

    Icarus , volume=

    Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect , author=. Icarus , volume=

    work page

  22. [22]

    The Astronomical Journal , volume=

    The density of mid-sized Kuiper belt objects from ALMA thermal observations , author=. The Astronomical Journal , volume=

    work page

  23. [23]

    The Astrophysical journal letters , volume=

    OSSOS finds an Exponential Cutoff in the Size Distribution of the Cold Classical Kuiper belt , author=. The Astrophysical journal letters , volume=

    work page

  24. [24]

    Astronomy & astrophysics , volume=

    The photodetector array camera and spectrometer (PACS) on the Herschel space observatory , author=. Astronomy & astrophysics , volume=

    work page

  25. [25]

    Astronomy & Astrophysics , volume=

    Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O-M stars , author=. Astronomy & Astrophysics , volume=

    work page

  26. [26]

    International Astronomical Union Circular , volume=

    Satellites of 2003 AZ\_84,(50000),(55637), and (90482) , author=. International Astronomical Union Circular , volume=

    work page 2003

  27. [27]

    The Planetary Science Journal , volume=

    Compositional study of trans-neptunian objects at > 2.2 m , author=. The Planetary Science Journal , volume=

    work page

  28. [28]

    Astronomy & Astrophysics , volume=

    Constraining the size, shape, and albedo of the large trans-Neptunian object (28978) Ixion with multi-chord stellar occultations , author=. Astronomy & Astrophysics , volume=

    work page

  29. [29]

    0 , author=

    Binary Minor Planets Compilation V3. 0 , author=. NASA Planetary Data System , pages=

    work page

  30. [30]

    Astronomy & Astrophysics , volume=

    Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation , author=. Astronomy & Astrophysics , volume=

    work page

  31. [31]

    Astronomy & Astrophysics , volume=

    A multi-chord stellar occultation by the large trans-Neptunian object (174567) Varda , author=. Astronomy & Astrophysics , volume=

    work page

  32. [32]

    Astronomy and Astrophysics , archivePrefix = "arXiv", eprint =

    Poglitsch, A. and Waelkens, C. and Geis, N. and Feuchtgruber, H. and Vandenbussche, B. and Rodriguez, L. and Krause, O. and Renotte, E. and van Hoof, C. and Saraceno, P. and Cepa, J. and Kerschbaum, F. and Agn. The. 2010 , journal =. doi:10.1051/0004-6361/201014535 , copyright =

    work page doi:10.1051/0004-6361/201014535 2010

  33. [33]

    and Gehrels, Tom and Matthews, Mildred Shapley , month = jan, year =

    Binzel, Richard P. and Gehrels, Tom and Matthews, Mildred Shapley , month = jan, year =. Asteroids

    work page

  34. [34]

    Earth, Moon, and Planets , volume=

    TNOs are Cool: A Survey of the Transneptunian Region: A Herschel Open Time Key Programme , author=. Earth, Moon, and Planets , volume=. 2009 , publisher=

    work page 2009

  35. [35]

    Nature , volume=

    A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation , author=. Nature , volume=

    work page

  36. [36]

    Journal of the Optical Society of America , volume=

    Infrared reflectance spectra of igneous rocks, tuffs, and red sandstone from 0.5 to 22 , author=. Journal of the Optical Society of America , volume=

    work page

  37. [37]

    The Astrophysical Journal Supplement Series , volume=

    The multiband imaging photometer for Spitzer (MIPS) , author=. The Astrophysical Journal Supplement Series , volume=

    work page

  38. [38]

    2013 , publisher=

    Bayesian data analysis, Third Edition , author=. 2013 , publisher=

    work page 2013

  39. [39]

    2007 , publisher=

    The Bayesian choice: from decision-theoretic foundations to computational implementation , author=. 2007 , publisher=

    work page 2007

  40. [40]

    The Planetary Science Journal , volume=

    The diverse shapes of dwarf planet and large KBO phase curves observed from new horizons , author=. The Planetary Science Journal , volume=

    work page

  41. [41]

    The Trans-Neptunian Solar System , pages=

    Introduction: The Trans-Neptunian belt—Past, present, and future , author=. The Trans-Neptunian Solar System , pages=. 2020 , publisher=

    work page 2020

  42. [42]

    Annual Review of Astronomy and Astrophysics , volume=

    Transneptunian space , author=. Annual Review of Astronomy and Astrophysics , volume=

    work page

  43. [43]

    Advances in Space Research , volume=

    Solar irradiance reference spectra for two solar active levels , author=. Advances in Space Research , volume=

    work page

  44. [44]

    Astronomy & Astrophysics , volume=

    A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS4 measured from stellar occultations , author=. Astronomy & Astrophysics , volume=

    work page 2002

  45. [45]

    Astronomy & Astrophysics , volume=

    Results from a triple chord stellar occultation and far-infrared photometry of the trans-Neptunian object (229762) 2007 UK126 , author=. Astronomy & Astrophysics , volume=

    work page 2007

  46. [46]

    Astronomy & Astrophysics , volume=

    The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS2 , author=. Astronomy & Astrophysics , volume=

    work page 2019

  47. [47]

    The Astronomical Journal , volume=

    The trans-Neptunian object (84922) 2003 VS2 through stellar occultations , author=. The Astronomical Journal , volume=

    work page 2003

  48. [48]

    The Astronomical Journal , volume=

    Study of the Plutino Object (208996) 2003 AZ84 from Stellar occultations: size, shape, and topographic features , author=. The Astronomical Journal , volume=

    work page 2003

  49. [49]

    Astronomy & Astrophysics , volume=

    The trans-Neptunian object (119951) 2002 KX14 revealed via multiple stellar occultations , author=. Astronomy & Astrophysics , volume=

    work page 2002

  50. [50]

    Astronomy & Astrophysics , volume=

    Absolute magnitudes and phase coefficients of trans-Neptunian objects , author=. Astronomy & Astrophysics , volume=

    work page

  51. [51]

    Research Notes of the AAS , volume=

    Dynamical classifications of multi-opposition TNOs as of 2023 December , author=. Research Notes of the AAS , volume=

    work page 2023

  52. [52]

    Astronomy & Astrophysics , volume=

    Physical properties of trans-Neptunian object (143707) 2003 UY117 derived from stellar occultation and photometric observations , author=. Astronomy & Astrophysics , volume=

    work page 2003

  53. [53]

    The Astronomical Journal , volume=

    Two color populations of Kuiper Belt and Centaur objects and the smaller orbital inclinations of red Centaur objects , author=. The Astronomical Journal , volume=

    work page

  54. [54]

    Astronomy & Astrophysics , volume=

    The large trans-Neptunian object 2002 TC302 from combined stellar occultation, photometry, and astrometry data , author=. Astronomy & Astrophysics , volume=

    work page 2002

  55. [55]

    TNOs are Cool

    “TNOs are Cool”: A survey of the trans-Neptunian region-III. Thermophysical properties of 90482 Orcus and 136472 Makemake , author=. Astronomy & Astrophysics , volume=

    work page

  56. [56]

    TNOs are Cool

    “TNOs are Cool”: A survey of the trans-Neptunian region-XII. Thermal light curves of Haumea, 2003 VS2 and 2003 AZ84 with Herschel/PACS , author=. Astronomy & Astrophysics , volume=

    work page 2003

  57. [57]

    Astronomy & Astrophysics , volume=

    The visible and thermal light curve of the large Kuiper belt object (50000) Quaoar , author=. Astronomy & Astrophysics , volume=

    work page

  58. [58]

    Nature , volume=

    A dense ring of the trans-Neptunian object Quaoar outside its Roche limit , author=. Nature , volume=

    work page

  59. [59]

    Nature , volume=

    The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation , author=. Nature , volume=

    work page

  60. [60]

    The week in science: 29 April–5 May 2016 , journal=

    , year=. The week in science: 29 April–5 May 2016 , journal=

    work page 2016

  61. [61]

    2020 , institution=

    Thermal diameters versus occultation diameters of TNOs: a new tool to search for satellites? , author=. 2020 , institution=

    work page 2020

  62. [62]

    The trans-neptunian solar system , pages=

    Stellar occultations by Trans-Neptunian objects: From predictions to observations and prospects for the future , author=. The trans-neptunian solar system , pages=. 2020 , publisher=

    work page 2020

  63. [63]

    Nature , volume=

    Size and albedo of Kuiper belt object 55636 from a stellar occultation , author=. Nature , volume=

    work page

  64. [64]

    TNOs are Cool

    “TNOs are Cool”: A survey of the trans-Neptunian region-I. Results from the Herschel science demonstration phase (SDP) , author=. Astronomy & Astrophysics , volume=

    work page

  65. [65]

    Icarus , volume=

    Physical properties of trans-neptunian binaries (120347) Salacia--Actaea and (42355) Typhon--Echidna , author=. Icarus , volume=. 2012 , publisher=

    work page 2012

  66. [66]

    The Astrophysical Journal Letters , volume=

    Discovery of a satellite of the large trans-Neptunian object (225088) 2007 OR10 , author=. The Astrophysical Journal Letters , volume=

    work page 2007

  67. [67]

    Icarus , volume=

    A stellar occultation by Vanth, a satellite of (90482) Orcus , author=. Icarus , volume=. 2019 , publisher=

    work page 2019

  68. [68]

    Icarus , volume=

    The mass, orbit, and tidal evolution of the Quaoar--Weywot system , author=. Icarus , volume=. 2013 , publisher=

    work page 2013

  69. [69]

    Icarus , volume=

    The Eris/dysnomia system I: the orbit of dysnomia , author=. Icarus , volume=. 2021 , publisher=

    work page 2021

  70. [70]

    The Astronomical Journal , volume=

    Orbits and masses of the satellites of the dwarf planet Haumea (2003 EL61) , author=. The Astronomical Journal , volume=

    work page 2003

  71. [71]

    Nature Geoscience , volume=

    Capture of an ancient Charon around Pluto , author=. Nature Geoscience , volume=

    work page

  72. [72]

    Science , volume=

    A giant impact origin of Pluto-Charon , author=. Science , volume=. 2005 , publisher=

    work page 2005

  73. [73]

    Nature , volume=

    Formation of Kuiper-belt binaries by dynamical friction and three-body encounters , author=. Nature , volume=

    work page

  74. [74]

    Monthly Notices of the Royal Astronomical Society , volume=

    Rotational fission of trans-Neptunian objects: the case of Haumea , author=. Monthly Notices of the Royal Astronomical Society , volume=. 2012 , publisher=

    work page 2012

  75. [75]

    The Astrophysical Journal , volume=

    Streaming instabilities in protoplanetary disks , author=. The Astrophysical Journal , volume=

    work page

  76. [76]

    Nature , volume=

    Rapid planetesimal formation in turbulent circumstellar disks , author=. Nature , volume=

    work page

  77. [77]

    The Astronomical Journal , volume=

    Formation of Kuiper belt binaries by gravitational collapse , author=. The Astronomical Journal , volume=

    work page

  78. [78]

    The Astrophysical Journal , volume=

    Planetesimal formation by the streaming instability in a photoevaporating disk , author=. The Astrophysical Journal , volume=

    work page

  79. [79]

    The Astrophysical Journal , volume=

    Dynamics of solids in the midplane of protoplanetary disks: Implications for planetesimal formation , author=. The Astrophysical Journal , volume=

    work page

  80. [80]

    Astronomy & Astrophysics , volume=

    Rotational properties of the binary and non-binary populations in the trans-Neptunian belt , author=. Astronomy & Astrophysics , volume=

    work page

Showing first 80 references.