Diverse protoplanetary disk morphology produced by a Jupiter-mass planet

Abstract

Combining hydrodynamic planet-disk interaction simulations with dust evolution models, we show that protoplanetary disks having a giant planet can reveal diverse morphology in (sub-)millimeter continuum, including a full disk without significant radial structure, a transition disk with an inner cavity, a disk with a single gap and a central continuum peak, and a disk with multiple rings and gaps. Such a diversity originates from (1) the level of viscous transport in the disk which determines the number of gaps a planet can open; (2) the size and spatial distributions of grains determined by the coagulation, fragmentation, and radial drift, which in turn affects the emmisivity of the disk at (sub-)millimeter wavelengths; and (3) the angular resolution used to observe the disk. In particular, our results show that disks having the same underlying gas distribution can have very different grain size/spatial distributions and thus appearance in continuum, depending on the interplay among coagulation, fragmentation, and radial drift. This suggests that proper treatments for the grain growth have to be included in models of protoplanetary disks concerning continuum properties and that complementary molecular line observations are highly desired in addition to continuum observations to reveal the true nature of disks. The fact that a single planet can produce diverse disk morphology emphasizes the need to search for more direct, localized signatures of planets in order to confirm (or dispute) the planetary origin of observed ringed substructures.

arXiv comment12 pages, 8 figures, Accepted for publication in the ApJ Letters

References in corpus (62)

• Rapid planetesimal formation in turbulent circumstellar discs
• Streaming Instabilities in Protoplanetary Disks
• First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region
• Circumstellar Dust Disks in Taurus-Auriga: The Submillimeter Perspective
• A simple model for the evolution of the dust population in protoplanetary disks
• The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts
• Gas- and dust evolution in protoplanetary disks
• The effect of gas drag on the growth of protoplanets -- Analytical expressions for the accretion of small bodies in laminar disks
• FARGO: a fast eulerian transport algorithm for differentially rotating disks
• Ringed Substructure and a Gap at 1 AU in the Nearest Protoplanetary Disk
• Closed-form expressions for particle relative velocities induced by turbulence
• Dust Properties of Protoplanetary Disks in the Taurus-Auriga Star Forming Region from Millimeter Wavelengths
• Zonal Flows and Long-Lived Axisymmetric Pressure Bumps in Magnetorotational Turbulence
• Trapping dust particles in the outer regions of protoplanetary disks
• Disks ARound TTauri Stars with Sphere (DARTTS-S) I: Sphere / IRDIS Polarimetric Imaging of 8 prominent TTauri Disks
• Evidence of fast pebble growth near condensation fronts in the HL Tau protoplanetary disk
• The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. I. The Role of Self-Gravity
• A Kinematical Detection of Two Embedded Jupiter Mass Planets in HD 163296
• Sintering-induced Dust Ring Formation in Protoplanetary Disks: Application to the HL Tau Disk
• Kinematic evidence for an embedded protoplanet in a circumstellar disc
• Accreting Protoplanets in the LkCa 15 Transition Disk
• Weak Turbulence in the HD 163296 Protoplanetary Disk Revealed by ALMA CO Observations
• FARGO3D: A new GPU-oriented MHD code
• How to form planetesimals from mm-sized chondrules and chondrule aggregates
• Direct Imaging of Fine Structures in Giant Planet Forming Regions of the Protoplanetary Disk around AB Aurigae
• Observational Signatures of Planets in Protoplanetary Disks II: Spiral Arms Observed in Scattered Light Imaging Can be Induced by Planets
• How Empty are Disk Gaps Opened by Giant Planets?
• A young protoplanet candidate embedded in the circumstellar disk of HD100546
• Multiple Disk Gaps and Rings Generated by a Single Super-Earth
• Gap Opening by Extremely Low Mass Planets in a Viscous Disk
• Two-Component Secular Gravitational Instability in a Protoplanetary Disk: A Possible Mechanism for Creating Ring-Like Structures
• Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilities
• ALMA continuum observations of the protoplanetary disk AS 209. Evidence of multiple gaps opened by a single planet
• Measuring Turbulence in TW Hya with ALMA: Methods and Limitations
• Standing on the shoulders of giants: Trojan Earths and vortex trapping in low mass self-gravitating protoplanetary disks of gas and solids
• Formation of a disc gap induced by a planet: Effect of the deviation from Keplerian disc rotation
• Resolving the HD 100546 Protoplanetary System with the Gemini Planet Imager: Evidence for Multiple Forming, Accreting Planets
• On the formation of multiple concentric rings and gaps in protoplanetary disks
• Planet formation signposts: observability of circumplanetary disks via gas kinematics
• Can dead zones create structures like a transition disk?
• Radiation Hydrodynamical Turbulence In Protoplanetary Disks: Numerical Models and Observational Constraints
• What is the Mass of a Gap-Opening Planet?
• Multiple Gaps in the Disk of the Class I Protostar GY 91
• Modeling Dust Emission of HL Tau Disk Based on Planet-Disk Interactions
• Planet Formation in AB Aurigae: Imaging of the inner gaseous Spirals observed inside the Dust Cavity
• Complex Spiral Structure in the HD 100546 Transitional Disk as Revealed by GPI and MagAO
• On the Commonality of 10-30AU Sized Axisymmetric Dust Structures in Protoplanetary Disks
• Planet-driven spiral arms in protoplanetary disks: I. Formation mechanism
• Rings and gaps in the disc around Elias 24 revealed by ALMA
• A Gap with a Deficit of Large Grains in the protoplanetary disk around TW Hya
• Dust Evolution Can Produce Scattered Light Gaps in Protoplanetary Disks
• On the Radio Detectability of Circumplanetary Discs
• On the origin of the spiral morphology in the Elias 2-27 circumstellar disc
• How Bright are Planet-Induced Spiral Arms in Scattered Light?
• Dust-driven viscous ring-instability in protoplanetary disks
• How Spirals and Gaps Driven by Companions in Protoplanetary Disks Appear in Scattered Light at Arbitrary Viewing Angles
• Planet-driven spiral arms in protoplanetary disks: II. Implications
• Prograde rotation of protoplanets by accretion of pebbles in a gaseous environment
• Planetary Signatures in the SAO 206462 (HD 135344B) Disk: A Spiral Arm Passing Through Vortex?
• Shock-driven Accretion in Circumplanetary Disks: Observables and Satellite Formation
• Constraining turbulence mixing strength in transitional discs with planets using SPHERE and ALMA
• Saturn's formation and early evolution at the origin of Jupiter's massive moons

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• Gas density perturbations induced by forming planet(s) in the AS 209 protoplanetary disk as seen with ALMA
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• Molecules with ALMA at Planet-forming Scales (MAPS). Complex Kinematics in the AS 209 Disk Induced by a Forming Planet and Disk Winds
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• Gap opening by planets in discs with magnetised winds
• A kinematic excess in the annular gap and gas depleted cavity in the disc around HD 169142
• DBNets: A publicly available deep learning tool to measure the masses of young planets in dusty protoplanetary discs
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• Growth after the streaming instability: The radial distance dependence of the planetary growth
• Improving Planet Detection with Disk Modeling: Keck/NIRC2 Imaging of the HD 34282 Single-armed Protoplanetary Disk
• Architecture of planetary systems predicted from protoplanetary disks observed with ALMA I: mass of the possible planets embedded in the dust gap
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• Distributions of gas and small and large grains in the LkH$\alpha 330$ disk trace a young planetary system
• Substructures in protoplanetary disks imprinted by compact planetary systems
• The Ophiuchus DIsk Survey Employing ALMA (ODISEA): A Unified Evolutionary Sequence of Planet-Driven Substructures Explaining the Diversity of Disk Morphologies
• Constraints on a Putative Planet Sculpting the V4046 Sagittarii Circumbinary Disk
• Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks $\mathrm{I}$. Steady-state model
• Dust Rings and Cavities in the Protoplanetary Disks around HD 163296 and DoAr 44
• Monte Carlo post-processing for radiation hydro simulations of accreting planets in protoplanetary disks