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Cited article:

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The strength of outgassed porous dust aggregates

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The effect of nonlocal disk processes on the volatile CHNOS budgets of planetesimal-forming material

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Micrometre-sized ice particles for planetary science experiments – CoPhyLab cryogenic granular sample production and storage

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RAS Techniques and Instruments 2 (1) 686 (2023)
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Size Dependence of the Bouncing Barrier in Protoplanetary Dust Growth

Sota Arakawa, Satoshi Okuzumi, Misako Tatsuuma, Hidekazu Tanaka, Eiichiro Kokubo, Daisuke Nishiura, Mikito Furuichi and Taishi Nakamoto
The Astrophysical Journal Letters 951 (1) L16 (2023)
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A quantitative description of comet 67P’s dust and gas production remains enigmatic

D Bischoff, C Schuckart, N Attree, B Gundlach and J Blum
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Observed Polarized Scattered Light Phase Functions of Planet-forming Disks

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Formulating Compressive Strength of Dust Aggregates from Low to High Volume Filling Factors with Numerical Simulations

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Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk

Shangjia Zhang, Zhaohuan Zhu, Takahiro Ueda, Akimasa Kataoka, Anibal Sierra, Carlos Carrasco-González and Enrique Macías
The Astrophysical Journal 953 (1) 96 (2023)
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Learning about comets from the study of mass distributions and fluxes of meteoroid streams

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Sub-mm/mm optical properties of real protoplanetary matter derived from Rosetta/MIRO observations of comet 67P

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The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks

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Global Modeling of Nebulae with Particle Growth, Drift, and Evaporation Fronts. II. The Influence of Porosity on Solids Evolution

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Are there any pristine comets? Constraints from pebble structure

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Sublimation of organic-rich comet analog materials and their relevance in fracture formation

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Modeling the Fragmentation of Dust–Ice Clusters at the Snow Line in Protoplanetary Disks

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A method to distinguish between micro- and macro-granular surfaces of small Solar system bodies

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Sublimation of ice-dust mixtures in cooled vacuum environments to reproduce cometary morphologies

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Electric heating and angular momentum transport in laminar models of protoplanetary discs

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Dust-to-Gas and Refractory-to-Ice Mass Ratios of Comet 67P/Churyumov-Gerasimenko from Rosetta Observations

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Experimental Phase Function and Degree of Linear Polarization Curves of Millimeter-sized Cosmic Dust Analogs

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On the activity of comets: understanding the gas and dust emission from comet 67/Churyumov–Gerasimenko’s south-pole region during perihelion

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Unveiling Dust Aggregate Structure in Protoplanetary Disks by Millimeter-wave Scattering Polarization

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CubeSat Particle Aggregation Collision Experiment (Q-PACE): Design of a 3U CubeSat mission to investigate planetesimal formation

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From grains to pebbles: the influence of size distribution and chemical composition on dust emission properties

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Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet

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Homogeneity of 67P/Churyumov-Gerasimenko as seen by CONSERT: implication on composition and formation

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Laboratory measurements of the sub-millimetre opacity of amorphous and micro-particulate H2O ices for temperatures above 80 K

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Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift

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