Do icy dust aggregates break up when they pass the snow line?

Icy dust aggregates can break up when they pass the snow line or when a heating event occurs because of the sublimation of H 2 O ice. However, the original aggregate may absorb the fragment conducting the Brownian motion because the thickness of the icy mantle of a grain is less than the typical grain radius of ∼ 1 0 − 5 cm. On the other hand, the vapor pressure caused by the sublimated H 2 O molecules accelerates the fragment to escape. Rotation of the aggregate and electrostatic repulsion may also promote the escape of the fragment aggregate. Here, I determined a lower bound of the escaping fragment radius, including the effects of the vapor pressure, rotation, and electrostatic repulsion. It has been found that the breakup to the single grain does not occur, and the fragment radius strongly depends on the thickness of the icy mantle. The vapor pressure and the rotation produce fragments from large aggregates. The fragments escape from small aggregates by the electrostatic repulsion. Possible consequences of the breakup are discussed. • The fragment radius produced by the sublimation of H 2 O ice that can escape is estimated. • Rotation and H 2 O vapor pressure promote the escaping from the large aggregates. • Fragments escape from small aggregates by electrostatic repulsion. • The thickness of the icy mantle is a critical parameter.

Authors

Institutions

Publication Details

Journal
Icarus
Published
2024-12-18
DOI
https://doi.org/10.1016/j.icarus.2024.116430
Primary Topic
Cryospheric studies and observations
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Do icy dust aggregates break up when they pass the snow line?

Sin‐iti Sirono
Icarus
Cryospheric studies and observations
article

Do icy dust aggregates break up when they pass the snow line?

Sin‐iti Sirono
article en

Abstract

Icy dust aggregates can break up when they pass the snow line or when a heating event occurs because of the sublimation of H 2 O ice. However, the original aggregate may absorb the fragment conducting the Brownian motion because the thickness of the icy mantle of a grain is less than the typical grain radius of ∼ 1 0 − 5 cm. On the other hand, the vapor pressure caused by the sublimated H 2 O molecules accelerates the fragment to escape. Rotation of the aggregate and electrostatic repulsion may also promote the escape of the fragment aggregate. Here, I determined a lower bound of the escaping fragment radius, including the effects of the vapor pressure, rotation, and electrostatic repulsion. It has been found that the breakup to the single grain does not occur, and the fragment radius strongly depends on the thickness of the icy mantle. The vapor pressure and the rotation produce fragments from large aggregates. The fragments escape from small aggregates by the electrostatic repulsion. Possible consequences of the breakup are discussed. • The fragment radius produced by the sublimation of H 2 O ice that can escape is estimated. • Rotation and H 2 O vapor pressure promote the escaping from the large aggregates. • Fragments escape from small aggregates by electrostatic repulsion. • The thickness of the icy mantle is a critical parameter.

IcarusVol. 429
Nagoya University (JP)
Climate action
Openalex Percentile: Top 74%
Cryospheric studies and observations
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.