activity
20112025
most citedA new method to determine the grain size of planetary regolith

247 citations · 778 across the 6 of their papers we have counts for

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Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2025★ 4 cited

Constraints on the ejecting-crust activity model on comet 67P/Churyumov-Gerasimenko

Nicholas Attree, Pedro Gutiérrez, Christian Schuckart +6

Reproducing the observed activity of comets with thermophysical models remains a primary challenge of cometary science. We use a pebble-based thermophysical model of gas-pressure b…

astro-ph.EP2024

Localised ejection of dust and chunks on comet 67P/Churyumov-Gerasimenko: testing how comets work

Nicholas Attree, Christian Schuckart, Dorothea Bischoff +2

We extend an existing thermophysical activity model of comet 67P/Churyumov-Gerasimenko to include pressure buildup inside the pebbles making up the nucleus. We test various quantit…

astro-ph.EP2014★ 127 cited

Comets formed in solar-nebula instabilities! -- An experimental and modeling attempt to relate the activity of comets to their formation process (corrigendum included)

Jürgen Blum, Bastian Gundlach, Steffen Mühle +1

When comet nuclei approach the Sun, the increasing energy flux through the surface layers leads to sublimation of the underlying ices and subsequent outgassing that promotes the ob…

astro-ph.EP2012★ 247 cited

A new method to determine the grain size of planetary regolith

Bastian Gundlach, Jürgen Blum

Airless planetary bodies are covered by a dusty layer called regolith. The grain size of the regolith determines the temperature and the mechanical strength of the surface layers.…

astro-ph.EP2011★ 200 cited

Dust release and tensile strength of the non-volatile layer of cometary nuclei

Yuri Skorov, Jürgen Blum

We developed a thermophysical model for cometary nuclei, which is based upon the assumption that comets form by the gravitational instability of an ensemble of dust and ice aggrega…