Comet 67P/Churyumov–Gerasimenko / Science

Science · Comet 67P/Churyumov–Gerasimenko

What the research says about Comet 67P/Churyumov–Gerasimenko

These are six research papers, all free to read on arXiv, about Comet 67P/Churyumov–Gerasimenko. We summarize each one in plain English from its abstract.

  • Papers 6
  • Topics 3
  • Reviewed Oct 24, 2026
  • Source arXiv.org
Illustrative · not to scale

Our own artist's impression. No figures are taken from the papers.

01

Surface & composition

3 papers

What Comet 67P/Churyumov–Gerasimenko is made of and how its surface behaves.

[1]2015astro-ph.EPPreprint

Pits formation from volatile outgassing on 67P/Churyumov-Gerasimenko

O. Mousis, A. Guilbert-Lepoutre, B. Brugger & 8 others

What they foundThe active pits Rosetta saw could form when buried ice cages (clathrates) break down or amorphous ice crystallises at the depth of the pits.

Why it mattersIt links the comet's dramatic pits to processes inside its ice, either as sinkholes or after outbursts.
What they studied

Computer models of heat flowing into the subsurface of 67P's Seth region.

[2]2023astro-ph.EPPeer-reviewed

The ice composition close to the surface of comet 67P/Churyumov-Gerasimenko

Matthias Laeuter, Tobias Kramer, Martin Rubin & 1 other

What they foundThe team mapped where 14 gases, from water and CO₂ to methanol and ethanol, come off 67P's surface over the two-year mission.

Why it mattersLinking gas output to surface patches shows how the ice just below the surface is distributed.
What they studied

Rosetta ROSINA COPS and DFMS gas-density measurements, fitted onto the comet's shape model.

[3]2017astro-ph.EPPeer-reviewed

Aggregate dust particles at comet 67P/Churyumov-Gerasimenko

Mark S. Bentley, Roland Schmied, Thurid Mannel & 9 others

What they foundDust at 67P is made of aggregates of smaller, elongated grains.

Why it mattersThese are about as pristine as cometary dust gets, so they reveal how dust stuck together when planets were forming.
What they studied

In-place measurements by an instrument on the Rosetta orbiter that collected dust particles.

02

Orbit & dynamics

2 papers

How Comet 67P/Churyumov–Gerasimenko moves, and the gravity and sunlight forces that shape its path.

[4]2019astro-ph.EPPeer-reviewed

Outgassing induced acceleration of comet 67P/Churyumov-Gerasimenko

Tobias Kramer & Matthias Laeuter

What they foundRosetta's own tracking data revealed how 67P's outgassing pushes on the comet and how the push varies through each comet day.

Why it mattersMeasuring this push helps predict comet orbits and test ideas about how ice sublimates.
What they studied

Orbit refinement of Rosetta's trajectory and rotation data.

[5]2003astro-phPeer-reviewed

67P/Churyumov-Gerasimenko - potential target for the Rosetta mission

Malgorzata Krolikowska

What they foundBefore Rosetta, modelling of the forces from outgassing suggested 67P is a slightly elongated body (axial ratio about 1.16).

Why it mattersIt is an early, pre-mission study of the comet Rosetta later visited.
What they studied

Fits of 67P's observed motion including non-gravitational forces.

arXiv:astro-ph/0309130Abstract (opens arXiv)PDF (opens arXiv)
03

Origins & history

1 paper

Where Comet 67P/Churyumov–Gerasimenko came from and how it formed and changed over time.

[6]2020astro-ph.EPPreprint

Thermal inertias of pebble-pile comet 67P/Churyumov-Gerasimenko

Sota Arakawa & Kazumasa Ohno

What they foundModels of 67P as a pile of small dust 'pebbles' reproduce its measured heat-holding behaviour.

Why it mattersThat supports the idea that comets formed by the gentle collapse of pebble clouds in the early Solar System.
What they studied

Calculations of thermal inertia for layered aggregates of pebbles, compared with Rosetta observations.

New research

New papers on Comet 67P/Churyumov–Gerasimenko, checked weekly, summarized after a person reads it.

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How we choose papers

We search arXiv for Comet 67P/Churyumov–Gerasimenko papers and keep the ones that add something new, are clearly written up and are relevant to a general reader. A person reads every abstract.

Our own words, our own drawings

Summaries are written by us from each paper’s abstract, not copied. Diagrams are our own simplified drawings, not figures from the papers.

Preprint vs. peer-reviewed

“Peer-reviewed” means arXiv lists a journal reference for the paper. Everything else is marked “Preprint”: shared openly, possibly before or without journal review.

Paper metadata courtesy of arXiv. Summaries written by us; read the original papers via the links. Paper metadata from arXiv.org, which does not endorse this site.