Search Publications

Land of gas and dust - exploring bursting cavities on comet 67P
DOI: 10.1093/mnras/staf180 Bibcode: 2025MNRAS.537.2997M

De Keyser, Johan; Berthelier, Jean-Jacques; Wurz, Peter +9 more

Gas and dust outbursts are recurring phenomena on comets, offering critical insights into their subsurface activities. On comet 67P/Churyumov-Gerasimenko, two distinct outburst types have been identified: CO$_{2}$-dominated 'summer fireworks' near perihelion and wat…

2025 Monthly Notices of the Royal Astronomical Society
Rosetta 0
Thermal stresses as a possible mechanism for initiating the destruction of comet Shoemaker-Levy 9
DOI: 10.1093/mnras/staf081 Bibcode: 2025MNRAS.537.2151S

Omarov, Chingis; Shestakova, Lyubov I.; Spassyuk, Ruslan

It is now widely accepted that the breakup of comet Shoemaker-Levy 9 (SL9) was caused by tidal forces. This explanation applies to bodies that enter a planet's Roche zone and have a loose 'rubble pile' structure with no internal strength. Observations from the Rosetta mission to comet 67P/Churyumov-Gerasimenko initially supported this hypothesis, …

2025 Monthly Notices of the Royal Astronomical Society
Rosetta 0
The GUAPOS project - V: The chemical ingredients of a massive stellar protocluster in the making
DOI: 10.1093/mnras/stae676 Bibcode: 2024MNRAS.529.3244L

Testi, L.; Mininni, C.; Lorenzani, A. +9 more

Most stars, including the Sun, are born in rich stellar clusters containing massive stars. Therefore, the study of the chemical reservoir of massive star-forming regions is crucial to understand the basic chemical ingredients available at the dawn of planetary systems. We present a detailed study of the molecular inventory of the hot molecular cor…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 7
Properties of the gas escaping from a non-isothermal porous dust surface layer of a comet
DOI: 10.1093/mnras/stad3994 Bibcode: 2024MNRAS.52712268S

Mottola, S.; Küppers, M.; Thomas, N. +6 more

Estimation of the properties of the sublimation products leaving the cometary nucleus is one of the significant questions in the study of the dusty-gas flow following the Rosetta mission. It is widely assumed that the temperature of the water molecules emitted is the temperature of ice directly exposed to the surface. However, it is the simplest n…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 6
Cliff collapse on Comet 67P/Churyumov-Gerasimenko - I. Aswan
DOI: 10.1093/mnras/stad3055 Bibcode: 2024MNRAS.527..112D

Davidsson, Björn J. R.

The Aswan cliff on Comet 67P/Churyumov-Gerasimenko collapsed on 2015 July 10. Thereby, relatively pristine comet material from a depth of $\sim 12\, \mathrm{m}$ was exposed at the surface. Observations of the collapse site by the microwave instrument Rosetta/Microwave Instrument for Rosetta Orbiter (MIRO) have been retrieved from 8 months prior to…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 5
Deciphering cometary outbursts: linking gas composition changes to trigger mechanisms
DOI: 10.1093/mnras/stae622 Bibcode: 2024MNRAS.529.2763M

Mall, Urs; De Keyser, Johan; Berthelier, Jean-Jacques +9 more

Dust and gas outbursts are recurrent cometary phenomena, playing a crucial role in shaping the coma. Proposed outburst trigger mechanisms include cliff collapse, pressure pockets, and amorphous-to-crystalline phase transition of water ice; however, the underlying processes remain inadequately understood. In this study, we analyse Rosetta/ROSINA da…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 5
Cliff collapse on Comet 67P/Churyumov-Gerasimenko - II. Imhotep and Hathor
DOI: 10.1093/mnras/stae657 Bibcode: 2024MNRAS.529.2258D

Davidsson, Björn J. R.

Cliff collapses on Comet 67P/Churyumov-Gerasimenko expose relatively pristine nucleus matter and offer rare opportunities to characterize ice-rich comet material. Here, Microwave Instrument for Rosetta Orbiter (MIRO) observations of two collapsed or crumbling cliffs in the Imhotep and Hathor regions have been assembled. The empirical diurnal anten…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 4
Imaging polarimetry of comet 67 P/Churyumov-Gerasimenko: homogeneous distribution of polarization and its implications
DOI: 10.1093/mnras/stae1284 Bibcode: 2024MNRAS.531.1638G

Kolokolova, Ludmilla; Moreno, Fernando; Snodgrass, Colin +8 more

Comet 67P/Churyumov-Gerasimenko (67P) become observable for the first time in 2021 since the Rosetta rendezvous in 2014-2016. Here, we present pre-perihelion polarimetric measurements of 67P from 2021 performed with the Very Large Telescope (VLT), as well as post-perihelion polarimetric measurements from 2015 to 2016 obtained with the VLT and the …

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 3
Detection and characterization of icy cavities on the nucleus of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stae1290 Bibcode: 2024MNRAS.531.2494L

Lamy, Philippe; Groussin, Olivier; Faury, Guillaume +1 more

We report on the detection of three icy cavities on the nucleus of comet 67P/Churyumov-Gerasimenko. They were identified on high-resolution anaglyphs built from images acquired by the Optical, Spectroscopic, and Infrared Remote Imaging System instrument aboard the Rosetta spacecraft on 2016 April 9 and 10. Visually, they appear as bright patches o…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 2
On the similarity of rotational motion of dust particles in the inner atmosphere of comets
DOI: 10.1093/mnras/stad2665 Bibcode: 2024MNRAS.528.5723I

Fulle, M.; Moreno, F.; Rotundi, A. +6 more

In situ measurements of individual dust grain parameters in the immediate vicinity of a cometary nucleus are being carried by the Rosetta spacecraft at comet 67P/Churyumov-Gerasimenko. For interpretation of these observational data, a model of dust grain motion as realistic as possible is requested. In particular, the results of Stardust mission a…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 2