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Two methods for determining the temperature on the surface of the cometary nucleus based on spectroscopic measurements
DOI: 10.1016/j.pss.2024.106027 Bibcode: 2025P&SS..25506027W

Wesołowski, Marcin; Potera, Piotr; Kucab, Krzysztof

The paper presents two methods that can be used to determine the surface temperature of a cometary nucleus. The key role in this approach is played by the measurement of hemispherical albedo for selected dust analogues, which was performed using a Cary 5000 spectrometer. To most accurately reflect the actual structure of the dust layer present on …

2025 Planetary and Space Science
Rosetta 1
The refractory-to-ice ratio in comet 67P: Implications on the composition of the comet-forming region of the protoplanetary disk
DOI: 10.1016/j.pss.2025.106061 Bibcode: 2025P&SS..25906061M

Morbidelli, Alessandro; Marschall, Raphael; Marrocchi, Yves

Comets, asteroids, and other small bodies are thought to be remnants of the original planetesimal population of the Solar System. As such, their physical, chemical, and isotopic properties hold crucial details on how and where they formed and how they evolved. Yet, placing precise constraints on the formation region of these bodies has been challe…

2025 Planetary and Space Science
Rosetta 1
Key structural characteristics of porous layers in diffusion modelling: A study on polydispersity, shape, and hierarchy
DOI: 10.1016/j.pss.2025.106078 Bibcode: 2025P&SS..26006078R

Skorov, Yuri; Reshetnyk, Volodymyr; Blum, Jürgen +5 more

In this study, we explored various open-source models for generating porous media. These models enabled us to examine different types of porous beds, including layers of polydisperse spheres with various size distributions, layers of porous aggregates – either fragments of parent porous layers or those formed during the agglomeration of polydisper…

2025 Planetary and Space Science
Rosetta 0
A fully kinetic perspective on weakly active comets: Asymmetric outgassing
DOI: 10.1016/j.pss.2025.106064 Bibcode: 2025P&SS..25806064D

Henri, Pierre; Galand, Marina; Divin, Andrey +3 more

The European Space Agency's Rosetta mission measured the complex plasma environment surrounding comet 67P/Churyumov-Gerasimenko for more than two years. In this work, the collisionless dynamics of the plasma interaction during the comet's weakly outgassing phases is investigated through a fully kinetic semi-implicit particle-in-cell approach. The …

2025 Planetary and Space Science
Rosetta 0
On structural properties of Comet 67/P dust particles collected in situ by ROSETTA/COSIMA from observations of electrical fragmentation
DOI: 10.1016/j.pss.2023.105747 Bibcode: 2023P&SS..23605747K

Klaus, Hornung; Eva, Maria Mellado; Oliver, J. Stenzel +20 more

After landing on the target, the kinetic energy can be dissipated within the fragment if it consists of many elements (as in the example of the Kerttu-Ender fragment, Fig. 2). If it consists of only a few elements, as is the case for most fragments traveling longer distances, the kinetic energy is dissipated by rolling. In the case of impact fragm…

2023 Planetary and Space Science
Rosetta 2
New constraints on the chemical composition and outgassing of 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.pss.2021.105194 Bibcode: 2021P&SS..20005194H

Thomas, N.; Rubin, M.; Mousis, O. +4 more

Strong heterogeneities in the composition of the volatile species have been detected in the coma of comet 67P/Churyumov-Gerasimenko (67P/C-G) by the ROSINA instrument onboard the ESA's Rosetta spacecraft. However, it is not clear if these heterogeneities are indicative of heterogeneities in the near-surface nucleus composition or if the coma compo…

2021 Planetary and Space Science
Rosetta 3
Dynamics of material ejected from the Hatmehit depression and landslides on comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.pss.2021.105358 Bibcode: 2021P&SS..20905358C

Czechowski, Leszek; Kossacki, Konrad J.

In this work we investigate trajectories and regions of deposition of material ejected from depression Hatmehit on comet 67P/Churyumov-Gerasimenko. This depression, located on the lobe Head, could be a result of endogenic, possibly still ongoing, activity. We calculated trajectories of the ejecta with different initial velocities and we determined…

2021 Planetary and Space Science
Rosetta 0
Outbursts of comets at large heliocentric distances: Concise review and numerical simulations of brightness jumps
DOI: 10.1016/j.pss.2020.104867 Bibcode: 2020P&SS..18404867W

Wesołowski, M.; Gronkowski, P.; Tralle, I.

The outburst of comet brightness is spectacular and well-known manifestation of the physical activity of these relatively small cosmic bodies. The outbursts of brightness are observed for periodic comets, as well as for the comets moving along parabolic trajectories. The most known comet representing such kind of activity is the comet 29P/Schwassm…

2020 Planetary and Space Science
Rosetta 11
Zodiacal light observations and its link with cosmic dust: A review
DOI: 10.1016/j.pss.2020.104973 Bibcode: 2020P&SS..19004973L

Lasue, Jeremie; Levasseur-Regourd, Anny-Chantal; Renard, Jean-Baptiste

The zodiacal light is a nightglow mostly visible along the plane of the ecliptic. It represents the background radiation associated with solar light scattered by the tenuous flattened interplanetary cloud of dust particles surrounding the Sun and the planets. It is an interesting subject of study, as the source of the micrometeoroids falling on Ea…

2020 Planetary and Space Science
Rosetta 11
Analogues of interplanetary dust particles to interpret the zodiacal light polarization
DOI: 10.1016/j.pss.2018.04.022 Bibcode: 2020P&SS..18304527H

Lasue, J.; Levasseur-Regourd, A. C.; Hadamcik, E. +1 more

2020 Planetary and Space Science
Rosetta 10