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The dynamics of a rigid cometary nucleus is described by the evolutions of its center-of-mass and of its rotation state. Solar irradiation that reaches the surface of a cometary nucleus causes the sublimation of volatiles that form the coma…

Earth and Planetary Astrophysics · Physics 2025-07-09 Matthias Laeuter , Tobias Kramer

We investigate the ability of a simultaneous fitting of comet 67P/Churyumov-Gerasimenko's non-gravitational forces, torques and total water-outgassing rate, as observed by Rosetta, to constrain complex thermophysical models of cometary…

Earth and Planetary Astrophysics · Physics 2024-10-07 N. Attree , P. Gutiérrez , O. Groussin , J. Bürger , H. U. Keller , T. Kramer , R. Lasagni Manghi , M. Läuter , P. Lemos , J. Markkanen , R. Marschall , C. Schuckart

Cometary activity affects the orbital motion and rotation state due to sublimation induced forces. The availability of precise rotation-axis orientation and position data from the Rosetta mission allows one to accurately determine the…

Earth and Planetary Astrophysics · Physics 2019-09-25 Tobias Kramer , Matthias Laeuter

An influence of the non-gravitational effects on the motion of short-period comet 67P/Churyumov-Gerasimenko is investigated. It was found that the normal component of the non-gravitational force exceeds the transverse one and a model of the…

Astrophysics · Physics 2007-05-23 Malgorzata Krolikowska

Aims. Understanding the activity is vital for deciphering the structure, formation, and evolution of comets. We investigate models of cometary activity by comparing them to the dynamics of 67P/Churyumov-Gerasimenko. Methods. We matched…

Small bodies in our Solar System are considered remnants of their early formation. Studying their physical and dynamic properties can provide insights into their evolution, stability, and origin. ESA's Rosetta mission successfully landed…

Earth and Planetary Astrophysics · Physics 2026-03-03 Leonardo Braga , Andre Amarante , Alessandra Ferreira , Caio Gomes , Luis Ceranto

The dynamics of irregularly-shaped particles subjected to the combined effect of gas drag and radiative forces and torques in a cometary environment is investigated. The equations of motion are integrated over distances from the nucleus…

We report on the first major temporal morphological changes observed on the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, in the smooth terrains of the Imhotep region. We use images of the OSIRIS cameras onboard Rosetta to…

The aim of this study is first to determine the gravity field of the comet 67P Churyumov-Gerasimenko and second to derive the solar component of the precession rate and nutation coefficients of the spin axis of the comet nucleus, i.e.…

Earth and Planetary Astrophysics · Physics 2016-10-03 Christoph Lhotka , Stefan Reimond , Jean Souchay , Oliver Baur

This study provides a continuous ephemeris reconstruction for comet 67P/Churyumov-Gerasimenko by reanalyzing Rosetta radiometric measurements and Earth-based astrometry. Given the comet-to-spacecraft relative trajectory provided by the…

Earth and Planetary Astrophysics · Physics 2025-03-13 Riccardo Lasagni Manghi , Marco Zannoni , Paolo Tortora , Frank Budnik , Bernard Godard , Nicholas Attree

Starting from several monthly data sets of Rosetta's COmetary Pressure Sensor we reconstruct the gas density in the coma around comet 67P/Churyumov-Gerasimenko. The underlying inverse gas model is constructed by fitting ten thousands of…

Earth and Planetary Astrophysics · Physics 2017-05-29 Tobias Kramer , Matthias Laeuter , Martin Rubin , Kathrin Altwegg

The so-called "early activity" of comet 67P/Churyumov-Gerasimenko has been observed to originate mostly in parts of the concave region or "neck" between its two lobes. Since activity is driven by the sublimation of volatiles, this is a…

Earth and Planetary Astrophysics · Physics 2015-09-11 V. Alí-Lagoa , M. Delbo' , G. Libourel

Aims. We use four observational data sets, mainly from the Rosetta mission, to constrain the activity pattern of the nucleus of comet 67P/Churyumov-Gerasimenko. Methods. We develop a numerical model that computes the production rate and…

Comets display with decreasing solar distance an increased emission of gas and dust particles, leading to the formation of the coma and tail. Spacecraft missions provide insight in the temporal and spatial variations of the dust and gas…

Earth and Planetary Astrophysics · Physics 2018-01-10 Tobias Kramer , Matthias Noack , Daniel Baum , Hans-Christian Hege , Eric J. Heller

We collect observational evidence that supports the scheme of mass transfer on the nucleus of comet 67P/Churyumov-Gerasimenko. The obliquity of the rotation axis of 67P causes strong seasonal variations. During perihelion the southern…

Rosetta observations of 67P/Churyumov-Gerasimenko (67P) reveal that most changes occur in the fallback-generated smooth terrains, vast deposits of granular material blanketing the comet's northern hemisphere. These changes express…

This paper presents the past evolution of the orbital elements of comet 67P/Churyumov-Gerasimenko, target of the Rosetta spacecraft. The gravitational orbit of the comet is affected by the sublimation of ice from the nucleus that triggers…

Earth and Planetary Astrophysics · Physics 2015-07-01 Lucie Maquet

Sublimative outgassing of comets produces torques that alter the rotation state of their nuclei. Recently, parameterized sublimative torque models have been developed to study rotation state changes of individual comet nuclei and…

Earth and Planetary Astrophysics · Physics 2018-06-06 Jordan K. Steckloff , Nalin H. Samarasinha

We simulate the stresses induced by temperature changes in a putative hard layer near the surface of comet 67P/Churyumov--Gerasimenko with a thermo-viscoelastic model. Such a layer could be formed by the recondensation or sintering of water…

We analyze the physical properties and dynamical origin of a curved jet of comet 67P/Churyumov-Gerasimenko that was observed repeatedly in several nucleus rotations starting on May 30 and persisting until early August, 2015. We simulated…

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