about
Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar SystemE-type asteroid (2867) Steins as imaged by OSIRIS on board Rosetta.Large heterogeneities in comet 67P as revealed by active pits from sinkhole collapse.Two independent and primitive envelopes of the bilobate nucleus of comet 67P.Cometary science. Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the Sun.Cometary science. The morphological diversity of comet 67P/Churyumov-Gerasimenko.Catching a comet. Rosetta begins its comet tale. Introduction.Surface changes on comet 67P/Churyumov-Gerasimenko suggest a more active past.Rosetta's comet 67P/Churyumov-Gerasimenko sheds its dusty mantle to reveal its icy nature.Neutral Sodium from Comet Hale-Bopp: A Third Type of TailTriple F—a comet nucleus sample return missionThe dust coma of the active Centaur P/2004 A1 (LONEOS): a CO-driven environment?Osiris—The optical, spectroscopic and infrared remote imaging system for the Rosetta OrbiterThe Grain Impact Analyser and Dust Accumulator (GIADA) Experiment for the Rosetta Mission: Design, Performances and First ResultsOSIRIS observations of meter-sized exposures of H2O ice at the surface of 67P/Churyumov-Gerasimenko and interpretation using laboratory experimentsQ56041050Multicolor Photometry of the Uranus Irregular Satellites Sycorax and CalibanThe rotation state of 67P/Churyumov-Gerasimenko from approach observations with the OSIRIS cameras on RosettaOn the nucleus structure and activity of comet 67P/Churyumov-GerasimenkoThe GIADA experiment for ROSETTA mission to comet 46P/wirtanen: Design and performancesGravitational slopes, geomorphology, and material strengths of the nucleus of comet 67P/Churyumov-Gerasimenko from OSIRIS observationsEvidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebblesChanges in the physical environment of the inner Coma of 67P/Churyumov-Gerasimenko with decreasing heliocentric distanceThe 2016 Feb 19 outburst of comet 67P/CG: an ESA Rosetta multi-instrument studyThe primordial nucleus of comet 67P/Churyumov-GerasimenkoThe dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 AU heliocentric distance range inboundOrbital elements of the material surrounding comet 67P/Churyumov-GerasimenkoSpectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from the OSIRIS instrument onboard the ROSETTA spacecraft67P/Churyumov-Gerasimenko: Activity between March and June 2014 as observed from Rosetta/OSIRISShape model, reference system definition, and cartographic mapping standards for comet 67P/Churyumov-Gerasimenko – Stereo-photogrammetric analysis of Rosetta/OSIRIS image dataDaily variability of Ceres’ albedo detected by means of radial velocities changes of the reflected sunlightDetection of exposed H2O ice on the nucleus of comet 67P/Churyumov-GerasimenkoThe pristine interior of comet 67P revealed by the combined Aswan outburst and cliff collapseA three-dimensional modelling of the layered structure of comet 67P/Churyumov-GerasimenkoCharacterization of dust aggregates in the vicinity of the Rosetta spacecraftConstraints on cometary surface evolution derived from a statistical analysis of 67P’s topographyDust mass distribution around comet 67P/Churyumov–Gerasimenko determined via parallax measurements using Rosetta's OSIRIS camerasEvidence of sub-surface energy storage in comet 67P from the outburst of 2016 July 03Geomorphological and spectrophotometric analysis of Seth's circular niches on comet 67P/Churyumov–Gerasimenko using OSIRIS imagesLong-term monitoring of comet 67P/Churyumov–Gerasimenko’s jets with OSIRIS onboard Rosetta
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P50
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researcher, ORCID id # 0000-0001-8435-5287
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wetenschapper
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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Marco Fulle
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P106
P1153
6701573273
P21
P31
P496
0000-0001-8435-5287