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Ivano Bertini

Researcher at University of Padua

Publications -  175
Citations -  8842

Ivano Bertini is an academic researcher from University of Padua. The author has contributed to research in topics: Comet & Asteroid. The author has an hindex of 47, co-authored 168 publications receiving 7614 citations. Previous affiliations of Ivano Bertini include Versailles Saint-Quentin-en-Yvelines University & Spanish National Research Council.

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On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko

Holger Sierks, +70 more
- 23 Jan 2015 - 
TL;DR: Images from the OSIRIS scientific imaging system onboard Rosetta show that the nucleus of 67P/Churyumov-Gerasimenko consists of two lobes connected by a short neck, which raises the question of whether the two Lobes represent a contact binary formed 4.5 billion years ago, or a single body where a gap has evolved via mass loss.
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Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the Sun

Alessandra Rotundi, +90 more
- 23 Jan 2015 - 
TL;DR: In this article, the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko was used to detect 35 outflowing grains of mass 10−10 to 10−7 kilograms.
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The morphological diversity of comet 67P/Churyumov-Gerasimenko

TL;DR: Images of comet 67P/Churyumov-Gerasimenko acquired by the OSIRIS imaging system onboard the European Space Agency’s Rosetta spacecraft offer some support for subsurface fluidization models and mass loss through the ejection of large chunks of material.
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The global shape, density and rotation of Comet 67P/Churyumov-Gerasimenko from preperihelion Rosetta/OSIRIS observations

TL;DR: In this article, a high-resolution shape model of the nucleus of the comet 67P/Churyumov-Gerasimenko was used to estimate the porosity of the surface of the cometary nucleus.
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Shape model, reference system definition, and cartographic mapping standards for comet 67P/Churyumov-Gerasimenko Stereo-photogrammetric analysis of Rosetta/OSIRIS image data

TL;DR: In this article, the authors used stereo-photogrammetric methods (SPG) to analyze the rotational elements of 67P and derived a volume for the northern hemisphere of 9.35 km3 ± 0.1 km3.