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P. J. Gutiérrez

Researcher at Spanish National Research Council

Publications -  51
Citations -  3285

P. J. Gutiérrez is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Comet & Comet dust. The author has an hindex of 30, co-authored 51 publications receiving 2932 citations.

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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.
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Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar System

Holger Sierks, +60 more
- 28 Oct 2011 - 
TL;DR: A spacecraft flyby of an asteroid reveals a high-density body that is more like a planetesimal than a rubble pile, which contrasts with smaller asteroids visited by previous spacecraft, which are probably shattered bodies, fragments of larger parents, or reaccumulated rubble piles.
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Spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from the OSIRIS instrument onboard the ROSETTA spacecraft

TL;DR: In this paper, the photometric and spectrophotometric properties of the nucleus of the comet 67P/Churyumov-Gerasimenko (67P) were derived from the OSIRIS imaging system, which consists of a WAC and a Narrow Angle Camera (NAC).
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Insolation, erosion, and morphology of comet 67P/Churyumov-Gerasimenko

TL;DR: In this article, the authors investigate the insolation of the cometary surface in order to predict the sublimation of water ice, and they use a two-layer model of a thin porous dust cover above an icy surface.
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Evolution of the Dust Size Distribution of Comet 67P/Churyumov-Gerasimenko from 2.2. AU to Perihelion

Marco Fulle, +81 more
TL;DR: The Rosetta probe, orbiting Jupiter-family comet 67P/Churyumov-Gerasimenko, has been detecting individual dust particles of mass larger than 10−10 kg by means of the GIADA dust collector and the OSIRIS Wide Angle Camera and Narrow Angle Camera as mentioned in this paper.