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Churyumov-Gerasimenko Comet

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Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 95–100.
... trace their heritage to the interstellar medium from which the protosolar nebula eventually emerged. The most recent cometary space mission, Rosetta , carried instruments designed to characterize, in unprecedented detail, the organic species in comet 67P/ChuryumovGerasimenko (67P). Rosetta...
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Exploration of <span class="search-highlight">comet</span> 67P&#x2F;<span class="search-highlight">Churyumov</span>-<span class="search-highlight">Gerasimenko</span> by the ESA-NASA Rosetta prob...
Published: 01 October 2020
Figure 7.2 Exploration of comet 67P/Churyumov-Gerasimenko by the ESA-NASA Rosetta probe. (a) 67P/G-C upon arrival. (b) Artist’s view of the Rosetta spacecraft, with insert showing the double focusing mass spectrometer (DFMS) of the ROSINA instrument that analysed volatiles released
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Panoramic view of <span class="search-highlight">comet</span> 67P&#x2F;<span class="search-highlight">Churyumov</span>–<span class="search-highlight">Gerasimenko</span> taken by  Rosetta &#x27;s OSIR...
Published: 01 April 2018
Figure 1 Panoramic view of comet 67P/ChuryumovGerasimenko taken by Rosetta 's OSIRIS narrow-angle camera on 3 August 2014 from a distance of 285 km. The comet is 4.3 km in its longest dimension and 4.1 km at its widest. Image Id: 317032. Image credit: ESA/Rosetta/MPS for OSIRIS Team.
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An agglomerate dust particle from <span class="search-highlight">comet</span> 67P&#x2F;<span class="search-highlight">Churyumov</span>–<span class="search-highlight">Gerasimenko</span>, as colle...
Published: 01 June 2016
F igure 5 An agglomerate dust particle from comet 67P/ChuryumovGerasimenko, as collected by COSIMA (cometary secondary ion mass analyzer). The image was obtained using grazing illumination from the right. The length of the shadows indicates that the altitude above the substrate reaches about
Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 101–106.
... ). The Rosetta mission also observed strong dichotomies in the relative ratios of CO 2 /H 2 O between the northern and southern hemispheres of comet 67P/ChuryumovGerasimenko, as well as changing mixing ratios of less abundant molecules, as seen from in situ near-IR measurements ( Hässig et al. 2015 ). However...
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Journal Article
Published: 01 October 2020
Geochemical Perspectives (2020) 9 (2): 242–253.
...Figure 7.2 Exploration of comet 67P/Churyumov-Gerasimenko by the ESA-NASA Rosetta probe. (a) 67P/G-C upon arrival. (b) Artist’s view of the Rosetta spacecraft, with insert showing the double focusing mass spectrometer (DFMS) of the ROSINA instrument that analysed volatiles released...
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Journal Article
Journal: Elements
Published: 01 February 2024
Elements (2024) 20 (1): 31–37.
... to 0.035 ( Yabuta et al. 2023 ) and are within the range of N/C ratios of IOM in carbonaceous chondrites and those of organic particles from comet 67P/ChuryumovGerasimenko (e.g., Yabuta et al. 2017 ; Fray et al. 2017 ; F ig . 4 ). Organic matter from particles from comet 81P/Wild2, interplanetary dust...
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Journal Article
Journal: Elements
Published: 01 June 2016
Elements (2016) 12 (3): 185–189.
...F igure 5 An agglomerate dust particle from comet 67P/ChuryumovGerasimenko, as collected by COSIMA (cometary secondary ion mass analyzer). The image was obtained using grazing illumination from the right. The length of the shadows indicates that the altitude above the substrate reaches about...
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Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 87–93.
... by spacecraft. Prior to the investigation of comet 67P/ChuryumovGerasimenko by the European Space Agency's Rosetta mission (Grady et al. 2018 this issue), there had been close encounters with six other comets ( Fig. 1 ). Rosetta included both a rendezvous spacecraft for extended measurements near...
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Journal Article
Journal: Elements
Published: 01 February 2024
Elements (2024) 20 (1): 7–12.
... organic molecules in the icy particles of a protoplanetary disk were detected using NASA’s newly launched James Webb Space Telescope (JWST) ( Yang et al. 2022 ). Previously, the Rosetta space mission detected large organic molecules in the dust particles of comet ChuryumovGerasimenko (67P/CG), which...
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Journal Article
Journal: Elements
Published: 01 February 2024
Elements (2024) 20 (1): 19–23.
..., have been detected in comets ( Biver and Bockelée-Morvan 2019 ). In-situ space missions, such as the Rosetta mission to comet 67P/ChuryumovGerasimenko have further identified more than 60 individual organic molecules ( Altwegg et al. 2017 ), including glycine, alcohols, carbonyls, amines, nitriles...
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The N/C elemental ratio of Ryugu’s macromolecular organic matter ( Y abuta ...
Published: 01 February 2024
Figure 4. The N/C elemental ratio of Ryugu’s macromolecular organic matter ( Y abuta et al . 2023 ) is compared with those of organic solids in various extraterrestrial materials, such as insoluble organic matter (IOM) in carbonaceous chondrites, organic particles from comet 67P/Churyumov
Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 107–112.
.... Comets and their meteoroids have a low density. Matter must have assembled with low relative speed to create the contact-binary and onion-shell morphology of comet 67P/ChuryumovGerasimenko, observed in close proximity by the Rosetta mission (see Grady et al. 2018 this issue). Once they had formed...
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Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 75.
... imagination in a way little else can. Who could not be enthralled by the evocatively named Stardust mission returning a few thousand grains of dust from comet Wild 2 to Earth? We collectively shared the despair when communication was lost from Rosetta 's Philae lander on comet 67P/ChuryumovGerasimenko...
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Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 83–86.
... orders of magnitude (see Fig. 2 ). In the latest giant step, the Rosetta spacecraft orbited, and deposited a probe on comet 67P/ChuryumovGerasimenko, as described by Grady et al. (2018 this issue). In many ways, we live at the perfect time to be “cometologists”. However, the mission that most...
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( A ) Closeup of <span class="search-highlight">comet</span> 103P&#x2F;Hartley 2 (∼1.6 km in diameter) from the  EPOXI...
Published: 01 April 2018
Figure 2 ( A ) Closeup of comet 103P/Hartley 2 (∼1.6 km in diameter) from the EPOXI mission, showing the night-side jet activity driven by subsurface CO 2 sublimation. Credit: NASA/JPL-Caltech/UMD. ( B ) Mass spectrum (mass-to-charge ratio, m/z) from the coma of 67P/ChuryumovGerasimenko
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Mass spectra of the local environment taken 20 minutes after first touchdow...
Published: 01 April 2018
Figure 4 Mass spectra of the local environment taken 20 minutes after first touchdown of Philae on the surface of comet 67P/ChuryumovGerasimenko. Spectra are plotted as counts versus molar mass (in daltons, symbol Da) ( A ) Spectra from the COSAC instrument. Spectra A redrawn from Goesmann et
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Examples of extraterrestrial case hardening. ( A ) Image of the surface of ...
Published: 01 June 2017
Figure 8 Examples of extraterrestrial case hardening. ( A ) Image of the surface of comet 67P/ChuryumovGerasimenko (view is ~900 m across). While dust appears to generate smooth surfaces, unknown agents have created induration features, as evidenced by eroded edges of the crust (arrowed). Image
Journal Article
Journal: Geology
Published: 01 August 2023
Geology (2023) 51 (10): 947–951.
... that can be seen from orbit; these patterns have been reported on Venus, Earth, Mars, Titan, Io, Pluto, and the 67P/Churyumov-Gerasimenko comet ( Fig. 1 ; Bourke et al., 2010 ; Thomas et al., 2015 ; Telfer et al., 2018 ; McDonald et al., 2022 ). Because dunes and their patterns form and evolve...
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Visual properties of terrain and photo-textured surfaces in LIME. (A) Three...
Published: 10 January 2019
/Churyumov-Gerasimenko (credit: European Space Agency–Rosetta navcam; used under Creative Commons license BY-SA IGO 3.0, http://creativecommons.org/licenses/by-sa/3.0/igo/ ), shaded according to surface normal mapped to red, green, blue (RGB) color space, and with 100 m contour interval. Comet is ∼4 km