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Transmission Electron Microscopy of CONCORDIA UltraCarbonaceous Antarctic MicroMeteorites (UCAMMs): Mineralogical properties
DOI: 10.1016/j.gca.2011.10.025 Bibcode: 2012GeCoA..76...68D

Engrand, C.; Rouzaud, J. -N.; Duprat, J. +2 more

We performed mineralogical and petrographic studies of three UltraCarbonaceous Antarctic Micrometeorites (UCAMMs) by analytical transmission electron microscopy (TEM). The UCAMMs were identified in the CONCORDIA micrometeorite collection (2002 and 2006) recovered from central Antarctic snow, and are of probable cometary origin. UCAMMs are dominate…

2012 Geochimica et Cosmochimica Acta
Rosetta 78
The calculation of Afρ and mass loss rate for comets
DOI: 10.1016/j.icarus.2012.09.001 Bibcode: 2012Icar..221..721F

Rubin, Martin; Fink, Uwe

Ab initio calculations of Afρ are presented using Mie scattering theory and a Direct Simulation Monte Carlo (DSMC) dust outflow model in support of the Rosetta mission and its target 67P/Churyumov-Gerasimenko (CG). These calculations are performed for particle sizes ranging from 0.010 µm to 1.0 cm. The present status of our knowledge of vari…

2012 Icarus
Rosetta 72
Atomic model of the type III secretion system needle
DOI: 10.1038/nature11079 Bibcode: 2012Natur.486..276L

Baker, David; Loquet, Antoine; Sgourakis, Nikolaos G. +8 more

Pathogenic bacteria using a type III secretion system (T3SS) to manipulate host cells cause many different infections including Shigella dysentery, typhoid fever, enterohaemorrhagic colitis and bubonic plague. An essential part of the T3SS is a hollow needle-like protein filament through which effector proteins are injected into eukaryotic host ce…

2012 Nature
Rosetta 70
Interpretation of combined infrared, submillimeter, and millimeter thermal flux data obtained during the Rosetta fly-by of Asteroid (21) Lutetia
DOI: 10.1016/j.icarus.2012.08.002 Bibcode: 2012Icar..221..395K

Capaccioni, F.; Lee, S.; Hofstadter, M. +9 more

The European Space Agency’s Rosetta spacecraft is the first Solar System mission to include instrumentation capable of measuring planetary thermal fluxes at both near-IR (VIRTIS) and submillimeter-millimeter (smm-mm, MIRO) wavelengths. Its primary mission is a 1 year reconnaissance of Comet 67P/Churyumov-Gerasimenko beginning in 2014. During a 201…

2012 Icarus
Rosetta 52
The nucleus of Comet 67P/Churyumov-Gerasimenko. A new shape model and thermophysical analysis
DOI: 10.1051/0004-6361/201220116 Bibcode: 2012A&A...548A..12L

Lowry, S.; Snodgrass, C.; Green, S. F. +5 more

Context. Comet 67P/Churyumov-Gerasimenko is the target of the European Space Agency Rosetta spacecraft rendez-vous mission. Detailed physical characteristation of the comet before arrival is important for mission planning as well as providing a test bed for ground-based observing and data-analysis methods.
Aims: To conduct a long-term observa…

2012 Astronomy and Astrophysics
Rosetta eHST 52
The geomorphology of (21) Lutetia: Results from the OSIRIS imaging system onboard ESA's Rosetta spacecraft
DOI: 10.1016/j.pss.2011.10.003 Bibcode: 2012P&SS...66...96T

Jorda, L.; Stephan, K.; Lamy, P. +27 more

The surface of (21) Lutetia is highly complex with significant interactions between ancient and more recent structures. This work attempts to summarize the surface geomorphology observed using the high resolution images from OSIRIS, the imaging system onboard the European Space Agency's Rosetta spacecraft. A wide range of surface morphologies are …

2012 Planetary and Space Science
Rosetta 51
Boulders on Lutetia
DOI: 10.1016/j.pss.2011.11.004 Bibcode: 2012P&SS...66...71K

Lara, L. M.; Bertaux, J. -L.; Lamy, P. +37 more

More than 200 boulders are among the many prominent geological features seen on Lutetia by the OSIRIS cameras onboard Rosetta. Most are concentrated around the central crater in Baetica regio with a few more apparently associated with Patavium crater. The size range of boulders visible to OSIRIS is about 60-300 m. We model the trajectories of boul…

2012 Planetary and Space Science
Rosetta 49
Narrow Dust Jets in a Diffuse Gas Coma: A Natural Product of Small Active Regions on Comets
DOI: 10.1088/0004-637X/749/1/29 Bibcode: 2012ApJ...749...29C

Combi, M. R.; Fougere, N.; Gombosi, T. I. +2 more

Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring them into the inner solar system and sunlight sublimates the ice on the nucleus. Comets are also understood to have one or more active areas covering only a fraction of the total surface active with sublimating volatile ices. Calculations of the gas …

2012 The Astrophysical Journal
Rosetta 48
Shape modeling technique KOALA validated by ESA Rosetta at (21) Lutetia
DOI: 10.1016/j.pss.2011.12.018 Bibcode: 2012P&SS...66..200C

Jorda, L.; Lara, L. M.; Bertaux, J. -L. +44 more

We present here a comparison of our results from ground-based observations of asteroid (21) Lutetia with imaging data acquired during the flyby of the asteroid by the ESA Rosetta mission. This flyby provided a unique opportunity to evaluate and calibrate our method of determination of size, 3-D shape, and spin of an asteroid from ground-based obse…

2012 Planetary and Space Science
Rosetta 47
Radar properties of comets: Parametric dielectric modeling of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2012.09.023 Bibcode: 2012Icar..221..925H

Kofman, Wlodek; Heggy, Essam; Palmer, Elizabeth M. +3 more

In 2014, the European Space Agency’s Rosetta mission is scheduled to rendezvous with Comet 67P/Churyumov-Gerasimenko (Comet 67P). Rosetta’s CONSERT experiment aims to explore the cometary nucleus’ geophysical properties using radar tomography. The expected scientific return and inversion algorithms are mainly dependent on our understanding of the …

2012 Icarus
Rosetta 45