Search Publications

Thermal desorption of circumstellar and cometary ice analogs
DOI: 10.1051/0004-6361/201322824 Bibcode: 2014A&A...564A...8M

Martín-Doménech, R.; Muñoz Caro, G. M.; Bueno, J. +1 more

Context. Thermal annealing of interstellar ices takes place in several stages of star formation. Knowledge of this process comes from a combination of astronomical observations and laboratory simulations under astrophysically relevant conditions.
Aims: For the first time we present the results of temperature programmed desorption (TPD) experi…

2014 Astronomy and Astrophysics
Rosetta 100
The rotation state of 67P/Churyumov-Gerasimenko from approach observations with the OSIRIS cameras on Rosetta
DOI: 10.1051/0004-6361/201424590 Bibcode: 2014A&A...569L...2M

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +46 more


Aims: Approach observations with the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) experiment onboard Rosetta are used to determine the rotation period, the direction of the spin axis, and the state of rotation of comet 67P's nucleus.
Methods: Photometric time series of 67P have been acquired by OSIRIS since the pos…

2014 Astronomy and Astrophysics
Rosetta 89
Formation of pebble-pile planetesimals
DOI: 10.1051/0004-6361/201424369 Bibcode: 2014A&A...570A..47W

Johansen, Anders; Wahlberg Jansson, Karl

Asteroids and Kuiper belt objects are remnant planetesimals from the epoch of planet formation. The first stage of planet formation is the accumulation of dust and ice grains into mm- and cm-sized pebbles. These pebbles can clump together through the streaming instability and form gravitationally bound pebble clouds. Pebbles inside such a cloud wi…

2014 Astronomy and Astrophysics
Rosetta 68
Methanol along the path from envelope to protoplanetary disc
DOI: 10.1093/mnras/stu1789 Bibcode: 2014MNRAS.445..913D

Walsh, Catherine; Harsono, Daniel; van Dishoeck, Ewine F. +2 more

Interstellar methanol is considered to be a parent species of larger, more complex organic molecules. A physicochemical simulation of infalling parcels of matter is performed for a low-mass star-forming system to trace the chemical evolution from cloud to disc. An axisymmetric 2D semi-analytic model generates the time-dependent density and velocit…

2014 Monthly Notices of the Royal Astronomical Society
Rosetta 61
Plasma environment of a weak comet - Predictions for Comet 67P/Churyumov-Gerasimenko from multifluid-MHD and Hybrid models
DOI: 10.1016/j.icarus.2014.07.021 Bibcode: 2014Icar..242...38R

Altwegg, K.; Glassmeier, K. -H.; Richter, I. +8 more

The interaction of a comet with the solar wind undergoes various stages as the comet's activity varies along its orbit. For a comet like 67P/Churyumov-Gerasimenko, the target comet of ESA's Rosetta mission, the various features include the formation of a Mach cone, the bow shock, and close to perihelion even a diamagnetic cavity. There are differe…

2014 Icarus
Rosetta 59
Astra: Interdisciplinary study on enhancement of the end-to-end accuracy for spacecraft tracking techniques
DOI: 10.1016/j.actaastro.2013.06.011 Bibcode: 2014AcAau..94..699I

Iess, Luciano; Tortora, Paolo; Di Benedetto, Mauro +3 more

Navigation of deep-space probes is accomplished through a variety of different radio observables, namely Doppler, ranging and Delta-Differential One-Way Ranging (Delta-DOR). The particular mix of observations used for navigation mainly depends on the available on-board radio system, the mission phase and orbit determination requirements. The accur…

2014 Acta Astronautica
Rosetta 55
Temperature dependence of the sublimation rate of water ice: Influence of impurities
DOI: 10.1016/j.icarus.2014.01.025 Bibcode: 2014Icar..233..101K

Kossacki, Konrad J.; Leliwa-Kopystynski, Jacek

The sublimation rate of ice is commonly calculated using the simple Hertz-Knudsen formula. This formula is derived from the kinetic theory of gases and ignores microphysical processes determining the actual sublimation rate. The microphysical processes can be accounted for by including the temperature dependent sublimation coefficient (Kossacki, K…

2014 Icarus
Rosetta 41
How to link the relative abundances of gas species in coma of comets to their initial chemical composition?
DOI: 10.1016/j.icarus.2014.07.001 Bibcode: 2014Icar..242..225M

Marboeuf, Ulysse; Schmitt, Bernard

Comets are expected to be the most primitive objects in the Solar System. The chemical composition of these objects is frequently assumed to be directly provided by the observations of the abundances of volatile molecules in the coma. The present work aims to determine the relationship between the chemical composition of the coma, the outgassing p…

2014 Icarus
Rosetta 37
An Early Look of Comet C/2013 A1 (Siding Spring): Breathtaker or Nightmare?
DOI: 10.1088/0004-637X/787/2/115 Bibcode: 2014ApJ...787..115Y

Ye, Quan-Zhi; Hui, Man-To

The dynamically new comet, C/2013 A1 (Siding Spring), is to make a close approach to Mars on 2014 October 19 at 18:30 UT at a distance of 40 ± 1 Martian radii. Such an extremely rare event offers a precious opportunity for the spacecrafts on Mars to closely study a dynamically new comet itself as well as the planet-comet interaction. Meanwhile, th…

2014 The Astrophysical Journal
Rosetta 32
Giada: its Status after the Rosetta Cruise Phase and On-Ground Activity in Support of the Encounter with Comet 67P/CHURYUMOV-GERASIMENKO
DOI: 10.1142/S2251171713500116 Bibcode: 2014JAI.....350011D

Lamy, P.; Fulle, M.; Rodrigo, R. +33 more

GIADA (Grain Impact Analyser and Dust Accumulator) on-board the Rosetta mission to comet 67P/Churyumov-Gerasimenko was designed to study the physical and dynamical properties of dust particles ejected by the comet during the encounter. In this paper we report the results of the analysis of data collected by GIADA during the past seven years of the…

2014 Journal of Astronomical Instrumentation
Rosetta 28