Search Publications

The dust environment of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361:20035806 Bibcode: 2004A&A...422..357F

Rauer, H.; Fulle, M.; Barbieri, C. +4 more

The new target of the ESA Rosetta Mission is comet 67P/Churyumov-Gerasimenko, which passed its last perihelion on 18 August 2002 and was well observed from fall 2002 to spring 2003. Its most prominent feature was a thin dust tail, which is best fitted by the Neck-Line model. Fits of the whole tail provide the dust environment of 67P during a year …

2004 Astronomy and Astrophysics
Rosetta 58
UV-photoprocessing of interstellar ice analogs: Detection of hexamethylenetetramine-based species
DOI: 10.1051/0004-6361:20031447 Bibcode: 2004A&A...413..209M

Schutte, W. A.; Greenberg, J. M.; Muñoz Caro, G. M. +2 more

The physical conditions governing the dense cloud environment are reproduced in a high vacuum experimental setup at low temperature T ≈ 12 K. The accretion and photoprocessing of ices on grain surfaces is simulated by depositing an ice layer on a cold finger, while it is irradiated by ultraviolet (UV) photons. After irradiation the sample is slowl…

2004 Astronomy and Astrophysics
Rosetta 56
Rosetta target comet 67P/Churyumov-Gerasimenko. Postperihelion gas and dust production rates
DOI: 10.1051/0004-6361:20040190 Bibcode: 2004A&A...422L..19S

Schulz, R.; Boehnhardt, H.; Stüwe, J. A.

The evolution of the activity and composition of the coma of ROSETTA target comet 67P/Churyumov-Gerasimenko was studied along its postperihelion orbit from 2.29 AU to 3.22 AU. The comet had a major drop of activity between 2.5 AU and 2.9 AU, which manifested most obviously in its light curve (the brightness decreased by 3 mag), but is also confirm…

2004 Astronomy and Astrophysics
Rosetta 51
Optical observations of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361:20031610 Bibcode: 2004A&A...414..749W

Rauer, H.; Weiler, M.; Helbert, J.

From longslit spectra obtained during the 1996 perihelion passage of Comet 67P/Churyumov-Gerasimenko, a CN production rate of (1.35 ± 0.35) × 1025 molecules s-1 was determined and an upper limit for the C3 production rate of 1 × 1025 molecules s-1 was derived. The dust color and dust activity …

2004 Astronomy and Astrophysics
Rosetta 48
Visible spectral properties of asteroid 21 Lutetia, target of Rosetta Mission
DOI: 10.1051/0004-6361:200400054 Bibcode: 2004A&A...425L..25L

Barbieri, C.; Lazzarin, M.; Marchi, S. +1 more

Rosetta spacecraft was successfully launched on March 2nd 2004 after its launch postponement in January 2003. Owing to this delay all the original targets, comet and asteroids, have been changed. In particular, on its 10 years journey to the new comet 67P/Churyumov-Gerasimenko, the spacecraft will pass close to the asteroid 21 Lutetia. In this pap…

2004 Astronomy and Astrophysics
Rosetta 34
Dust in Comet 67P/Churyumov-Gerasimenko
DOI: 10.1086/423268 Bibcode: 2004ApJ...613.1263M

Lara, L. M.; López-Moreno, J. J.; Moreno, F. +2 more

Comet 67P/Churyumov-Gerasimenko has been designated the new target for the ESA Rosetta mission, launched successfully on 2004 March 2. We have analyzed an image set taken in 2003 March, in which the comet appeared to have a conspicuous dust antitail. We employed a Monte Carlo code, similar to that by Fulle (1989), by which we have computed the dus…

2004 The Astrophysical Journal
Rosetta 33
A study of the electrical charging of the Rosetta orbiter: 1. Numerical model
DOI: 10.1029/2003JA009836 Bibcode: 2004JGRA..109.1104R

Berthelier, Jean-Jacques; Roussel, Jean-FrançOis

Charging of spacecraft in terrestrial or planetary ionospheres and magnetospheres is a well-known effect which may have detrimental consequences for in-situ plasma measurements. The case of the Rosetta mission is of particular importance because the expected temperatures of cometary ions and electrons in the inner coma of comet Wirtanen are very l…

2004 Journal of Geophysical Research (Space Physics)
Rosetta 18
Dust production and coma morphology of 67P/Churyumov-Gerasimenko during the 2002/2003 apparition. II. A comparative study of dust production in 46P/Wirtanen and 67P/Churyumov-Gerasimenko during their 2002/2003 apparition
DOI: 10.1051/0004-6361:20035877 Bibcode: 2004A&A...420..389K

Kidger, M. R.

A comparison is made of the light curves and and dust production of the initial target for the ROSETTA mission, 46P/Wirtanen and the new target 67P/Churyumov-Gerasimenko during their recent 2002/2003 apparition. The study is based on amateur CCD monitoring using a standardised method to produce consistent photometry in Johnson-Kron-Cousins system.…

2004 Astronomy and Astrophysics
Rosetta 18
Photochemical Concepts on the Origin of Biomolecular Asymmetry
DOI: 10.1023/B:ORIG.0000009832.71546.1d Bibcode: 2004OLEB...34..111M

Meierhenrich, Uwe J.; Thiemann, Wolfram H. -P.

Biopolymers like DNA and proteins are strongly selective towards the chirality of their monomer units. The use of homochiral monomers is regarded as essential for the construction and function of biopolymers; the emergence of the molecular asymmetry is therefore considered as a fundamental step in Chemical Evolution. This work focuses on physicoch…

2004 Origins of Life and Evolution of the Biosphere
Rosetta 18
A cometary neutral gas simulator for gas dynamic sensor and mass spectrometer calibration
DOI: 10.1029/2003JE002188 Bibcode: 2004JGRE..109.7S08G

Wurz, P.; Altwegg, K.; Balsiger, H. +6 more

The goal of the European Space Agency's Rosetta mission is a rendezvous with the Edgewood-Kuiper Belt comet 67P/Churyumov-Gerasimenko. After the initial encounter the spacecraft will accompany the comet for one to two years toward the Sun and throughout the perihelion passage. For the calibration of the onboard comet mass spectrometers a calibrati…

2004 Journal of Geophysical Research (Planets)
Rosetta 17