Add to ORKGThe ν3 vibrational band of H2O at 2.67 μm was observed with the high spectral-resolution channel of the Visible InfraRed Thermal Imaging Spectrometer (VIRTIS-H) onboard Rosetta. The spectral resolution is adequate to resolve the rovibrational structure of the band. High signal-to-noise ratios allow us to measure both the rotational temperature and the ortho-para ratio of water (OPR) in comet 67P/C-G. The measured OPR value will be presented and compared to measurements obtained in other comets from ground-based and space telescopes
Heat transport and ice sublimation in comets are interrelated processes reflecting properties acquir...
The Rosetta spacecraft has reached its final target, comet 67P/Churyumov-Gerasimenko, in early Augus...
Highlights of Astronomy. 2002. vol. 12Cometary water, the main constituent of nucleus ices, is diffi...
International audienceContext. Abundance ratios of the nuclear-spin isomers of H2O and NH3 have been...
Using the high spectral-resolution channel of the Visible InfraRed Thermal Imaging Spectrometer (V...
The paper will describe the major results obtained throughout the nominal mission by the instrument ...
VIRTIS (Visible Infrared and Thermal Imaging Spectrometer) is the spectrometer onboard the Rosetta/E...
Since August 2014, the VIRTIS imaging spectrometer onboard the Rosetta ESA spacecraft has intensivel...
Since July 2014, the Visual IR Thermal Imaging Spectrometer (VIRTIS) onboard the ESA’s Rosetta s...
Taking advantage of Rosetta’s terminator orbits around 67P/CG nucleus in December 2014, VIRTIS-M, t...
Context. Outgassing from cometary nuclei involves complex surface and subsurface processes that need...
International audienceThe VIRTIS spectrometer on the Rosetta mission performed infrared observations...
After a cruise phase of more than ten years the Rosetta spacecraft entered orbit around comet 67P/Ch...
Context. Studying the coma environment of comet 67P/Churyumov-Gerasimenko (67P) is one of the primar...
Infrared observations of the coma of 67P/Churyumov-Gerasimenko were carried out from 2015 July to Se...
Heat transport and ice sublimation in comets are interrelated processes reflecting properties acquir...
The Rosetta spacecraft has reached its final target, comet 67P/Churyumov-Gerasimenko, in early Augus...
Highlights of Astronomy. 2002. vol. 12Cometary water, the main constituent of nucleus ices, is diffi...
International audienceContext. Abundance ratios of the nuclear-spin isomers of H2O and NH3 have been...
Using the high spectral-resolution channel of the Visible InfraRed Thermal Imaging Spectrometer (V...
The paper will describe the major results obtained throughout the nominal mission by the instrument ...
VIRTIS (Visible Infrared and Thermal Imaging Spectrometer) is the spectrometer onboard the Rosetta/E...
Since August 2014, the VIRTIS imaging spectrometer onboard the Rosetta ESA spacecraft has intensivel...
Since July 2014, the Visual IR Thermal Imaging Spectrometer (VIRTIS) onboard the ESA’s Rosetta s...
Taking advantage of Rosetta’s terminator orbits around 67P/CG nucleus in December 2014, VIRTIS-M, t...
Context. Outgassing from cometary nuclei involves complex surface and subsurface processes that need...
International audienceThe VIRTIS spectrometer on the Rosetta mission performed infrared observations...
After a cruise phase of more than ten years the Rosetta spacecraft entered orbit around comet 67P/Ch...
Context. Studying the coma environment of comet 67P/Churyumov-Gerasimenko (67P) is one of the primar...
Infrared observations of the coma of 67P/Churyumov-Gerasimenko were carried out from 2015 July to Se...
Heat transport and ice sublimation in comets are interrelated processes reflecting properties acquir...
The Rosetta spacecraft has reached its final target, comet 67P/Churyumov-Gerasimenko, in early Augus...
Highlights of Astronomy. 2002. vol. 12Cometary water, the main constituent of nucleus ices, is diffi...