Infrared reflectance spectra were measured of dark primitive asteroids in the 2 to 5 micron wavelength region. The search was for organic complexes such and CN, CH, and NH in dark material on small bodies in the solar system. A search and study was made of volatiles such as nitrogen, methane, ammonia, and carbon monoxide, both as free ices and hydrates/clathrates, on icy surfaces in the outer solar system, using high resolution spectra obtained with a multichannel cooled grating, infrared spectrometer. An absorption that can be attributed to X-C (triple bond) N in the matrix of dark materials on the primitive asteroids
Radiation processing of the surface ices of outer solar system bodies may result in the production o...
Observational testing of the idea that the distribution of water is the key to understanding the vol...
Context. The increasing sensitivity and resolution of ground-based telescopes have enabled the detec...
Spectroscopic studies with ground-based telescopes at low resolution can give compositional informat...
Small bodies hold keys to our understanding of the Solar System. By studying these populations we se...
This is an ongoing groundbased infrared study of solar system objects. This is a broadbased program ...
The compositional distribution of asteroids provides clues to understanding solar system formation a...
We have been continuing our studies of the spectral properties of dark asteroids in the solar system...
A major accomplishment during last year is the recongition of and modeling of the solid-state greenh...
Space-based facilities provide groundbreaking insight into the composition and evolutionary history ...
We investigate the spectra of asteroids at near- and mid-infrared wavelengths. In 2010 and 2011 we r...
International audienceTriton is the largest moon of the Neptune system and possesses a thin nitrogen...
The vibrational spectra from 4000 to 33 cm-1 of several modecules which may be present in the atmosp...
Infrared spectroscopy provides unique insights into the chemistry and dynamics of the atmospheres of...
Triton is the largest moon of the Neptune system and possesses a thin nitrogen atmosphere with trace...
Radiation processing of the surface ices of outer solar system bodies may result in the production o...
Observational testing of the idea that the distribution of water is the key to understanding the vol...
Context. The increasing sensitivity and resolution of ground-based telescopes have enabled the detec...
Spectroscopic studies with ground-based telescopes at low resolution can give compositional informat...
Small bodies hold keys to our understanding of the Solar System. By studying these populations we se...
This is an ongoing groundbased infrared study of solar system objects. This is a broadbased program ...
The compositional distribution of asteroids provides clues to understanding solar system formation a...
We have been continuing our studies of the spectral properties of dark asteroids in the solar system...
A major accomplishment during last year is the recongition of and modeling of the solid-state greenh...
Space-based facilities provide groundbreaking insight into the composition and evolutionary history ...
We investigate the spectra of asteroids at near- and mid-infrared wavelengths. In 2010 and 2011 we r...
International audienceTriton is the largest moon of the Neptune system and possesses a thin nitrogen...
The vibrational spectra from 4000 to 33 cm-1 of several modecules which may be present in the atmosp...
Infrared spectroscopy provides unique insights into the chemistry and dynamics of the atmospheres of...
Triton is the largest moon of the Neptune system and possesses a thin nitrogen atmosphere with trace...
Radiation processing of the surface ices of outer solar system bodies may result in the production o...
Observational testing of the idea that the distribution of water is the key to understanding the vol...
Context. The increasing sensitivity and resolution of ground-based telescopes have enabled the detec...