Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Marla H. Moore"'
Publikováno v:
Icarus. 215:370-380
We report laboratory studies on the 0.8 MeV proton irradiation of ices composed of sulfuric acid (H2SO4), sulfuric acid monohydrate (H2SO4 H2O), and sulfuric acid tetrahydrate (H2SO4 4H2O) between 10 and 180 K. Using infrared spectroscopy, we identif
Publikováno v:
Icarus. 210:480-487
The radiation chemistry, thermal stability, and vapor pressure of solid-phase carbonic acid (H2CO3) have been studied with mid-infrared spectroscopy. A new procedure for measuring this molecule's radiation stability has been used to obtain intrinsic
Publikováno v:
The Astrophysical Journal Supplement Series. 191:96-112
Spectra and optical constants of nitrile ices known or suspected to be in Titan's atmosphere are presented from 2.0 to 333.3 μm (~5000-30 cm–1). These results are relevant to the ongoing modeling of Cassini CIRS observations of Titan's winter pole
Autor:
Marla H. Moore, Reggie L. Hudson
Publikováno v:
The Astrophysical Journal. 857:89
Infrared spectra of ices containing alcohols that are known or potential interstellar molecules are examined before and after irradiation with 1 MeV protons at ~20 K. The low-temperature oxidation (hydrogen loss) of six alcohols is followed, and conc
Publikováno v:
Icarus. 203:677-680
We report recent experiments on ethane ices made at temperatures applicable to the outer Solar System. New near- and mid-infrared data for crystalline and amorphous ethane, including new spectra for a seldom-studied solid phase that exists at 35-55 K
Publikováno v:
The Astrophysical Journal. 684:1210-1220
Extensive experimental studies have been performed on the solid-state formation of the OCS molecule in proton-irradiated water-free and water-dominated ices containing CO or CO2 as the carbon source and H2S or SO2 as the sulfur source. In each case O
Autor:
Reggie L. Hudson, Marla H. Moore
Publikováno v:
Astrobiology. 8:362-371
Publikováno v:
Icarus. 194:379-388
The chemistry and spectroscopy of proton-irradiated H2O + O2 ices have been investigated in relation to the production of oxidants in icy satellite surfaces. Hydrogen peroxide (H2O2), ozone (O3), and the hydroperoxy (HO2) and hydrogen trioxide (HO3)
Publikováno v:
Icarus. 190:260-273
Although water- and ammonia-ices have been observed or postulated as important components of the icy surfaces of planetary satellites in the outer Solar System, significant gaps exist in our knowledge of the spectra and behavior of such mixtures unde
Publikováno v:
Icarus. 189:409-423
Spectra of Europa, Ganymede, and Callisto reveal surfaces dominated by frozen water, hydrated materials, and minor amounts of SO2, CO2, and H2O2. These icy moons undergo significant bombardment by jovian magnetospheric radiation (protons, electrons,