First Principles Based Reactive Atomistic Simulations to Understand the Effects of Molecular Hypervelocity Impact on Cassini’s Ion and Neutral Mass
نویسندگان
چکیده
Introduction: NASA's Cassini Cassini's Ion and Neutral Mass Spectrometer (INMS) has returned a wealth of data on the composition of Titan's upper atmosphere and the plumes of Enceladus. However the encounter velocity (up to 17.73 km/sec) of the spacecraft with the plume or atmosphere has profound effects on the fragmentation of the observed molecules. Measured compositional changes of H 2 O, H 2 , CO 2 and CO appear to be correlated with velocity (see Figure 1). To understand this phenomenon , we have applied first principles based atomistic methods to simulate the physics of hy-pervelocity impacts of organic and inorganic molecules on metal surfaces. These methods include non-adiabatic and adiabatic reactive molecular dynamics calculations designed to elucidate the relationship between impact energy, fragmentation efficiency and fragmentation pathways. We report here on the predicted impact of species such as ice-water, CO 2 , CH 4 , and NH 3 , on oxidized titanium, as well as HC species on diamond surfaces. These simulations provide the dynamics of product distributions during and after a hypervelocity impact event, ionization fractions, and dissociation probabilities for the various species of interest as a function of impact velocity (energy). We are using these results to determine the relevance of the fragmentation process to Cassini INMS results, and to quantify its effects on the observed spectra. The Ion and Neutral Mass Spectrometer (INMS): The INMS is a quadrupole mass spectrometer equipped with two separate ion sources, the closed source and the open source. Data on the composition of the Enceladus plumes and the upper atmosphere of Titan has primarily been obtained with the closed source, whose operation we will briefly describe. The closed source is made up of a spherical titanium antechamber which is connected to a hot filament electron impact ionizer by means of a transfer tube[1]. The ionizer fragments and ionizes the incident molecules before they are focused in the quadrupole for mass analysis. The fragmentation patterns are an important means of identifying the parent molecules, and an accurate knowledge of these is necessary to deconvolute the overlapping peaks that result from the mixture of gases entering the mass spectrometer. Gas enters the antechamber through the entrance aperture, and is thermalized through collision with the antechamber walls before entering the ionizer. This arrangement achieves a ram enhancement of the gas pressure in the antechamber above that of the ambient gas, due to the high …
منابع مشابه
Hypervelocity Impact Effect of Molecules from Enceladus’ Plume and Titan’s Upper Atmosphere on NASA’s Cassini Spectrometer from Reactive Dynamics Simulations
The NASA/ESA Cassini probe of Saturn analyzed the molecular composition of plumes emanating from one of its moons, Enceladus, and the upper atmosphere of another, Titan. However, interpretation of this data is complicated by the hypervelocity (HV) flybys of up to ∼18 km/sec that cause substantial molecular fragmentation. To interpret this data we use quantum mechanical based reactive force fiel...
متن کاملHypervelocity impact effect of molecules from Enceladus' plume and Titan's upper atmosphere on NASA's Cassini spectrometer from reactive dynamics simulation.
The NASA/ESA Cassini probe of Saturn analyzed the molecular composition of plumes emanating from one of its moons, Enceladus, and the upper atmosphere of another, Titan. However, interpretation of this data is complicated by the hypervelocity (HV) flybys of up to ~18 km/sec that cause substantial molecular fragmentation. To interpret this data we use quantum mechanical based reactive force fiel...
متن کاملLarge-scale Molecular Simulations of Hypervelocity Impact of Materials
We describe the application of the ReaxFF reactive force field with short-range distance-dependent exponential inner wall corrections and the non-adiabatic electron Force Field (eFF) for studying the hypervelocity impact (HVI) effects on material properties. In particular, to understanding nonequilibrium energy/mass transfer, high strain/heat rate material decomposition, defects formation, plas...
متن کاملEffects of different atomistic water models on the velocity profile and density number of Poiseuille flow in a nano-channel: Molecular Dynamic Simulation
In the current study, five different atomistic water models (AWMs) are implemented, In order to investigate the impact of AWMs treatment on the water velocity profile and density number. For this purpose, Molecular dynamics simulation (MDS) of Poiseuille flow in a nano-channel is conducted. Considered AWMs are SPC/E, TIP3P, TIP4P, TIP4PFQ and TIP5P. To assessment of the ability of each model in...
متن کاملMultimillion Atom Reactive Simulations of Nanostructured Energetic Materials
For large-scale atomistic simulations involving chemical reactions to study nanostructured energeticmaterials, we have designed linear-scaling molecular dynamics algorithms: 1) first-principles-based fast reactive force field molecular dynamics, and 2) embedded divide-and-conquer density functional theory on adaptive multigrids for quantum-mechanical molecular dynamics. These algorithms have ac...
متن کامل