NASA has need for laboratory simulations of high velocity impacts with ice particles in order to test in-situ instruments intended for sampling material from planetary bodies such as comets and the water ice plumes of Enceladus. Specifically, beams of micrometer-size water ice grains moving in vacuum at speeds of 5 km/s or higher would be very useful. Light gas guns produce showers of high velocity ice grains that are not well controlled or well characterized, and are not easily combined with the sensitive instrumentation to be tested. Free jet molecular beam sources cannot reach velocities much greater than 2 km/s. The goal of the phase II effort is to develop and characterize an in-vacuo electrospray generator of highly charged ice grains suitable for controlled electrostatic acceleration to hyper-velocities. We will characterize the mass, charge, and speed of the ice grains using RadMet’s charge detection mass spectrometer hardware. The 2-year effort will deliver a ice grain accelerator system to NASA which aims to accelerate 1 micron particles to speeds greater than 3 km/s using just 10 kV of acceleration potential.
The ICE grain accelerator apparatus is envisioned to be adaptable to a variety of existing vacuum systems and could find use in a number of test chambers at various NASA centers. Further development of the core charge detection mass spectrometry technology could benefit the development of NASA in-situ instruments such as cosmic dust analyzers, and detectors for characterizing Lunar and Martian surface electrostatics.
Charge Detection Mass Spectrometry (CDMS) is currently being used to characterize large macromolecules such as viruses. The novel cryogenic ion source could be useful for mass spectroscopy of biological molecules.CDMS is also valuable for measuring the electric charge on particles in the pharmaceutical and agricultural industries and in the xerographic printing field.