On Mars, the properties of CO2 radiation frost formed in a CO2 atmosphere are basically unknown, but are important to understanding the polar caps, atmosphere, and climate of Mars. The broad-band solar albedo and infrared emissivity of Martian seasonal frost deposits dominate the annual polar heat balance, which controls a significant amount of seasonal variation in atmospheric mass as well as the potential for atmospheric collapse at the extremes of Mars epochal obliquity variations. Our goal is to perform realistic laboratory simulations of the thermal and radiative environment on the surface of Mars and produce the first-ever samples of carbon dioxide frost formed the same way it does on Mars, by radiative cooling in a nearly-pure CO2 atmosphere. To create and analyze simulated Mars CO2 frost, we have been constructing a Radiation Frost Chamber (RFC). The outer shell of the chamber has already been constructed so my specific role in the research and development process is to help acquire, design, build, and test components to be used for measurements and experiments in the RFC; specifically, a fiberscope, a calibration cup, quartz beads, and other Martian soil analog materials. The fiberscope will be used to view and record the physical morphology and texture of the CO2 frost. Also, its output light will help measure the broadband and spectral albedo of the frost. The quartz beads are being used for testing a theoretical model for thermal conductivity of planetary soils and the calibration cup is going to be used for testing techniques to measure ice content of soil. The base will contain the Mars analog soil at about 600 Pa of pressure of CO2 in order to simulate the Martian environment. Once the RFC has been built it is our goal to finally simulate the Martian environment in a lab setting accurately.