Conventional belief has held that the icy regions of our solar system and planet are too cold to support life. However, new research has suggested that below the surface of some moons, like Saturn's Enceladus, lay pockets or oceans of liquid water. In addition, lakes, rivers, and whole ecosystems have been discovered beneath glaciers, areas previously thought devoid of such features. Unfortunately, accessibility remains a primary challenge to further study of these areas. One Applied Physics Laboratory experiment aims to provide a simple and practical alternative to current ice bore-hole technology by developing a heated probe that simply melts through the ice collecting data as it descends. As part of this project, I designed and developed a thermal temperature string, to be deployed behind the probe as it descends, to monitor the conditions of the glacier at depth. The result is a sensor array capable of providing data on the internal glacial temperature for prolonged periods of time. The thermal string consists of a number of sensors evenly spaced along a 100-meter bus wire and controlled by a microcontroller. This microcontroller samples the temperature of the ice at each sensor and stores the resulting data in onboard memory. Currently, the prototype setup transmits the data to a computer, which employs software I have written to interpret this data and display the sensor temperatures. In the future, the software will apply a quadratic calibration correction to achieve expected accuracies of ±0.05°C or better, compared to ±0.5°C without it. We plan to use this sensor array as part of the available instrumentation onboard the probe in places like the Greenland ice sheet or Antarctica. The design can also be modified for other types of sensors or experiments.