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The QCL source addresses the challenges of inefficiency, high power consumption, and bulky designs typically associated with existing solutions. It is fabricated with 80 to 100 alternating layers of semiconductor materials, each layer only a few microns thick. These layers create a cascade effect that amplifies terahertz-energy photon generation while consuming significantly less voltage. To mitigate the natural beam dissipation of QCLs, the source is integrated with a waveguide and thin optical antenna, reducing signal loss by 50%. Additionally, the waveguide employs a flared design with a diagonal feed horn, achieving high modal confinement and increasing beam coupling efficiency to 82%, compared to 37% in conventional setups. This compact design, smaller than a U.S. quarter, fits within payload constraints and enables high-powered terahertz beams for precise spectroscopic measurements. The terahertz transceiver enhances measurement precision by integrating two back-to-back hybrid couplers and Schottky diodes as detectors, providing a 35 dB dynamic range. Operating in the 2.0–3.2 THz frequency range, the transceiver is optimized for versatility across astrophysics, heliophysics, and planetary science applications. It seamlessly couples the QCL-generated signal onto the waveguide, ensuring stable and accurate spectroscopic data collection. This compact and energy-efficient transceiver delivers exceptional sensitivity, enabling it to analyze planetary materials, atmospheric components, and interstellar phenomena with unmatched resolution. With its compact, tunable design and high spectral resolution, the QCL source and transceiver represents a significant advancement for remote sensing and planetary surface characterization, offering a versatile solution for both NASA and commercial applications. The QCL system is at technology readiness level (TRL) 4 (component and/or breadboard validation in lab) and is available for patent licensing.