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Utilized to investigate the thermal properties and composition of dust, asteroids, and cometary comas.

Measures the intensity of light from stars and galaxies to determine distances and composition.

Employed to study the high-energy processes in the universe, such as star formation and the interstellar medium.

In planetary exploration, used for mineral identification and detecting organic materials.

Used to analyze the reflected sunlight from planetary surfaces, determining chemical compositions.

Provides insights into the space environment around planets by detecting energetic neutral atoms.

Enables the study of the most energetic events and objects in the universe such as gamma-ray bursts and active galactic nuclei.

Used in situ on planetary missions to directly characterize the composition of atmospheres and surfaces.

Allows the examination of cold gas clouds and cosmic microwave background radiation.