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

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

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

Used to investigate high-energy phenomena such as black holes, neutron stars, and supernova remnants.

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

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

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

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

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