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

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

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

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

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

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.

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

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