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Main objectives were to study the outer Solar System and beyond, while radio astronomy-related discoveries include detection of radio emissions from Jupiter and studies of the solar wind.

Aimed to study Saturn and its moons. Discovered radio signals emanating from Saturn itself that are associated with auroras near the poles.

Primary mission to study Jupiter and its moons. Radio astronomy component included mapping of Jupiter's magnetic field and detection of radio emissions.

Focuses on X-ray astronomy but also has capabilities for studying radio sources. Important for high-resolution images of radio source related X-ray emissions.

While primarily for optical and ultraviolet, it has contributed to radio astronomy by identifying counterparts and sources of radio emissions.

The main objective is to study Jupiter's atmosphere, magnetic field, and gravity. Radio astronomy involvement includes the monitoring of radio waves to study Jupiter’s magnetic field.

Missions focused on Jupiter and Saturn, respectively. Radio astronomy findings included studying the solar wind and cosmic ray intensity with their onboard instruments.

Launched to study Pluto and the Kuiper Belt. Radio science experiments were used for studying the atmospheric composition and pressure of Pluto.

Designed to study the Sun's corona. It uses radio waves to understand the inner workings of the solar wind and magnetic fields.

Main mission to discover Earth-like exoplanets. Has an indirect radio astronomy connection through the study of exoplanet host stars, which sometimes are also radio sources.

While not in space, FAST is the world's largest radio telescope and its objectives include the observation of pulsars and galaxy structures.

Though primarily an infrared observatory, JWST will enhance radio observations by providing data on objects that may be sources of radio emissions.

A radio astronomy observatory that's been pivotal in astronomical discoveries. While ground-based, it has contributed to understanding radio phenomena from black holes to protoplanetary disks.

Another ground-based array, ALMA observes the universe in millimeter and submillimeter wavelengths and has discovered cold dust in the early universe and molecular gas in galaxies.