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Dragonfly Science

NASA's Dragonfly, the first-of-its-kind rotorcraft to explore another world, will fly to various locations on Saturn’s moon Titan and investigate the moon’s habitability.

Dragonfly close up

Exploring Titan

Titan was discovered in 1655 by Dutch astronomer Christiaan Huygens, who called it Luna Saturni, or Saturn’s moon. In 1847, British astronomer John Herschel gave Titan and the other six then-known satellites of Saturn their names, which are still used today.

The NASA-ESA Cassini-Huygens mission spent more than a decade relaying spectacular images and trailblazing data from Saturn and its moons until its mission end in 2017. Among the myriad findings about Titan was the discovery of a vast ocean some 35-50 miles (55-80 km) below that moon’s icy surface.

NASA’s exploration of ocean worlds – such as the Europa Clipper mission currently on its way to collect data from the vast ocean beneath the icy crust of Jupiter’s moon Europa – looks for signs of habitability in carbon-rich organic molecules. Titan’s complex chemistry on its ice surface makes it an ideal destination for such examination.

Artist's concept of Cassini during the Saturn orbit insertion maneuver.
NASA/JPL-Caltech

Dragonfly Science at Titan

  • Surface and atmospheric science observations

    Sampling surface material and measuring molecular compositions with a mass spectrometer to identify the chemical components and processes that produce biologically relevant compounds.

    Measuring bulk elemental surface composition with a neutron-activated gamma-ray spectrometer.

    Monitoring atmospheric and surface conditions, including diurnal and spatial variations, with meteorology and geophysics sensors.

    Performing seismic studies to detect subsurface activity.

    Imaging at a range of spatial scales to characterize surface materials and geologic features.

    A mountainous formation on Titan with a lake and cloudy atmosphere.
    Artist's concept of a hydrocarbon lake and methane rain clouds on Titan
    Jenny McElligott/eMITS
  • In-flight measurements

    Atmospheric profiles.

    Aerial images of surface geology.

    Providing context for surface measurements.

    Scouting of potential future landing sites of interest.

    A stitched image of a mountainous formation on Titan
    Huygens captured this aerial view of Titan from an altitude of 33,000 feet.
    ESA/NASA/JPL/University of Arizona