LORRI Pluto, Kuiper Belt Objects, and Comets
The Long Range Reconnaissance Imager (LORRI) is a telescopic camera built to enable distant imaging of the farthest regions of the solar system.
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L’LORRI Asteroids
The Lucy-Long Range Reconnaissance Imager (L’LORRI) is a telescopic camera built to image Jupiter’s Trojan asteroids.
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GUVI Earth
The Global Ultraviolet Imager (GUVI) observes Earth’s thermosphere, ionosphere, and mesosphere.
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MISE Outer Moons
The Mapping Imaging Spectrometer for Europa (MISE) will map elements on the surface of Jupiter’s icy moon Europa.
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EIS Outer Moons
The Europa Imaging System (EIS) will map and image Jupiter’s icy moon Europa in unprecedented resolution.
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DRACO Asteroids
The Didymos Reconnaissance and Asteroid Camera for Optical navigation (DRACO) provided asteroid imaging and spacecraft navigation on the first planetary defense mission.
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CRISM Terrestrial Planets
The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) maps minerals on the Martian surface to study how the crust formed and was altered by water.
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ULEIS Sun and Solar Wind
The Ultra Low Energy Isotope Spectrometer (ULEIS) determines the range and abundances of isotopes during massive solar events.
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IMAP-Ultra Interstellar Medium
Advancing designs built to study energetic particles around Earth and Saturn, IMAP-Ultra will image energetic particles from the edge of the solar system, providing detailed visuals of what happens when the Sun’s solar wind meets interstellar space. IMAP-Ultra is one of 10 instruments that will be included on the spacecraft.
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SIS Sun and Solar Wind
The Suprathermal Ion Spectrograph (SIS) determines elements by measuring how long it takes a particle to move through the instrument.
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PEPSSI Pluto, Kuiper Belt Objects, and Comets
The Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) is the most compact, lowest-power directional energetic-particle spectrometer flown in space.
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PIMS Giant Planets
The Plasma Instrument for Magnetic Sounding (PIMS) will use space physics to investigate Europa’s ice shell and ocean.
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JoEE/JENI Outer Moons
The Jovian Energetic Neutrals and Ions (JENI) and the Jovian Energetic Electrons (JoEE) detectors will “see” the invisible, super-heated plasma and gas around Jupiter and its icy moons.
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LECP Sun and Solar Wind
The Low-Energy Charged Particle (LECP) detectors have measured ions and electrons in the outer solar system and beyond.
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JEDI Giant Planets
The Jupiter Energetic Particle Detector Instrument (JEDI) studies Jupiter’s magnetosphere and aurora.
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EPI-Lo Sun and Solar Wind
The Energetic Particle Instrument-Low energy (EPI-Lo) is investigating the Sun’s energetic particles from an unprecedented distance.
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EPD-EIS Earth
The Energetic Ion Spectrometer (EIS) measures energetic particles to study magnetic reconnection and acceleration in Earth’s magnetosphere.
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EPAM Sun and Solar Wind
The Electron, Proton, and Alpha Monitor (EPAM) is designed to detect energetic particles from the Sun, the galaxy, and interstellar space.
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MEGANE Terrestrial Planets
The Mars-moon Exploration with GAmma rays and NEutrons (MEGANE) spectroscopy instrument will study the Martian moon Phobos.
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Psyche GRNS Asteroids
The Psyche Gamma-Ray and Neutron Spectrometer (Psyche GRNS) instrument will determine the composition of the asteroid Psyche.
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DraGNS Outer Moons
The Dragonfly Gamma-ray and Neutron Spectrometer (DraGNS) will measure the surface composition of Titan.
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DraGMet Outer Moons
The Dragonfly Geophysics and Meteorology Package (DraGMet) is a suite of geophysical and meteorological sensors to assess conditions on Saturn’s moon Titan.
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Mini-RF Moon
Mini-RF data is advancing our understanding of the lunar poles — prime targets for humankind’s return to the Moon.
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Vector Magnetometers Moon
A small rover that will explore as much as 2 kilometers (just over a mile) of one of the Moon’s most famous magnetic “swirls.”
Learn more about Vector Magnetometers