
IDEX Instrument
The The Interstellar Dust Experiment (IDEX) instrument collects and analyzes interstellar dust and interplanetary dust particles found in our solar system to better understand their compositions, the speeds they travel, their concentrations within our solar system, and their interactions with the solar wind. instrument collects and analyzes Tiny particles of solid matter found in the interstellar medium that are believed to be formed from supernova star events that result in the formation of stars and planetary systems, including those found in our solar system. and The small particles of solid matter that are believed to originate from comets and asteroids found between planets in a system. particles found in our solar system to understand better their compositions, the speeds they travel, their concentrations within our solar system, and their interactions with the A stream of charged particles, mostly protons and electrons, that escapes into the Sun's outer atmosphere at high speeds and streams out into the solar system in all directions..
Interstellar dust are the small particles of solid matter that are believed to be formed from An explosive death of a star much bigger (more massive) than our Sun; a brilliant burst of light that occurs when a star reaches the end of its life cycle. star events that result in the formation of stars and planetary systems, including our very own. Interplanetary dust is similar but originates from comets and asteroids and is found between planets in a system.
Measuring the The specific components or “ingredients” that make up a substance or type of matter. and velocity of these dust particles helps scientists understand what is found in the The interstellar medium is the matter that exists in the space between the stars within a galaxy. This matter includes ionized and electrically neutral gas (primarily hydrogen and helium), dust, and cosmic rays. The ISM plays a crucial role in the lifecycle of stars and galaxies. It is the reservoir from which new stars are born and into which old stars expel material when they die. beyond, what can be found in the in-between spaces of our solar system, as well as what the The bubble-like region surrounding the solar system inflated by the solar wind, shielding the solar system from interstellar radiation. is made up of.
How It Works
A spring-activated door protects The Interstellar Dust Experiment (IDEX) instrument collects and analyzes interstellar dust and interplanetary dust particles found in our solar system to better understand their compositions, the speeds they travel, their concentrations within our solar system, and their interactions with the solar wind.’s sensor head from contamination while it is being integrated into the spacecraft and during launch. In space, the door swings open permanently, allowing interstellar and The small particles of solid matter that are believed to originate from comets and asteroids found between planets in a system. to flow into the instrument.
The collected dust passes through three sets of charged grids toward an impact target plate coated with pure gold. The grids prevent charged particles, electrons, and ions, from entering the instrument.
In a process called impact The process by which ions are produced, typically occurring by collisions with atoms or electrons ("collisional ionization") or by interaction with electromagnetic radiation ("photoionization")., the dust crashes into the gold-coated target at a high speed, smashing the dust grains into their composite ions – tiny, charged particles. These fragments then spray upwards and are directed through an opening at the center of the gold target to a An instrument which is used to discover that something is present somewhere, or to measure how much of something there is. that counts the number of ions that are received.
The ringed structure surrounding the instrument and shield-like A device used in the particle-detection instrument to improve the velocity measurements it makes. It uses an electric field to reflect ions back through a space, effectively lengthening their path and correcting for small differences in their energies, resulting in sharper and more precise time-of-flight measurements. at the top of the assembly use electric fields to keep the ions from escaping and direct them towards the detector. This also works to form a simple A measure of the flow of events.-of-flight (ToF) system by timing how long it takes the An atom that has become electrically charged by the gain or loss of one or more electrons. to reach the detector after impact ionization. Scientists use the amount of time and distance traveled from the target, up to the electric field and down to the detector to identify what elements the dust particles were made of. The heavier fragments (ions) of the dust move slower than smaller fragments, which means they are heavier elements such as iron and silicon. Faster ones are lighter elements, such as helium or hydrogen.
The final detector below the center counts the number of tiny dust particles collected by IDEX by measuring the amount of electrical charge they carry. Because space dust ions are so tiny, even a group of 1000 would not have a big enough charge for a sensor to pick up, so the charges need to be multiplied, or increased, to be detected.
This detector consists of a series of specially designed, electrically charged perforated disks, called dynodes, that have peaks and valleys surrounding each tiny hole. As the ions come through the opening in the middle of the gold target, they contact a peak of the The visible surface of the Sun (or any heavenly body) projected against the sky. that increases the ion’s charge and funnels it through the hole in the valley to the next disk where the charge is multiplied again as it meets the next peak. The ion is passed through the other disks like a pinball hitting bumpers, increasing its charge as it continues. By the time the particle reaches the final detector surface, the charge is large enough that it can be sensed and counted.
The impacts on IDEX’s gold-coated target leave a residue that can contaminate future collection of data. IDEX periodically on a previously set schedule heats up the target to high A measure of the average random speeds of the microscopic particles in a substance. that gets rid of this residue.
Explore the IDEX Model
Capturing StarDust
[This video has no sound.] Watch how IDEX captures stardust on the IMAP mission and uses it to understand better how life is possible on Earth.
How We Use IDEX Data
The Interstellar Dust Experiment (IDEX) instrument collects and analyzes interstellar dust and interplanetary dust particles found in our solar system to better understand their compositions, the speeds they travel, their concentrations within our solar system, and their interactions with the solar wind. reveals the The specific components or “ingredients” that make up a substance or type of matter. of the interstellar and interplanetary material locked in the dust grains. This helps gives scientists critical insight on the formation and evolution of matter both inside and outside our solar neighborhood. Composition data from IDEX also links the makeup of Tiny particles of solid matter found in the interstellar medium that are believed to be formed from supernova star events that result in the formation of stars and planetary systems, including those found in our solar system. with the composition of interstellar neutrals (ISNs) and pickup ions (PUIs) measured by IMAP-Lo, CoDICE, and SWAPI.
Understanding the number of particles of space dust in a certain area of the sky, along with their composition, informs scientists how much of each type of elemental material is out there in various regions of our The totality of all space and time; all that is, has been, and will be..
Meet the Team
IDEX was built and tested at the Laboratory for Atmospheric and Space Physics (LASP) at University of Colorado, Boulder under instrument lead Mihaly Horanyi.
Playing a role in the incredibly successful IDEX dust testing campaigns has been a highlight in my career. Testing like we fly required pushing the accelerator to its extremes for hypervelocity interstellar-like dust grains. The An astronomical measurement of an object's brightness; larger magnitudes represent fainter objects. of IDEX and the team's precision was seen in all aspects, including using almost every inch of test chambers for this large instrument. Go IDEX, go IMAP!
- John Fontanese, Former IMPACT Dust Accelerator Operator, IDEX

The IDEX team together at UC Boulder-LASP after their Pre-Environmental Review (PER).
Image Credit: NASA/UCBoulder-LASP