4 min read

Be Glad You Don’t Have to Dust in Space!

Come springtime you might be ready to throw open the windows and break out the feather duster, because that’s a great time to do a little cleaning! Fortunately, no one has to tidy up the dust in space — because there’s a lot of it — around 100 tons rain down on Earth alone every day! And there’s even more swirling around the solar system, our Milky Way galaxy, other galaxies, and the spaces in between.

Small specs of white and tan drift by, and a large, irregular shape floats into the image from the left, traveling to the right and down until it disappears off the bottom of the frame.
Specs of space dust float by in this illustration. Space dust is made of rock, ice, minerals, or organic compounds.

By studying the contents of the dust in your house — which can include skin cells, pet fur, furniture fibers, pollen, concrete particles, and more — scientists learn a lot about your environment. In the same way, scientists can learn a lot by looking at space dust. Also called cosmic dust, a fleck of space dust is usually smaller than a grain of sand and is made of rock, ice, minerals, or organic compounds. Scientists can study cosmic dust to learn about how it formed and how the universe recycles material.

Looking like an apparition rising from whitecaps of interstellar foam, the iconic Horsehead Nebula is shown in infrared light as imaged by the Hubble Space Telescope. The heart of the nebula appears in red like a capital letter T with wilted edges. Wrapped around this heart are white, gray, and transparent-looking clouds of material. All on a start-studded background.
The Horsehead Nebula is a dark cloud of dense gas and dust located just below the belt of Orion on the sky.
NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

“We are made of star-stuff,” Carl Sagan famously said. And it’s true! When a star dies, it sheds clouds of gas in strong stellar winds or in an explosion called a supernova. As the gas cools, minerals condense. Observations by our SOFIA mission suggest that in the wake of a supernova shockwave, dust may form more rapidly than scientists previously thought. These clouds of gas and dust created by the deaths of stars can sprawl across light-years and form new stars — like the Horsehead Nebula pictured above. Disks of dust and gas form around new stars and produce planets, moons, asteroids, and comets. Here on Earth, some of that space dust eventually became included in living organisms — like us! Billions of years from now, our Sun will die too. The gas and dust it sheds will be recycled into new stars and planets and so on and so forth, in perpetuity!

A molten-red ring of light surrounds the bright center of the M31 galaxy. Swirls of smaller yellow and red tendrils encircle the bright central spot, which is just slightly off-center.
NASA's Spitzer Space Telescope captured this stunning infrared view of the famous galaxy Messier 31, also known as Andromeda in 2004. It was the sharpest image ever taken of the dust in a spiral galaxy, other than our Milky Way.
NASA/JPL-Caltech/Univ. of Ariz.

Astronomers originally thought dust was a nuisance that got in the way of seeing the objects it surrounded. Dust scatters and absorbs light from stars and emits heat as infrared light. Once we started using infrared telescopes, we began to understand just how important dust is in the universe and how beautiful it can be. The picture of the Andromeda galaxy above was taken in the infrared by our Spitzer Space Telescope and reveals detailed spirals of dust that we can’t see in an optical image.

A double line of light gray breaks up a starfield dotted with points of light, running from left to right about a third of the way down this image. The image is looking through Jupiter’s main ring. The star field’s background is darker at the top and bottom of the image, with a gradient of gray from lighter to darker running below the double line.
As NASA's Juno spacecraft flew through the narrow gap between Jupiter's radiation belts and the planet and collected the first image of Jupiter's ring taken from the inside looking out. The bright bands in the center of the image are the main ring of Jupiter's ring system.

We also see plenty of dust right here in our solar system. Saturn’s rings are made of mostly ice particles and some dust, but scientists think that dust from meteorites may be darkening the rings over time. Jupiter also has faint dusty rings, although they’re hard to see — Voyager 1 only discovered them when it saw them backlit by the Sun. Astronomers think the rings formed when meteorite impacts on Jupiter’s moons released dust into orbit. The Juno spacecraft took the above picture in 2016 from inside the rings, looking out at the bright star Betelgeuse.

The bright light at the end of this country road is a close conjunction of two Venus and Jupiter from August 27, 2016. This vertical panorama shows the central Milky Way near zenith, posed on top of a pillar of zodiacal light along the ecliptic plane.
Copyright Josh Calcino, used with permission

And some space dust you can see from right here on Earth! In spring or autumn, right before sunrise or after sunset, you may be able to catch a glimpse of a hazy cone of light above the horizon created when the Sun’s rays are scattered by dust in the inner solar system. You can see an example in the image above, extending from above the tree on the horizon toward a spectacular view of the Milky Way. This phenomenon is called zodiacal light — and the dust that’s reflecting the sunlight probably comes from icy comets. Those comets were created by the same dusty disk that that formed our planets and eventually you and the dust under your couch!