The Cosmic Dust in Your Bones – NASA’s Webb Telescope Will Investigate the Intertwined Origins of Dust and Life
Evidence indicates that large amounts of cosmic dust are produced as the stellar winds of massive stars collide in Wolf-Rayet binary or multiple-star systems. As the stars orbit each other and dust is produced, a distinctive pinwheel pattern is formed, as shown in this image from the European Southern Observatory. Warm dust like this glows in the mid-infrared wavelengths of light detectable by NASA’s James Webb Space Telescope. Confirming the origin of dust will help account for the mysterious over-abundance of it found in galaxies, which is crucial to the later development of stars, planets, and life as we know it.
Credit: ESO/Callingham et al.
Dust may seem insignificant, but it plays a huge role in the universe, from the formation of stars and planets to facilitating the complex chemistry that becomes the stuff of life—including us. Big questions like “How did we get here?” come down to dust, and yet the origin and formation process of cosmic dust has eluded scientists. Astronomers refer to the unexplained abundance of dust in galaxies as the “dust budget crisis.” It is a mystery that astronomers are excited to get to work solving using the specialized technology ofNASA’s James Webb Space Telescope.
Discovering too much money in your bank account may not be what you would call a “crisis,” but it would still be unexpected and you should figure out how it got there. Astronomers find themselves in a similar position when calculating the amount of dust galaxies should have; there is more dust than expected, and they don’t know where it’s coming from. This matters because cosmic dust is essential to the function of the universe: it shelters forming stars, becomes part of planets, and can contain the organic compounds that lead to life as we know it. Dust led to us.
“What we refer to as the ‘dust budget crisis’ is the major problem in astronomy of not being able to account for all the dust that’s observed in galaxies, both in the nearby and distant, early universe,” says Ryan Lau of the Japan Aerospace Exploration Agency. Lau is leading an Director’s Discretionary-Early Release Science Program with NASA’s upcoming James Webb Space Telescope to study dust-producing Wolf-Rayet binary stars.
Wolf-Rayet stars are very hot and very bright. There is evidence that Wolf-Rayet stars, through interactions with a companion star, produce large amounts of dust in a distinctive pinwheel pattern as the two stars orbit each other and their stellar winds collide. It is possible that these binary-star systems account for a large percentage of a galaxy’s “dust budget.” However, the intense luminosity and heat coming from the Wolf-Rayet stars has made it difficult to study the faint, more diffuse dust of these systems. This is where Webb comes in.
This animation shows the production of dust in the binary star system WR 140 as the orbit of the Wolf-Rayet star approaches the O-type star and their stellar winds collide. The stronger winds of the Wolf-Rayet star blow back behind the O star, and dust is created in its wake as the mixed stellar material cools. As the process repeats over and over, the dust will form a distinctive pinwheel shape.
Credit: NASA, ESA, and J. Olmsted (STScI)
“The mid-infrared light that Webb can detect is exactly the wavelength of light we want to look at to study the dust and its chemical composition,” Lau explains. Infrared wavelengths are longer than the wavelengths of visible light, and so can slide between dust grains to reach the telescope, rather than getting caught up bouncing around in the dust cloud. Webb will detect this light and allow astronomers to read the information it carries, including the signature of chemicals in the dusty environment, some of which may be the same chemicals that form the building blocks of life on Earth.
“Webb has an unprecedented combination of spatial resolution and sensitivity in mid-infrared wavelengths that is really what enables us to conduct these interesting observations,” Lau says. “We can achieve the spatial resolution from ground-based telescopes, but lack the sensitivity that Webb can achieve from its observing location in space, without the interference of Earth’s atmosphere. Conversely, with previous infrared space-based telescopes like NASA’s Spitzer mission, we could achieve the sensitivity but lacked the spatial resolution.”
Targeting Two Dust Factories
Lau and the Director’s Discretionary-Early Release Science (DD-ERS) team will use Webb to study two Wolf-Rayet binary systems, using the telescope’s Mid-Infrared Instrument (MIRI) and Near Infrared Imager and Slitless Spectrograph (NIRISS). The WR140 binary system has been studied extensively in many wavelengths of light and so will provide a good baseline for gauging Webb’s best observing modes for this kind of cosmic subject. Another Wolf-Rayet binary, WR137, will experience its stars’ closest approach to each other—when the most dust is thought to be produced—early in Webb’s mission when the DD-ERS program observations are scheduled.
Beyond new discoveries about the formation and chemical composition of dust, the DD-ERS program also will be among the first opportunities astronomers have to test out best practices for Webb’s instruments and processing the data it delivers.