Published: Oct. 19, 2020 By
Artist's depiction of the SPRITE CubeSat orbiting Earth.

Artist's depiction of the SPRITE CubeSat orbiting Earth. (Credit: LASP)

Scientists at CU 麻豆影院 are developing a satellite about the size of a toaster oven to explore one of the cosmos鈥 most fundamental mysteries: How did radiation from stars punch its way out of the first galaxies to fundamentally alter the make-up of the universe as it we know it today.听

Those insights will come from the Supernova Remnants and Proxies for ReIonization Testbed Experiment (SPRITE), a NASA-funded mission led by the (LASP) at CU 麻豆影院.听

Scheduled to launch in 2022, the $4 million SPRITE is the latest in LASP鈥檚 line of little-spacecraft-that-could. This 鈥淐ubeSat鈥 will measure just over a foot in length and will weigh about 40 pounds. It will also collect unprecedented data from modern-day stars and supernovas to help scientists better understand a time in the history of the cosmos called the 鈥淓poch of Reionization鈥濃攁 period in which the universe鈥檚 first stars lived fast and hard, burning out and going supernova in a span of just a few million years.听

鈥淲e鈥檙e trying to establish what the universe was like when it first formed and how it evolved to where it is today,鈥 said Brian Fleming, a research professor at LASP who is leading the SPRITE mission.听

Artist's depiction of the universe's first stars.Hubble Space Telescope image of the blast wave expanding out from a supernova.

Top: An artist's depiction of what the universe's first stars surrounded by clouds of neutral hydrogen gas might have looked like; bottom: A Hubble Space Telescope image of a blast wave expanding out from a supernova. (Credits: NASA;听NASA, ESA听and G. Bacon, T. Borders, L. Frattare, Z. Levay, and F. Summers, STScI)

The team also hopes that SPRITE will show just how much CubeSats can achieve. To date, most of these miniature spacecraft have focused on studying phenomena that are closer to home鈥攕uch as weather on Earth or flares erupting from the surface of the sun.听

鈥淭here has been a perception that to do new astrophysics you need to collect a lot of light so you need something big,鈥 said Fleming, also of the Department of Astrophysical and Planetary Sciences. 鈥淪PRITE is trying to do something different. There鈥檚 a lot of science you can do by optimizing your design and using new technologies.鈥

Going clear

SPRITE, in other words, packs a lot of ambition into a small package.

Fleming explained that before the Epoch of Reionization, the universe wasn鈥檛 anything like it is today. The cosmos鈥 first stars and galaxies were just beginning to form, but their light couldn鈥檛 spread far into space like it does today鈥攖he vast distances between galaxies were filled with neutral gas that effectively fogged up the universe.听

Then, a little more than 13 billion years ago, that began to change: Radiation from these young stars started leaking out of their galaxies and ionizing the surrounding gas鈥攌icking electrons off of the hydrogen atoms and changing the nature of the matter that permeates the universe.

鈥淲e started seeing these bubbles of ionization appear,鈥 he said. 鈥淕radually, the bubbles got more and more numerous until they started merging.鈥

There鈥檚 just one problem with the theory: Scientists still aren鈥檛 sure how this light was able to escape from the universe鈥檚 first galaxies. One theory suggests that ancient supernovas blew the clouds of dense gas surrounding those early stars out of the way, a bit like giant leaf blowers in space.

鈥淪upernovas are very disruptive,鈥 Fleming said. 鈥淭hey may have been able to move the neutral gas out of the way so that the ionizing radiation was able to get out of these early galaxies.鈥

Getting creative

SPRITE won鈥檛 seek to observe those ancient eruptions directly. Instead, it will conduct two surveys closer to home. One will measure how nearby galaxies emit ionizing radiation. The second will look at the remains of exploded stars in the Magellanic Clouds, two dwarf galaxies that circle our own Milky Way.听

It won鈥檛 be easy. That kind of radiation can only be viewed in a narrow window of ultraviolet light鈥攐ne that has been historically difficult to spot with telescopes. To get around that limitation, the SPRITE team is experimenting with a range of new technologies that haven鈥檛 flown into space before. They include a special type of mirror coating designed to bounce that ultraviolet light into the CubeSat鈥檚 detectors.听

The SPRITE team is in the process of finalizing designs for the spacecraft and will begin to build prototype parts soon.

The mission will also be a learning opportunity for budding scientists and engineers at LASP. CubeSats, Fleming explained, offer students and young scientists and engineers a chance to work on a space mission from beginning to end鈥攏ot something that鈥檚 possible on many larger, more complicated projects.

That鈥檚 one reason why Dana Chafetz decided to work on SPRITE. She graduated from Northeastern University in Boston in December 2019 and joined Fleming鈥檚 lab as a mechanical engineer in April. Chafetz said that this CubeSat project has given her the chance to have more ownership听over the design process and the ability to try out ideas that no one has thought of before.

鈥淚f I want to do something new, as long as we can test it, we can do it,鈥 Chafetz said. 鈥淚t鈥檚 a really creative environment.鈥

The SPRITE team includes researchers from NASA Goddard Space Flight Center, the Jet Propulsion Laboratory, Johns Hopkins University, Williams College, Arizona State University, the WM Keck Observatory, Minnesota State Mankato and the Space Telescope Science Institute.