Tiny satellites called CubeSats have attracted a lot of attention in recent years.
Besides allowing researchers to test new technologies, their relative simplicity also offers hands-on training to early-career engineers.
A CubeSat recently deployed from the International Space Station is a key example of their potential, experimenting with CubeSats applied to astronomy.
For the next few months, a technology demonstration called ASTERIA (Arcsecond Space Telescope Enabling Research in Astrophysics) will test whether a CubeSat can perform precise measurements of change in a star’s light. This fluctuation is useful for a number of commercial and astrophysics applications, including the discovery and study of planets outside of our solar system, known as exoplanets.
ASTERIA was developed under the Phaeton Program at NASA’s Jet Propulsion Laboratory in Pasadena, California. Phaeton was developed to provide recent college graduates, under the guidance of experienced mentors, with the challenges of a flight project. ASTERIA is a collaboration with the Massachusetts Institute of Technology in Cambridge; MIT’s Sara Seager is principal investigator on the project.
A New Space Telescope Model
ASTERIA relies on precision photometry, a field that measures the flux, or intensity, of an object’s light. To be useful to any scientist, a space telescope has to correct for internal sources of error while making these measurements.
Engineers have learned to correct for “noise” in much larger space telescopes. If they were able to do the same for CubeSats, it could open an entirely new class of astronomy tools.
“CubeSats offer a relatively inexpensive means to test new technologies,” said Amanda Donner of JPL, mission assurance manager for ASTERIA. “The modular design of CubeSats also makes them customizable, giving even a small group of researchers and students access to space.”
She said it’s even possible for…