Home / Research / SPARCS: Star-Planet Activity Research CubeSat

SPARCS: Star-Planet Activity Research CubeSat

The Star-Planet Activity Research CubeSat (SPARCS) is a small space telescope about the size and shape of a family-size Cheerios box.

It is built of six cubical units, each about four inches on a side. These are joined to make a spacecraft two units wide by three long in what is termed a 6U spacecraft; solar power panels extend like wings from one end.

The mission which SPARCS will undertake is monitoring the flares and sunspot activity of M-type stars, also called red dwarfs, in the far- and near-ultraviolet. The purpose of this is to assess how habitable the space environment is for planets orbiting them.

The principal investigator for SPARCS is astrophysics professor Evgenya Shkolnik of the School of Earth and Space Exploration. Other professors from the School on the SPARCS project are Judd Bowman (Mission Operations System Lead), Daniel Jacobs (Systems Engineer), and Paul Scowen (Payload Systems Engineer).

The stars that SPARCS will focus on are small, dim, and cool by comparison to the Sun. They have less than half the Sun's size and temperature, and they shine with barely one percent its brightness.

While this might seem to make them a poor choice for hunting extrasolar planets, these stars are extremely numerous in our Milky Way galaxy. Roughly 75 billion M dwarf stars host at least one small planet in their habitable zones. This is the potentially life-friendly region close to the star where temperatures are neither too hot nor too cold for life as we know it, and liquid water could exist on a planet's surface.

However, ultraviolet radiation from M dwarf stars is strong and highly variable. This would erode a planet's atmosphere and would affect its composition and habitability.   

Knowing the ultraviolet environments of planets orbiting M dwarf stars will be crucial to understanding the planets' atmospheric composition. It will also be key factor in discriminating between biological and abiotic sources for any observed biosignatures.

The stellar modeling is being led by Travis Barman of the Lunar and Planetary Lab at the University of Arizona and the planet modeling by Victoria Meadows of the Virtual Planet Laboratory at the University of Washington.

SPARCS Science and Technology

(Click the image for the full-resolution graphic in PDF format; 18 MB)

The spacecraft will contain three major systems — the telescope, the camera, and the operational and science software. ASU astronomers will oversee the development of the telescope and camera, plus the software and the systems engineering.
 
The telescope uses a mirror system with coatings optimized for ultraviolet light. Together with the camera, the system can measure very small changes in the brightness of M dwarf stars to carry out the primary science of the mission. The instrument will be tested and calibrated at ASU in preparation for flight before being integrated into the rest of the spacecraft.
 
For each targeted star, SPARCS will observe continuously over at least one complete stellar rotation (5 to 45 days).

SPARCS will also advance ultraviolet detector technology by flying high quantum efficiency, UV-optimized detectors developed at NASA's Jet Propulsion Laboratory, led by Shouleh Nikzad. These Delta-doped detectors have a long history of deployment demonstrating greater than five times the quantum efficiency of the detectors used by the Galaxy Evolution Explorer (GALEX) mission.

SPARCS will pave the way for their application in missions like the Large UV/Optical/IR Surveyor (LUVOIR) or the Habitable Exoplanet Observatory (HabEx) missions, including interim UV-capable missions. SPARCS will also be capable of "target-of-opportunity" ultraviolet observations for the rocky planets in M-dwarf habitable zones soon to be discovered by NASA’s Transiting Exoplanet Survey Satellite (TESS) mission. This will provide the needed ultraviolet context for the first habitable planets that the James Webb Space Telescope will characterize.

SPARCS Timeline

SPARCS is aiming to be ready for launch by the end of 2021 to a Sun-synchronous orbit.

SPARCS Team

David Ardila (JPL)
Payload Scientist

Travis Barman (UA)
Stellar Atmospheres Lead

Matthew Beasley (SwRI)
Payload Team

Judd Bowman (ASU)
Mission Operations System Lead

 

Mary Elliott (ASU)
Project Manager

Varoujan Gorjian (JPL)
Science Team

Daniel Jacobs (ASU)
System Engineer

April Jewell (JPL)
Camera Team

Mary Knapp (MIT)
CubeSat Development

Joe Llama (Lowell)
Science Team

Victoria Meadows (UW)
Planetary Atmospheres Lead

Shouleh Nikzad (JPL)
Camera Lead

 

Tahina Ramiaramanantsoa (ASU)
Postdoctoral Student

 Sarah Peacock (UA)
Graduate Student

 

Paul Scowen (ASU)
Payload Systems Engineer

 

Evgenya Shkolnik (ASU)
Principal Investigator

 

Connie Spittler (ASU)
Graduate Student

Mark Swain (JPL)
JPL Lead

Robert Zellem (JPL)
Science Team

Press

ASU Astronomers to Build Space Telescope to Explore Nearby Stars

Additional Resources

On the Verge of an Astronomy CubeSat Revolution (PDF)
Monitoring the High-Energy Radiation Environment of Exoplanets Around Low-Mass Stars with SPARCS (PDF)
Ultraviolet Detectors for Astrophysics Missions: A Case Study With the Star-Planet Activity Research CubeSat (PDF)
The Star-Planet Activity Research CubeSat (SPARCS): A Mission to Understand the Impact of Stars in Exoplanets