NASA's TESS Spots Record-breaking Stellar Triplets

  • Released Wednesday, October 2, 2024

This artist’s concept illustrates how tightly the three stars in the system called TIC 290061484 orbit each other. If they were placed at the center of our solar system, all the stars’ orbits would be contained a space smaller than Mercury’s orbit around the Sun. The sizes of the triplet stars and the Sun are also to scale.Credit: NASA’s Goddard Space Flight Center

This artist’s concept illustrates how tightly the three stars in the system called TIC 290061484 orbit each other. If they were placed at the center of our solar system, all the stars’ orbits would be contained a space smaller than Mercury’s orbit around the Sun. The sizes of the triplet stars and the Sun are also to scale.

Credit: NASA’s Goddard Space Flight Center

Professional and amateur astronomers teamed up with artificial intelligence to find an unmatched stellar trio called TIC 290061484, thanks to cosmic “strobe lights” captured by NASA’s TESS (Transiting Exoplanet Survey Satellite).

The system contains a set of twin stars orbiting each other every 1.8 days, and a third star that circles the pair in just 25 days. The discovery smashes the record for shortest outer orbital period for this type of system, set in 1956, which had a third star orbiting an inner pair in 33 days.

Flickers in starlight helped reveal the tight trio, which is located in the constellation Cygnus. The system happens to be almost flat from our perspective. This means the stars each cross right in front of, or eclipse, each other as they orbit. When that happens, the nearer star blocks some of the farther star’s light.

Using machine learning, scientists filtered through enormous sets of starlight data from TESS to identify patterns of dimming that reveal eclipses. Then, a small team of citizen scientists filtered further, relying on years of experience and informal training to find particularly interesting cases.

Partly because the stars in the newfound system orbit in nearly the same plane, scientists say it’s likely very stable despite their tight configuration (the trio’s orbits fit within a smaller area than Mercury’s orbit around the Sun). Each star’s gravity doesn’t perturb the others too much, like they could if their orbits were tilted in different directions.

As the inner stars age, they will expand and ultimately merge, triggering a supernova explosion in around 20 to 40 million years.

Watch how the three stars in the system called TIC 290061484 eclipse each other over about 75 days. The line at the bottom is the plot of the system's brightness over time, as seen by TESS (Transiting Exoplanet Survey Satellite). The inset shows the system from above.

Credit: NASA's Goddard Space Flight Center

Watch this video on the NASA Video YouTube channel.

This graphic highlights the search areas of three transit-spotting missions: NASA’s upcoming Nancy Grace Roman Space Telescope, TESS (Transiting Exoplanet Survey Satellite), and the retired Kepler Space Telescope. Kepler found 13 triply eclipsing triple star systems, TESS has found more than 100 so far, and astronomers expect Roman to find more than 1,000.Credit: NASA’s Goddard Space Flight Center

This graphic highlights the search areas of three transit-spotting missions: NASA’s upcoming Nancy Grace Roman Space Telescope, TESS (Transiting Exoplanet Survey Satellite), and the retired Kepler Space Telescope. Kepler found 13 triply eclipsing triple star systems, TESS has found more than 100 so far, and astronomers expect Roman to find more than 1,000.

Credit: NASA’s Goddard Space Flight Center

Complete sequence of original lightcurve frames and video.

Credit: NASA’s Goddard Space Flight Center

Complete sequence showing a side view of the orbits of the three stars. Available as frames and video.

Credit: NASA’s Goddard Space Flight Center

Complete sequence showing a top view of the orbits of the three stars. Available as frames and video.

Credit: NASA’s Goddard Space Flight Center



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NASA's Goddard Space Flight Center.

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This page was originally published on Wednesday, October 2, 2024.
This page was last updated on Tuesday, September 24, 2024 at 3:01 PM EDT.


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