Michael Fausnaugh , assistant professor in the Department of Physics & Astronomy at Texas Tech University , is part of a group of researchers who have identified a planet orbiting a distant star, according to a news release from NASA.
Fausnaugh and astronomers from the University of New Mexico are authors of a paper explaining the findings, which were made possible through the use of NASA's TESS (Transiting Exoplanet Survey Satellite). The planet, called Gaia23bra b, was initially discovered in 2023 using the European Space Agency's now-retired Gaia space telescope and is described as a super Jupiter orbiting far from its host star.
"We had a background star with a foreground star in front of it magnifying its light," Fausnaugh said. "If there's a planet orbiting the foreground star, you can see the signature of the planet through gravitational microlensing. The technique is well-established, but we had never done it with TESS, and the unique thing about TESS is it takes images every couple of minutes."
After Gaia had initially flagged a star brightening, researchers went back through the archived TESS data and found the event had been captured there as well.
The team's analysis is scheduled to be published in The Astrophysical Journal Letters . According to the findings, the planet orbits an orange dwarf star that's about 80 percent of the sun's mass and is nearly 40,000 light-years away from Earth.
"In order to find planets, we have very limited ways of detecting them, and most of the planets we've found so far have been what you might consider the easy planets to find," Fausnaugh said. "The problem is those planets are close to the stars, and they go around the stars very quickly.
"Then there's others that are Jupiter size, but they're so close to the star that they are also very hot. They don't match what we have in our solar system."
Out of more than 6,000 known exoplanets, worlds outside our solar system, about 75% were discovered through the transit method, the typical technique employed by TESS. Astronomers monitor numerous stars looking for those that periodically dim as orbiting planets cross in front of them. This is known as a transit.
Meanwhile, microlensing has revealed less than 5% of known exoplanets. This occurs when two stars align closely with light from the more distant star curving as it travels through the warped space time caused by the nearer star's miss. If the alignment is especially close, the nearer star acts like a lens, focusing and magnifying light from the background star.
The transit method is best at finding large planets orbiting very close to their host stars; large planets block the most starlight, while close-in planets are more likely to pass in front of the host star. These extremely hot worlds are fascinating to scientists, but astronomers want to find planets like those in our solar system, too. Gravitational microlensing is best at detecting planets like Jupiter and Saturn, which are massive and orbit further from their host stars."
"Astronomy really sparks the imagination," Fausnaugh said. "There's always this gap between the data and the interpretation. It can be a complicated and technical process, but here, our best physical description of this star system says, 'There's a planet up there.'"
