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Home Astronomy

Bending Spacetime Reveals New Planet Hidden in Archived TESS Knowledge

July 4, 2026
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Bending Spacetime Reveals New Planet Hidden in Archived TESS Knowledge
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NASA’s Transiting Exoplanet Survey Satellite tv for pc (TESS) has captured proof of a Jupiter-like world orbiting one other star, utilizing a trick straight out of Einstein’s relativity: gravitational microlensing. The method marks a primary for TESS, and opens up the potential of a complete new class of planets the spacecraft would possibly uncover.

“When TESS launched, nobody anticipated it to ever be able to find this sort of planet,” mentioned Diana Dragomir, professor on the College of New Mexico, in a NASA press release. “The invention implies that there are most likely different so-called microlensing planets hiding in TESS’s knowledge that we hadn’t beforehand thought to search for.”

The paper asserting the invention was printed July 1, 2026 within the *Astrophysical Journal Letters*.

TESS is a planet-hunting virtuoso, having found greater than 800 new planets to this point. However normally, TESS finds planets orbiting very close to to their star. That’s as a result of it was designed to make use of the transit technique of detection, the place a planet passes shut in entrance of its star, dimming the sunshine in a manner that makes its presence recognized to astronomers.

This new super-Jupiter, dubbed Gaia23bra b, is an outlier amidst TESS’s discoveries. It orbits its star a lot additional out, at across the identical distance as Jupiter orbits the Solar. What’s extra, the star system itself is 40,000 light-years away from Earth, far past TESS’s normal detection vary of about 150 light-years.

The microlensing impact that made the detection potential is a results of gravitational lensing: the bending of spacetime round large objects, as predicted by the idea of basic relativity. On this case, Gaia23bra b and its star handed in entrance of an much more distant star, and as they moved, they warped the sunshine from that distant star, inflicting a magnifying-glass-like impact that enhanced the brightness of the distant star.

This animation illustrates the concept of gravitational microlensing. When one star in the sky (shown in the center of the animation) appears to pass nearly in front of another (located in the dashed circle at the right) from our vantage point, the light rays of the background star become bent due to the warped space-time around the foreground star. This star acts like a virtual magnifying glass, amplifying the brightness of the background star and causing its position to appear to slightly shift. If the nearer star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source. When astronomers find planets this way, they can measure their mass and orbital distance from their host star. NASA’s Goddard Space Flight Center/CI Lab *This animation illustrates the idea of gravitational microlensing. When one star within the sky (proven within the heart of the animation) seems to go almost in entrance of one other (situated within the dashed circle on the proper) from our vantage level, the sunshine rays of the background star grow to be bent because of the warped space-time across the foreground star. This star acts like a digital magnifying glass, amplifying the brightness of the background star and inflicting its place to seem to barely shift. If the nearer star harbors a planetary system, then these planets also can act as lenses, each producing a brief deviation within the brightness of the supply. When astronomers discover planets this manner, they will measure their mass and orbital distance from their host star. NASA’s Goddard Area Flight Heart/CI Lab*

Lensing occasions occur on a regular basis as stars cross one another’s paths, however what caught the astronomers’ eye on this explicit occasion is that the sunshine from the distant star was magnified twice: as soon as from the transferring star, and a second time from Gaia23bra b. This double lens impact revealed the hidden planet.

Lower than 5% of all recognized exoplanets had been found this manner, and the one-off nature of lensing occasions means we’re unlikely to get one other glimpse at Gaia23bra b anytime quickly.

“Microlensing occasions occur as soon as they usually’re gone — they don’t repeat. I prefer to joke that we’ll most likely discover the primary Earth analog with microlensing, after which wave at it because it goes by as a result of we’ll by no means see it once more,” mentioned Mallory Harris, PhD candidate on the College of New Mexico and lead writer of the research.

However they’re however worthwhile alternatives for exoplanet hunters.

“With microlensing, we are able to discover smaller planets with higher orbital distances, together with worlds within the liveable zone of their star and even farther away,” Harris mentioned.

By combining the transit technique with gravitational microlensing, a bigger number of planet varieties is open to discovery.

The invention additionally highlights the significance of sustaining a number of complementary telescope varieties to optimize planet-hunting methods. TESS’s discovery wouldn’t have been potential if the lensing impact had not first been captured by ESA’s Gaia spacecraft, which lately accomplished its science observations mapping the Milky Means in three dimensions.

Gaia’s large discipline of view over very long time intervals advised astronomers the place to look, in order that extra exact devices like TESS might then see in additional element what Gaia couldn’t by itself: a hidden planet. Solely by combining the strengths of each devices was this discovery made potential.



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