For the first time, NASA\u2019s TESS (Transiting Exoplanet Survey Satellite) mission has identified a planet orbiting a distant star thanks to ripples in space-time. Unlike the star-hugging transiting planets TESS regularly reveals, the newfound world is a super-Jupiter orbiting far from its host star.<\/p>\n
\u201cWhen TESS launched, no one expected it to ever be capable of finding this kind of planet,\u201d said Diana Dragomir, a professor at the University of New Mexico in Albuquerque and co-author of a paper describing the results. At 1.6 times Jupiter\u2019s mass and a similar orbital distance, it would be extremely unlikely to find such a planet via the primary detection method TESS was designed for. \u201cThe discovery implies that there are probably other so-called microlensing planets hiding in TESS\u2019s data that we hadn\u2019t previously thought to look for.\u201d<\/p>\n
Astronomers found the first hint of the planet, called Gaia23bra b, in 2023 using ESA’s (European Space Agency) now-retired Gaia space telescope. Gaia\u2019s alert system flagged a star that brightened \u2014 something that can happen when a foreground star passes in front of a more distant one and magnifies its light through gravitational microlensing.<\/p>\n
Researchers later looked back through archived TESS data and found TESS had caught it too.<\/p>\n
\u201cGaia\u2019s observations were too sparse to pick up on the planet,\u201d said Mallory Harris, a Ph.D. candidate at the University of New Mexico, who led the study. \u201cThe TESS spacecraft happened to be monitoring the same area of the sky during the event, and its denser time coverage showed extra features in the light curve caused by a planet.\u201d<\/p>\n
The team\u2019s analysis, published July 1 in The Astrophysical Journal Letters<\/a>, revealed that Gaia23bra b, which orbits an orange dwarf star that\u2019s about 80 percent of the Sun\u2019s mass, is nearly 40,000 light-years away from Earth, far exceeding TESS\u2019s usual search radius of about 150 light-years.<\/p>\n Out of more than 6,000 known exoplanets<\/a> (worlds outside our solar system), about three-fourths were discovered via the transit method, TESS\u2019s typical planet-hunting technique. Astronomers monitor hordes of stars, watching for ones that periodically dim as orbiting planets cross in front of them \u2014 an event called a transit.<\/p>\n Microlensing has revealed less than 5% of known exoplanets. This light-bending phenomenon occurs when two stars align closely from our vantage point. Light from the more distant star curves as it travels through the warped space-time caused by the nearer star\u2019s mass.<\/p>\n If the alignment is especially close, the nearer star acts like a cosmic lens, focusing and magnifying light from the background star. Planets orbiting the foreground star may also modify the distant star\u2019s light, acting as their own tiny lenses. Astronomers see the effect as a spike in the star\u2019s brightness.<\/p>\n 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 gargantuan, steamy worlds are fascinating to scientists, but astronomers want to find planets like those in our solar system, too. That\u2019s microlensing\u2019s specialty.<\/p>\n Mallory harris<\/p>\n Ph.D. candidate at the University of New Mexico<\/p>\n<\/p><\/div><\/div><\/div><\/div><\/div>\n<\/div>\n Microlensing isn\u2019t well suited to finding huge, close-in planets because their gravitational signals would just blur together.<\/p>\n \u201cTransits and microlensing are complementary because they each reveal a category of planet the other may not be able to detect,\u201d Dragomir said. \u201cAnd they offer different details. Transits give us the size of a planet, and in concert with other methods we can determine its mass and density. Microlensing gives us masses and orbital distances for planets we\u2019d otherwise never see.\u201d<\/p>\n But microlensing observations are time-limited opportunities.<\/p>\n Mallory Harris<\/p>\n Ph.D. candidate at the University of New Mexico<\/p>\n<\/p><\/div><\/div><\/div><\/div><\/div>\n<\/div>\n That makes detailed observations of microlensing planets tough. However, the method can serve as a powerful demographics tool that offers broad information about planetary populations.<\/p>\n \u201cThis is a bit like a preview of the microlensing NASA\u2019s Nancy Grace Roman Space Telescope<\/a> will do,\u201d said Michael Fausnaugh, a professor at Texas Tech University in Lubbock and a co-author of the study. On track for launch on August 30, 2026, Roman will observe the center of the Milky Way galaxy for one of its core surveys<\/a>, revealing an estimated 1,000 microlensing planets<\/a> and around 100,000 transiting planets<\/a>.<\/p>\n Roman will specifically target the heart of the galaxy because stars are packed so tightly together there, increasing the odds of seeing microlensing events. While that crowding would make many stars blend together in TESS\u2019s larger pixels,\u00a0TESS\u00a0looks at nearly the whole sky, where stars are\u00a0\u200bmore spread out.<\/p>\n \u201cSince TESS looks elsewhere in the galactic plane, it can naturally find microlensing planets in other parts of the galaxy, as demonstrated by this first microlensing planetary system,\u201d Dragomir said. \u201cThat means it could help us study planets in regions with different conditions.\u201d<\/p>\n That could have implications for the search for habitable worlds. The bustling galaxy center is rife with radiation from more frequent supernova explosions, which could sterilize planets. And gravitational encounters between crowded stars may disrupt planetary systems. Observations from TESS focus on a milder part of the galaxy.<\/p>\n \u201cThe key to Roman\u2019s microlensing survey is its dense time coverage targeting the galactic bulge,\u201d Fausnaugh said. \u201cThe TESS mission uniquely provides these rapid observations for stars in other parts of the galaxy, and pairing the two opens up prospects for understanding planet formation in a diverse population of stars. Since microlensing finds solar system-like planets, this offers a new chance to understand how planetary systems like our own vary in different regions of the galaxy.\u201d<\/p>\n To learn more about the TESS mission, visit:<\/p>\n https:\/\/www.nasa.gov\/tess<\/strong><\/a><\/p>\n Media contact:<\/strong><\/p>\n Claire Andreoli<\/a>Microlensing 101<\/strong><\/h4>\n
![\"Mallory](\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/rst\/team\/unm.png?w=271&h=271&fit=clip&crop=faces%2Cfocalpoint\")
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NASA\u2019s Goddard Space Flight Center<\/a>, Greenbelt, Md.
301-286-1940<\/strong><\/strong><\/p>\n<\/div>\n