Possibly Habitable Trappist-1 Exoplanet Destroying Atmosphere - Space PDF

Summary

Scientists have discovered that the potentially habitable exoplanet Trappist-1e is losing its atmosphere due to electric currents generated by its rapid orbit around its red dwarf star. This process could eventually make the planet uninhabitable. The findings highlight potential challenges in finding life on other planets.

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2/28/24, 7:21 AM Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere | Space Subscribe TRENDING Private moon lander tipped over! Next Full Moon Best Telescopes Best Binoculars Best S When you purchase through links on our site, we may earn an affiliate commission. Here’s how...

2/28/24, 7:21 AM Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere | Space Subscribe TRENDING Private moon lander tipped over! Next Full Moon Best Telescopes Best Binoculars Best S When you purchase through links on our site, we may earn an affiliate commission. Here’s how it works. Exoplanets Advertisement Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere News By Robert Lea published about 1 hour ago "I would imagine that all Trappist-1 planets are going to have a hard time holding on to any atmosphere."    Comments (0) An illustration of Trappist-1e shows the potentially habitable exoplanet being stripped of its atmosphere by harsh radiation from its red dwarf star as its planetary siblings watch on (Image credit: Robert Lea) Scientists have discovered that a potentially habitable planet is having its atmosphere stripped, a process that may eventually render the world, Trappist-1e, inhospitable to life. The stripping appears to be caused by electric currents created as the planet races around its red dwarf host star. https://www.space.com/trappist-1-exoplanet-habitability-atmospheric-stripping 1/11 2/28/24, 7:21 AM Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere | Space It's a significant discovery because the Trappist-1 system, in which this exoplanet orbits a small red dwarf star, has been one of the primary targets in the hunt for alien life. Of the seven rocky Earth-like worlds in the system, at least 3 are located in the habitable zone, a region around a star that is neither too hot nor too cold to allow a planet to support liquid water. A planet without an atmosphere can't hold on to liquid water, however, even if it is in the habitable zone, also known as the "Goldilocks zone." This shows that, though Trappist-1e may be in the habitable zone of the red dwarf Trappist-1, located 40 light-years from Earth, its habitability may be fleeting. Advertisement -25% -45% Sponsored Links Unveiling the 15 most beautiful women on the planet LPNAF The same phenomenon affecting Trappist-1e's atmosphere could be impacting the atmospheres of the other planets in this habitable zone as well, which is bad news for the possibility of finding life in this system. Related: This TRAPPIST-1 exoplanet seems to have no atmosphere — the truth may hide in its star, James Webb Space Telescope reveals Click here for more Space.com videos... Webb Telescope will study Trappist-1's potenti… The James Webb Space Telescope will look for biosignatures and mor… Get What You Love at Etsy More Videos Etsy Close MORE FROM SPACE... PLAY SOUND 1 Trappist-1e is roughly Earth-sized, yet has around 0.7 times the mass of our planet. It is the fourth planet from its star, orbiting at just 0.028 times the distance between Earth and the sun, completing one orbit in just 6.1 Earth days. NASA radar images show stadium-sized asteroid tumbling by Earth during flyby (photos) 2 Despite this proximity, because Trappist-1 is much smaller and cooler than the sun, its habitable zone is much closer to its surface when compared to our star's habitable zone. To that end, it isn't radiation from this red dwarf that seems to be stripping the TRAPPIST-1e's atmosphere, but rather a wind of charged particles blown from the star called the "stellar wind." Apollo astronaut's granddaughter opens immersive 'Lunar Light' moonwalk experience in Dallas 3 Put on your eclipse glasses and look up to see the biggest sunspot in years before it disappears from view 00:42 / 02:39 Ways to strip an exoplanet's atmosphere https://www.space.com/trappist-1-exoplanet-habitability-atmospheric-stripping 2/11 2/28/24, 7:21 AM Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere | Space "We looked at how the space weather changes through the planet's orbit, with TRAPPIST-1e transitions very rapidly between very different stellar wind conditions and pressures, leading to a sort of pulsing compression and relaxation of the planetary magnetic field," Cecilia Garraffo, team member and an astrophysicist at Harvard & Smithsonian, told Space.com. "This drives strong electric currents in the upper atmosphere — the ionosphere — that heat up the atmosphere just like an electric heater." 4 NASA's Dana Weigel will be the 1st female ISS program manager 5 Intuitive Machines' Odysseus probe beams home more photos from historic moon landing Advertisement An illustration showing the size difference between Trappist-1 and the sun. (Image credit: Robert Lea/NASA) Garraffo explained that Earth also experiences variations in the solar wind, which causes a similar heating of our atmosphere. The difference is that the heating felt by TRAPPIST-1e is up to 100,000 times stronger than what Earth experiences with the sun's solar winds. That's because Trappist-1e moves quickly around its star, and the motion drives powerful ionospheric currents that dissipate and create extreme heating, which the team calls "voltage-driven Joule heating." Even though the team had predicted this effect back in 2017, the researchers were surprised by just how powerful they have now found it to be. "It could be so strong for TRAPPIST-1e that the heat essentially evaporates the upper atmosphere," Garraffo said. "Over millions of years, the planet could lose its atmosphere entirely to this phenomenon." The team's research shows there are more than a couple of ways for a Advertisement planet to lose its atmosphere. Team member and Lowell Center for Space Science & Technology researcher Ofer Cohen told Space.com that, typically, the loss of exoplanet atmospheres is believed to be driven by some external process. This includes strong radiation from the star, which can cause the atmosphere to heat up and escape, or charged particles in the stellar wind pelting planets, causing a strong stripping effect. "In this case, the heating of the atmosphere, and its loss as a result, are driven only by the rapid planetary motion. So, the planet dooms itself to lose its atmosphere by simply moving around," Cohen said. "It's like the case when we are too lazy to clean the roof of our car from snow, and we just start driving, hoping that the air moving around the car would do the https://www.space.com/trappist-1-exoplanet-habitability-atmospheric-stripping 3/11 2/28/24, 7:21 AM Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere | Space work for us and take the snow off — at least that's what we do in the Boston area. "I think that it is very cool that planets can do this with their atmosphere." What about the other Trappist-1 planets? On Earth, our magnetosphere protects our atmosphere by diverting charged particles down magnetic field lines and out behind our planet. Mars, lacking a strong magnetic field, has had its atmosphere stripped by solar winds and harsh solar radiation. In fact, the Red Planet probably lost its water to space as a result. Trappist-1e is also believed to have a magnetosphere, but these findings show it might not be sufficient to prevent atmospheric stripping. "Normally, a planet's magnetic field acts as a protective bubble, but around TRAPPIST-1e, this bubble is compromised. The planet's magnetic field connects with the star's, creating pathways that allow the star's particles to hit the planet directly," Garraffo said. "This not only strips away the atmosphere but also heats it up significantly, leaving TRAPPIST-1e and its neighbors vulnerable to losing their atmospheres entirely." #1 Rated Custom Luxury… Casoro Jewelry Safes The entire Trappist-1 system would fit within the orbit of the solar system's innermost planet Mercury. (Image credit: NASA/JPL-Caltech) Trappist-1e is the fourth planet from the red dwarf star at the heart of this fascinating planetary system of rocky worlds. Astronomers have previously discovered that Trappist-1b, the closest exoplanet to the star, seems to have already lost its atmosphere. The team thinks voltage-driven Joule heating could also be impacting Trappist-1f and Trappist-1g, stripping them of their atmospheres as well, albeit to a lesser extent than they see happening with Trappist-1e. That's because, at 0.038 and 0.04683 times the distance between Earth and the sun from their star respectively, these planets are moving slower through the red dwarf's stellar winds than Trappist-1e is. "Closer-in planets of Trappist-1 will have an even more extreme fate, and further out ones a bit milder," Garraffo said. "I would imagine that all Trappist-1 planets are going to have a hard time holding on to any atmosphere." https://www.space.com/trappist-1-exoplanet-habitability-atmospheric-stripping 4/11 2/28/24, 7:21 AM Possibly habitable Trappist-1 exoplanet caught destroying its own atmosphere | Space RELATED STORIES:  — Exoplanets in the Trappist-1 system more likely to be habitable than scientists once thought, study suggests — The TRAPPIST-1 solar system not bombarded by space rocks like early Earth, study suggests — James Webb Space Telescope could help hunt for habitable alien worlds The team's findings could have implications outside the Trappist-1 system as well as in the search for habitable exoplanets and life outside the solar system. They suggest exoplanets close to their stars have likely lost their atmospheres even if they are well within the habitable zone of that star. The results could further help suggest which stars could host planets with molecules that indicate the presence of life: Biomarkers. "Our research suggests such low-mass host stars are probably not the most promising for hosting planets with atmospheres," Garraffo concluded. "Identifying which host stars can be conducive to habitable planets and observing those atmospheric transits with James Webb Space Telescope and future observatories, but also building the technology to interpret those results in terms of biomarkers." The team's research was published on Feb. 16 in the Astrophysical Journal. Join our Space Forums to keep talking space on the latest missions, night sky and more! And if you have a news tip, correction or comment, let us know at: [email protected]. Get the Space.com Newsletter Breaking space news, the latest updates on rocket launches, skywatching events and more! Your Email Address SIGN ME UP Contact me with news and offers from other Future brands Receive email from us on behalf of our trusted partners or sponsors By submitting your information you agree to the Terms & Conditions and Privacy Policy and are aged 16 or over. Robert Lea Contributing Writer Robert Lea is a science journalist in the U.K. whose articles have been published in Physics World, New Scientist, Astronomy Magazine, All https://www.space.com/trappist-1-exoplanet-habitability-atmospheric-stripping 5/11

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