Latest news with #MAROON-X
Economic Times
07-07-2025
- Science
- Economic Times
Scientists find second Earth hidden near red dwarf, could this water world reshape our future
Astronomers have found a new exoplanet named TOI-1846 b. This planet is nearly twice the size of Earth. It may contain a lot of water. The planet is 154 light-years away. It orbits a red dwarf star. Scientists used NASA's TESS data to find it. Further studies are needed to confirm its water content. Tired of too many ads? Remove Ads Tired of too many ads? Remove Ads Astronomers have discovered a new exoplanet nearly twice the size of Earth that may be rich in water, according to a study published on the arXiv preprint server. The planet, named TOI-1846 b , is located approximately 154 light-years from Earth and orbits a red dwarf star The discovery was led by Abderahmane Soubkiou and his team at the Oukaimeden Observatory in Morocco. The planet was detected using data from NASA 's Transiting Exoplanet Survey Satellite (TESS) and confirmed through ground-based photometry, high-resolution imaging, and spectroscopy.'We have validated TOI-1846 b using TESS and multicolor ground-based photometric data, high-resolution imaging, and spectroscopic observations,' the authors wrote, as reported by to the study, TOI-1846 b has a radius of approximately 1.792 times that of Earth and is about 4.4 times more massive. The planet completes one orbit around its host star every 3.93 days, suggesting it lies extremely close to the star. Its equilibrium temperature is estimated at 568.1 Kelvin (approximately 295°C).Researchers believe the planet likely has a water-rich composition, based on its size and density. However, they emphasized the need for further observations to confirm this. In particular, radial velocity (RV) measurements using instruments like MAROON-X could help determine its mass and internal structure more study also notes that the planet has a Transmission Spectroscopy Metric (TSM) of 47, which is below the benchmark value of 90 typically used for small sub-Neptune planets. This means that while its atmosphere may be more difficult to study, it remains a target of interest for future host star, TOI-1846, is a red dwarf with a mass of about 0.42 times that of the Sun and a radius of approximately 0.4 solar radii. It has an estimated age of 7.2 billion years and an effective temperature of 3,568 discovery adds to a growing list of super-Earths identified by astronomers in recent years. Earlier in 2025, researchers discovered another super-Earth, HD 20794 d, located just 20 light-years from Earth. That planet is about six times Earth's mass and lies within the habitable zone of its star, although its elliptical orbit may affect its potential to support b is not considered habitable due to its high temperature and close orbit, but its age and possible water-rich nature make it a valuable object for studying the formation and evolution of rocky exoplanets.
CNN
17-03-2025
- Science
- CNN
Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun
Summary Astronomers have discovered four sub-Earth size planets orbiting Barnard's Star, just six light-years from Earth. University of Chicago researchers used the MAROON-X instrument on Hawaii's Gemini North telescope to detect the planets. The planets are 19% to 34% of Earth's mass and complete their orbits in less than seven days. These small planets likely lack atmospheres and orbit too close to their star to be habitable. The discovery follows decades of false detections around Barnard's Star, Earth's nearest single star neighbor. After decades of searching, astronomers have uncovered some of the strongest evidence yet of exoplanets orbiting Barnard's Star, the nearest single star system to Earth. The four planets are classified as sub-Earths because each one is about 19% to 34% the mass of Earth, according to new research. 'It's a really exciting find — Barnard's Star is our cosmic neighbor, and yet we know so little about it,' said lead study author Ritvik Basant, doctoral student of astronomy and astrophysics at the University of Chicago, in a statement. 'It's signaling a breakthrough with the precision of these new instruments from previous generations.' Barnard's Star, discovered by American astronomer E.E. Barnard in 1916, is a low-mass red dwarf, one of the most common types of stars. Over the past decade, astronomers have found that many of these stars have multiple rocky planets orbiting them. Enter MAROON-X, an instrument mounted on the Gemini North telescope in Hawaii that's designed to search for exoplanets orbiting red dwarfs. The instrument seeks out planets by detecting the subtle wobble of stars as the gravity of orbiting planets tug on their stellar hosts, known as the radial velocity technique. Using MAROON-X, the study team spotted the least massive exoplanet ever found, and it hopes the find will lead to the discovery of more sub-Earth exoplanets across the cosmos. Astronomers believe smaller exoplanets may be more varied in composition than the larger exoplanets detected so far. Finding more minuscule worlds with the latest, highly sensitive instruments could open up a new way of understanding how planets form — and which ones could be habitable for life. A study detailing the findings was published March 11 in The Astrophysical Journal Letters. Four tiny worlds The planets are so small that they are more analogous to Mars, according to Basant. 'When compared to our solar system, each of the four planets are inside the distance of Mercury's orbit,' Basant said. The planets closely orbit Barnard's Star, zipping around their stellar host in a matter of days, compared with the year it takes Earth to complete one orbit around the sun. The outermost planet takes less than seven days to complete one orbit, while the innermost planet has an orbital period of less than three days, Basant said. Proximity at a price The planets are so close to the star that their surfaces are likely too hot to be means the foursome are also not within the habitable zone of the star, or just the right distance from the star where liquid water can stably exist on the surface of the planet. 'When Barnard's star was young and active … the star blasted these small planets with X-UV radiation, frequent flares, and dense winds,' said Edward Guinan, professor of astronomy and astrophysics at Villanova University in Pennsylvania, in an email. 'Because of this, these sub-Earth size planets probably don't have atmospheres, water, and life.' Guinan was not involved in the new study but has previously searched for planets around Barnard's Star. Planets of this size are largely unexplored beyond our solar system, making it a significant step forward as astronomers search for Earth-mass planets around sun-like stars, Basant said. 'A lot of what we do can be incremental, and it's sometimes hard to see the bigger picture,' said study coauthor Jacob Bean, a professor in the University of Chicago's department of astronomy and astrophysics. 'But we found something that humanity will hopefully know forever. That sense of discovery is incredible.' The search for nearby planets While the Proxima Centauri system is the closest to our solar system at a distance of 4.25 light-years away, it comprises three stars circling one another, making Barnard's Star the nearest single star system. Now, astronomers know that planets orbit the two closest star systems to our solar system. Barnard's Star has served as a kind of white whale for astronomers over the decades as they have tried to find evidence of planets orbiting it, only to be disproven as false positives later, 'likely due to the limited sensitivity of earlier instruments,' Basant said. Many exoplanets have been discovered as they transit, or pass in front of, their host star, creating an observable dip in starlight suggesting the presence of a planet. But the elusive planets orbiting Barnard's Star do not transit, meaning they don't pass in front of their star from the perspective of telescopes on Earth and can't be detected with powerful space observatories like the James Webb Space Telescope. The research team, led by Bean, captured data from Barnard's Star over the course of 112 nights spanning a period of three years. The data showed evidence for three planets orbiting Barnard's Star, two of which had been previously suggested as potential planets. The researchers then combined their findings with data captured using the ESPRESSO instrument on the Very Large Telescope in Chile by a different team that authored an October 2024 study. The combined dataset confirmed the existence of a fourth exoplanet. 'We observed at different times of night on different days. They're in Chile; we're in Hawaii. Our teams didn't coordinate with each other at all,' Basant said. 'That gives us a lot of assurance that these aren't phantoms in the data. It's thrilling to witness the precision of next-generation spectrographs like MAROON-X and ESPRESSO. Their ability to detect sub-Earth mass planets for the first time feels like unlocking a new level in a game, filled with unknown possibilities.' MAROON-X, which began as a temporary 'visitor' instrument, is now being converted to a permanent one after its detections. 'I am very happy to see that new MAROON-X data provide an independent confirmation of the planet b and candidates c and d, and together with the ESPRESSO data, the analysis makes the detection significantly more robust,' said Jonay González Hernández, lead author of the October 2024 paper and a researcher at the Instituto de Astrofísica de Canarias in Spain. He was not involved in the new study. Guinan said the planets described within the study 'look like a firm discovery.' 'Finally, real planets have been discovered around Barnard's Star after several false alarms over the past (50 years),' Guinan said.
Yahoo
17-03-2025
- Science
- Yahoo
Scientists Discover Four Intriguing Planets Around Closest Single-Star Solar System to Earth
Astronomers have spotted four smaller-than-Earth exoplanets orbiting the closest single-star system to us, called Barnard's Star. As detailed in a new paper published in the journal The Astrophysical Journal Letters, an international team of researchers discovered that the star — a small red dwarf star just 16 percent of our own Sun's mass and just under six light-years from Earth in the constellation Ophiuchus — has four tiny and seemingly rocky worlds orbiting it. According to the astronomers, these exoplanets — which are among the smallest ever discovered — could force us to reevaluate our understanding of how planets form and evolve. The four planets were spotted by the MAROON-X instrument, a highly sensitive piece of equipment attached to the Gemini North telescope at the International Gemini Observatory in Hilo, Hawaii. "It's a really exciting find — Barnard's Star is our cosmic neighbor, and yet we know so little about it," said University of Chicago PhD student and first author Ritvik Basant in a statement. "It's signaling a breakthrough with the precision of these new instruments from previous generations." MAROON-X was specifically designed to detect tiny exoplanets orbiting red dwarf stars by detecting the minuscule back-and-forth motion of a star caused by the gravitational pull of orbiting planets, a trick scientists call the radial velocity technique. Using the instrument, the team discovered four likely rocky exoplanets that are only anywhere from roughly 20 to 30 percent of the mass of Earth each. They orbit their star at an extremely close distance, completing a full revolution in a matter of a few Earth days. The team also used data from a 2024 study, which involved the ESPRESSO instrument at the European Southern Observatory's Very Large Telescope in Chile, to confirm the existence of one of the four exoplanets. Last year, astronomers detected an exoplanet with at least half the mass of Venus orbiting Barnard's Star. "We observed at different times of night on different days," said Basant in the statement. "They're in Chile; we're in Hawai'i. Our teams didn't coordinate with each other at all. That gives us a lot of assurance that these aren't phantoms in the data." One of the four exoplanets spotted by MAROON-X was the smallest to have been discovered using the radial velocity technique, which could set the stage for many future discoveries like it. Unfortunately, the planets are unlikely to harbor life since they're not in Barnard Star's habitable zone, the area around a star where temperatures allow liquid water to exist on a given planet's surface. "With the current dataset, we can confidently rule out any planets more massive than 40 to 60 percent of Earth's mass near the inner and outer edges of the habitable zone," Basant told "Additionally, we can exclude the presence of Earth-mass planets with orbital periods of up to a few years." But that doesn't necessarily mean that will also be the case for other single-star systems like it. As our exoplanet detection methods continue to improve, astronomers are hoping to spot even more rocky worlds, which may still turn out to be habitable. More on Barnard's Star: Astronomers Spot Mysterious Planet Orbiting the Closest Single Star
CNN
17-03-2025
- Science
- CNN
Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun
Summary Astronomers have discovered four sub-Earth size planets orbiting Barnard's Star, just six light-years from Earth. University of Chicago researchers used the MAROON-X instrument on Hawaii's Gemini North telescope to detect the planets. The planets are 19% to 34% of Earth's mass and complete their orbits in less than seven days. These small planets likely lack atmospheres and orbit too close to their star to be habitable. The discovery follows decades of false detections around Barnard's Star, Earth's nearest single star neighbor. After decades of searching, astronomers have uncovered some of the strongest evidence yet of exoplanets orbiting Barnard's Star, the nearest single star system to Earth. The four planets are classified as sub-Earths because each one is about 19% to 34% the mass of Earth, according to new research. 'It's a really exciting find — Barnard's Star is our cosmic neighbor, and yet we know so little about it,' said lead study author Ritvik Basant, doctoral student of astronomy and astrophysics at the University of Chicago, in a statement. 'It's signaling a breakthrough with the precision of these new instruments from previous generations.' Barnard's Star, discovered by American astronomer E.E. Barnard in 1916, is a low-mass red dwarf, one of the most common types of stars. Over the past decade, astronomers have found that many of these stars have multiple rocky planets orbiting them. Enter MAROON-X, an instrument mounted on the Gemini North telescope in Hawaii that's designed to search for exoplanets orbiting red dwarfs. The instrument seeks out planets by detecting the subtle wobble of stars as the gravity of orbiting planets tug on their stellar hosts, known as the radial velocity technique. Using MAROON-X, the study team spotted the least massive exoplanet ever found, and it hopes the find will lead to the discovery of more sub-Earth exoplanets across the cosmos. Astronomers believe smaller exoplanets may be more varied in composition than the larger exoplanets detected so far. Finding more minuscule worlds with the latest, highly sensitive instruments could open up a new way of understanding how planets form — and which ones could be habitable for life. A study detailing the findings was published March 11 in The Astrophysical Journal Letters. Four tiny worlds The planets are so small that they are more analogous to Mars, according to Basant. 'When compared to our solar system, each of the four planets are inside the distance of Mercury's orbit,' Basant said. The planets closely orbit Barnard's Star, zipping around their stellar host in a matter of days, compared with the year it takes Earth to complete one orbit around the sun. The outermost planet takes less than seven days to complete one orbit, while the innermost planet has an orbital period of less than three days, Basant said. Proximity at a price The planets are so close to the star that their surfaces are likely too hot to be means the foursome are also not within the habitable zone of the star, or just the right distance from the star where liquid water can stably exist on the surface of the planet. 'When Barnard's star was young and active … the star blasted these small planets with X-UV radiation, frequent flares, and dense winds,' said Edward Guinan, professor of astronomy and astrophysics at Villanova University in Pennsylvania, in an email. 'Because of this, these sub-Earth size planets probably don't have atmospheres, water, and life.' Guinan was not involved in the new study but has previously searched for planets around Barnard's Star. Planets of this size are largely unexplored beyond our solar system, making it a significant step forward as astronomers search for Earth-mass planets around sun-like stars, Basant said. 'A lot of what we do can be incremental, and it's sometimes hard to see the bigger picture,' said study coauthor Jacob Bean, a professor in the University of Chicago's department of astronomy and astrophysics. 'But we found something that humanity will hopefully know forever. That sense of discovery is incredible.' The search for nearby planets While the Proxima Centauri system is the closest to our solar system at a distance of 4.25 light-years away, it comprises three stars circling one another, making Barnard's Star the nearest single star system. Now, astronomers know that planets orbit the two closest star systems to our solar system. Barnard's Star has served as a kind of white whale for astronomers over the decades as they have tried to find evidence of planets orbiting it, only to be disproven as false positives later, 'likely due to the limited sensitivity of earlier instruments,' Basant said. Many exoplanets have been discovered as they transit, or pass in front of, their host star, creating an observable dip in starlight suggesting the presence of a planet. But the elusive planets orbiting Barnard's Star do not transit, meaning they don't pass in front of their star from the perspective of telescopes on Earth and can't be detected with powerful space observatories like the James Webb Space Telescope. The research team, led by Bean, captured data from Barnard's Star over the course of 112 nights spanning a period of three years. The data showed evidence for three planets orbiting Barnard's Star, two of which had been previously suggested as potential planets. The researchers then combined their findings with data captured using the ESPRESSO instrument on the Very Large Telescope in Chile by a different team that authored an October 2024 study. The combined dataset confirmed the existence of a fourth exoplanet. 'We observed at different times of night on different days. They're in Chile; we're in Hawaii. Our teams didn't coordinate with each other at all,' Basant said. 'That gives us a lot of assurance that these aren't phantoms in the data. It's thrilling to witness the precision of next-generation spectrographs like MAROON-X and ESPRESSO. Their ability to detect sub-Earth mass planets for the first time feels like unlocking a new level in a game, filled with unknown possibilities.' MAROON-X, which began as a temporary 'visitor' instrument, is now being converted to a permanent one after its detections. 'I am very happy to see that new MAROON-X data provide an independent confirmation of the planet b and candidates c and d, and together with the ESPRESSO data, the analysis makes the detection significantly more robust,' said Jonay González Hernández, lead author of the October 2024 paper and a researcher at the Instituto de Astrofísica de Canarias in Spain. He was not involved in the new study. Guinan said the planets described within the study 'look like a firm discovery.' 'Finally, real planets have been discovered around Barnard's Star after several false alarms over the past (50 years),' Guinan said.
Yahoo
17-03-2025
- Science
- Yahoo
Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun
Sign up for CNN's Wonder Theory science newsletter. Explore the universe with news on fascinating discoveries, scientific advancements and more. After decades of searching, astronomers have uncovered some of the strongest evidence yet of exoplanets orbiting Barnard's Star, the nearest single star system to Earth. The four planets are classified as sub-Earths because each one is about 19% to 34% the mass of Earth, according to new research. 'It's a really exciting find — Barnard's Star is our cosmic neighbor, and yet we know so little about it,' said lead study author Ritvik Basant, doctoral student of astronomy and astrophysics at the University of Chicago, in a statement. 'It's signaling a breakthrough with the precision of these new instruments from previous generations.' Barnard's Star, discovered by American astronomer E.E. Barnard in 1916, is a low-mass red dwarf, one of the most common types of stars. Over the past decade, astronomers have found that many of these stars have multiple rocky planets orbiting them. Enter MAROON-X, an instrument mounted on the Gemini North telescope in Hawaii that's designed to search for exoplanets orbiting red dwarfs. The instrument seeks out planets by detecting the subtle wobble of stars as the gravity of orbiting planets tug on their stellar hosts, known as the radial velocity technique. Using MAROON-X, the study team spotted the least massive exoplanet ever found, and it hopes the find will lead to the discovery of more sub-Earth exoplanets across the cosmos. Astronomers believe smaller exoplanets may be more varied in composition than the larger exoplanets detected so far. Finding more minuscule worlds with the latest, highly sensitive instruments could open up a new way of understanding how planets form — and which ones could be habitable for life. A study detailing the findings was published March 11 in The Astrophysical Journal Letters. The planets are so small that they are more analogous to Mars, according to Basant. 'When compared to our solar system, each of the four planets are inside the distance of Mercury's orbit,' Basant said. The planets closely orbit Barnard's Star, zipping around their stellar host in a matter of days, compared with the year it takes Earth to complete one orbit around the sun. The outermost planet takes less than seven days to complete one orbit, while the innermost planet has an orbital period of less than three days, Basant said. The planets are so close to the star that their surfaces are likely too hot to be means the foursome are also not within the habitable zone of the star, or just the right distance from the star where liquid water can stably exist on the surface of the planet. 'When Barnard's star was young and active … the star blasted these small planets with X-UV radiation, frequent flares, and dense winds,' said Edward Guinan, professor of astronomy and astrophysics at Villanova University in Pennsylvania, in an email. 'Because of this, these sub-Earth size planets probably don't have atmospheres, water, and life.' Guinan was not involved in the new study but has previously searched for planets around Barnard's Star. Planets of this size are largely unexplored beyond our solar system, making it a significant step forward as astronomers search for Earth-mass planets around sun-like stars, Basant said. 'A lot of what we do can be incremental, and it's sometimes hard to see the bigger picture,' said study coauthor Jacob Bean, a professor in the University of Chicago's department of astronomy and astrophysics. 'But we found something that humanity will hopefully know forever. That sense of discovery is incredible.' While the Proxima Centauri system is the closest to our solar system at a distance of 4.25 light-years away, it comprises three stars circling one another, making Barnard's Star the nearest single star system. Now, astronomers know that planets orbit the two closest star systems to our solar system. Barnard's Star has served as a kind of white whale for astronomers over the decades as they have tried to find evidence of planets orbiting it, only to be disproven as false positives later, 'likely due to the limited sensitivity of earlier instruments,' Basant said. Many exoplanets have been discovered as they transit, or pass in front of, their host star, creating an observable dip in starlight suggesting the presence of a planet. But the elusive planets orbiting Barnard's Star do not transit, meaning they don't pass in front of their star from the perspective of telescopes on Earth and can't be detected with powerful space observatories like the James Webb Space Telescope. The research team, led by Bean, captured data from Barnard's Star over the course of 112 nights spanning a period of three years. The data showed evidence for three planets orbiting Barnard's Star, two of which had been previously suggested as potential planets. The researchers then combined their findings with data captured using the ESPRESSO instrument on the Very Large Telescope in Chile by a different team that authored an October 2024 study. The combined dataset confirmed the existence of a fourth exoplanet. 'We observed at different times of night on different days. They're in Chile; we're in Hawaii. Our teams didn't coordinate with each other at all,' Basant said. 'That gives us a lot of assurance that these aren't phantoms in the data. It's thrilling to witness the precision of next-generation spectrographs like MAROON-X and ESPRESSO. Their ability to detect sub-Earth mass planets for the first time feels like unlocking a new level in a game, filled with unknown possibilities.' MAROON-X, which began as a temporary 'visitor' instrument, is now being converted to a permanent one after its detections. 'I am very happy to see that new MAROON-X data provide an independent confirmation of the planet b and candidates c and d, and together with the ESPRESSO data, the analysis makes the detection significantly more robust,' said Jonay González Hernández, lead author of the October 2024 paper and a researcher at the Instituto de Astrofísica de Canarias in Spain. He was not involved in the new study. Guinan said the planets described within the study 'look like a firm discovery.' 'Finally, real planets have been discovered around Barnard's Star after several false alarms over the past (50 years),' Guinan said.
