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Supreme Court stays CBI probe against Kerala Chief Minister's top advisor
Supreme Court stays CBI probe against Kerala Chief Minister's top advisor

India Today

time30-04-2025

  • Politics
  • India Today

Supreme Court stays CBI probe against Kerala Chief Minister's top advisor

The Supreme Court stayed a Kerala High Court order that had previously directed the Central Bureau of Investigation (CBI) to register a First Information Report (FIR) and investigate KM Abraham, Chief Principal Secretary to Kerala Chief Minister Pinarayi Vijayan, in a case related to disproportionate assets.A bench of Justices Dipankar Datta and Manmohan made this ruling while responding to an appeal filed by Abraham. The court also issued a notice to the CBI, the Kerala government, and the complainant, asking them to respond to the issues raised in Abraham's Abraham, senior advocate R Basant argued that the FIR, registered under the Prevention of Corruption Act, was procedurally invalid. Basant supported his claim by citing Section 17A of the Act which mandates prior sanction from a competent authority before registering an FIR against a public servant. According to Basant, no such sanction was obtained in Abraham's case. The Kerala High Court had, on April 11, based on a petition filed by activist Jomon Puthenpurackal, directed the CBI to take over the investigation. The High Court stated that Abraham appeared to own properties beyond his known income, including a Rs 3 crore apartment in Mumbai, a Rs 1 crore flat in Thiruvananthapuram and a shopping complex in Kollam worth Rs 8 Vigilance and Anti-Corruption Bureau had previously probed the matter but the High Court found their investigation unreliable, stating it 'wouldn't instill confidence in the public.' As a result, the High Court insisted that a central agency like the CBI was needed to ensure a fair and unbiased the court criticised a 2017 decision by the Enquiry Commissioner-cum-Special Judge in Thiruvananthapuram, who had dismissed the original complaint against Abraham. The High Court described that decision as 'perverse and wholly unreasonable', noting that the judge had failed to consider important details about the properties Abraham had allegedly on his part, has denied all allegations, stating that all the properties were legally acquired and there was no By Devang Durlav Das IN THIS STORY#Kerala

Several planets found orbiting star less than 6 light-years away
Several planets found orbiting star less than 6 light-years away

Yahoo

time18-03-2025

  • Science
  • Yahoo

Several planets found orbiting star less than 6 light-years away

Astronomers have confirmed the existence of four planets orbiting a star less than 6 light-years away with help from some of the world's most powerful telescopes. Research published in October 2024 revealed that one planet was rotating around Barnard's Star, the second-closest single star system to Earth. But a combination of telescopes all over the world confirmed the presence of four small exoplanets, according to a study published last week in The Astrophysical Journal Letters. MORE: How global warming could threaten satellites, according to new study The Gemini Telescope in Hawaii and the Very Large Telescope in Chile were used to detect the additional rocky planets, the astronomers said. "It's signaling a breakthrough with the precision of these new instruments from previous generations," said Ritvik Basant, Ph.D student at the University of Chicago and lead author of the paper, in a statement. The first planet was detected using a 27-foot diameter telescope at the European Space Observatory's Paranal Observatory in Chile and a spectrograph that could quickly detect changes in the star's velocity, according to the 2024 paper, published in the journal Astronomy & Astrophysics. MORE: 3.5 billion-year-old crater created by meteorite impact found in Australia, scientists say Barnard's Star, a low-mass red dwarf, was discovered in 1916. Since then, astronomers have discovered that at least 70% of all stars in the Milky Way are this type of star, which is why researchers want to know about the types of planets that orbit them, according to the University of Chicago. "It's a really exciting find -- Barnard's Star is our cosmic neighbor, and yet we know so little about it," Basant said. The planets are 20% to 30% the mass of Earth and make a full orbit around the sun in days, according to the paper. They are likely rocky planets, rather than gas. Since they are so close to Barnard's Star, they are likely too hot to sustain life. The researchers ruled out the existence of other planets within the habitable zone of Barnard's Star. MORE: Parade of planets this month will feature celestial bodies in alignment The planets are difficult to detect because their stars shine so brightly next to them, the researchers said. Scientists from the Gemini Observatory, National Science Foundation NOIRLab, Heidelberg University and the University of Amsterdam calibrated and analyzed data taken during 112 different nights over three years, where they found "solid evidence" to the existence of the additional planets orbiting Barnard's Star, according to the paper. "We observed at different times of night on different days," Basant said. "They're in Chile; we're in Hawaii. Our teams didn't coordinate with each other at all." MORE: Binary star system found near the Milky Way's black hole: An 'amazing' discovery, astrophysicists say He added, "That gives us a lot of assurance that these aren't phantoms in the data." Several planets found orbiting star less than 6 light-years away originally appeared on

Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun
Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun

CNN

time17-03-2025

  • 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.

Scientists Discover Four Intriguing Planets Around Closest Single-Star Solar System to Earth
Scientists Discover Four Intriguing Planets Around Closest Single-Star Solar System to Earth

Yahoo

time17-03-2025

  • 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

Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun
Entire planetary system of four tiny exoplanets found orbiting the nearest single star to the sun

CNN

time17-03-2025

  • 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.

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