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For first time, Webb telescope discovers an alien planet

For first time, Webb telescope discovers an alien planet

GMA Network15 hours ago

An image of the protoplanetary disk around the star TWA 7, recorded using the European Southern Observatory's Chile-based Very Large Telescope's SPHERE instrument, is seen with an image captured with the James Webb Space Telescope's MIRI instrument overlayed in this image released on June 25, 2025. The empty area around exoplanet TWA 7 B is shown in the R2 ring, CC #1. AM Lagrange et al/JWST/ESO/Handout via REUTERS
WASHINGTON — In addition to providing a trove of information about the early universe, the James Webb Space Telescope since its 2021 launch has obtained valuable data on various already-known planets beyond our solar system, called exoplanets. Now, for the first time, Webb has discovered an exoplanet not previously known.
Webb has directly imaged a young gas giant planet roughly the size of Saturn, our solar system's second-largest planet, orbiting a star smaller than the sun located about 110 light-years from Earth in the constellation Antlia, researchers said. A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km).
A never-before-seen planet! ????
This is Webb's first discovery of a planet using direct imaging. With a mass similar to Saturn, it's also the lightest exoplanet yet seen using this technique! https://t.co/ptWcXlFfmW pic.twitter.com/XTGwIqgH8n — NASA Webb Telescope (@NASAWebb) June 25, 2025
Most of the roughly 5,900 exoplanets discovered since the 1990s have been detected using indirect methods, such as through observation of the slight dimming of a star's light when a planet passes in front of it, called the transit method. Less than 2% of them have been directly imaged, as Webb did with the newly identified planet.
While this planet is large when considered in the context of our solar system, it is actually the least massive one ever discovered through direct imaging—10 times less massive than the previous record holder. This speaks to the sensitivity of Webb's instruments.
This discovery was achieved using a French-produced coronagraph, a device that blocks out the bright light from a star, installed on Webb's Mid-Infrared Instrument, or MIRI.
"Webb opens a new window—in terms of mass and the distance of a planet to the star—of exoplanets that had not been accessible to observations so far. This is important to explore the diversity of exoplanetary systems and understand how they form and evolve," said astronomer Anne-Marie Lagrange of the French research agency CNRS and LIRA/Observatoire de Paris, lead author of the study published on Wednesday in the journal Nature.
The planet orbits its host star, called TWA 7, at a distance about 52 times greater than Earth's orbital distance from the sun. To put that in perspective, our solar system's outermost planet Neptune orbits about 30 times further from the sun than Earth. The transit method of discovering exoplanets is particularly useful for spotting those orbiting close to their host star rather than much further out like the newly identified one.
"Indirect methods provide incredible information for planets close to their stars. Imaging is needed to robustly detect and characterize planets further away, typically 10 times the Earth- to-sun distance," Lagrange said.
The birth of a planetary system begins with a large cloud of gas and dust—called a molecular cloud— that collapses under its own gravity to form a central star. Leftover material spinning around the star in what is called a protoplanetary disk forms planets.
The star and the planet in this research are practically newborns—about 6 million years old, compared to the age of the sun and our solar system of roughly 4.5 billion years.
Because of the angle at which this planetary system is being observed—essentially looking at it from above rather than from the side—the researchers were able to discern the structure of the remaining disk. It has two broad concentric ring-like structures made up of rocky and dusty material and one narrow ring in which the planet is sitting.
The researchers do not yet know the composition of the planet's atmosphere, though future Webb observations may provide an answer. They also are not certain whether the planet, being as young as it is, is still gaining mass by accumulating additional material surrounding it.
While this planet is the smallest ever directly imaged, it is still much more massive than rocky planets like Earth that might be good candidates in the search for life beyond our solar system. Even with its tremendous capabilities of observing the cosmos in near-infrared and mid-infrared wavelengths, Webb is still not able to directly image Earth-sized exoplanets.
"Looking forward, I do hope the projects of direct imaging of Earth-like planets and searches for possible signs of life will become a reality," Lagrange said. — Reuters

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For first time, Webb telescope discovers an alien planet
For first time, Webb telescope discovers an alien planet

GMA Network

time15 hours ago

  • GMA Network

For first time, Webb telescope discovers an alien planet

An image of the protoplanetary disk around the star TWA 7, recorded using the European Southern Observatory's Chile-based Very Large Telescope's SPHERE instrument, is seen with an image captured with the James Webb Space Telescope's MIRI instrument overlayed in this image released on June 25, 2025. The empty area around exoplanet TWA 7 B is shown in the R2 ring, CC #1. AM Lagrange et al/JWST/ESO/Handout via REUTERS WASHINGTON — In addition to providing a trove of information about the early universe, the James Webb Space Telescope since its 2021 launch has obtained valuable data on various already-known planets beyond our solar system, called exoplanets. Now, for the first time, Webb has discovered an exoplanet not previously known. Webb has directly imaged a young gas giant planet roughly the size of Saturn, our solar system's second-largest planet, orbiting a star smaller than the sun located about 110 light-years from Earth in the constellation Antlia, researchers said. A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). A never-before-seen planet! ???? This is Webb's first discovery of a planet using direct imaging. With a mass similar to Saturn, it's also the lightest exoplanet yet seen using this technique! — NASA Webb Telescope (@NASAWebb) June 25, 2025 Most of the roughly 5,900 exoplanets discovered since the 1990s have been detected using indirect methods, such as through observation of the slight dimming of a star's light when a planet passes in front of it, called the transit method. Less than 2% of them have been directly imaged, as Webb did with the newly identified planet. While this planet is large when considered in the context of our solar system, it is actually the least massive one ever discovered through direct imaging—10 times less massive than the previous record holder. This speaks to the sensitivity of Webb's instruments. This discovery was achieved using a French-produced coronagraph, a device that blocks out the bright light from a star, installed on Webb's Mid-Infrared Instrument, or MIRI. "Webb opens a new window—in terms of mass and the distance of a planet to the star—of exoplanets that had not been accessible to observations so far. This is important to explore the diversity of exoplanetary systems and understand how they form and evolve," said astronomer Anne-Marie Lagrange of the French research agency CNRS and LIRA/Observatoire de Paris, lead author of the study published on Wednesday in the journal Nature. The planet orbits its host star, called TWA 7, at a distance about 52 times greater than Earth's orbital distance from the sun. To put that in perspective, our solar system's outermost planet Neptune orbits about 30 times further from the sun than Earth. The transit method of discovering exoplanets is particularly useful for spotting those orbiting close to their host star rather than much further out like the newly identified one. "Indirect methods provide incredible information for planets close to their stars. Imaging is needed to robustly detect and characterize planets further away, typically 10 times the Earth- to-sun distance," Lagrange said. The birth of a planetary system begins with a large cloud of gas and dust—called a molecular cloud— that collapses under its own gravity to form a central star. Leftover material spinning around the star in what is called a protoplanetary disk forms planets. The star and the planet in this research are practically newborns—about 6 million years old, compared to the age of the sun and our solar system of roughly 4.5 billion years. Because of the angle at which this planetary system is being observed—essentially looking at it from above rather than from the side—the researchers were able to discern the structure of the remaining disk. It has two broad concentric ring-like structures made up of rocky and dusty material and one narrow ring in which the planet is sitting. The researchers do not yet know the composition of the planet's atmosphere, though future Webb observations may provide an answer. They also are not certain whether the planet, being as young as it is, is still gaining mass by accumulating additional material surrounding it. While this planet is the smallest ever directly imaged, it is still much more massive than rocky planets like Earth that might be good candidates in the search for life beyond our solar system. Even with its tremendous capabilities of observing the cosmos in near-infrared and mid-infrared wavelengths, Webb is still not able to directly image Earth-sized exoplanets. "Looking forward, I do hope the projects of direct imaging of Earth-like planets and searches for possible signs of life will become a reality," Lagrange said. — Reuters

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PH-Japan educational ties strengthen 'Golden Age' relations — envoy

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Webb telescope spots infant planets in different stages of development
Webb telescope spots infant planets in different stages of development

GMA Network

time13-06-2025

  • GMA Network

Webb telescope spots infant planets in different stages of development

An artist's rendition of the sun-like star YSES-1 in the center, with the planet YSES-1 b and its dusty circumplanetary disk (right) and the planet YSES-1 c with silicate clouds in its atmosphere (left), is seen in this handout image obtained by Reuters on June 11, 2025. Ellis Bogat/Handout via REUTERS/Illustration WASHINGTON - The James Webb Space Telescope has observed two large planets at different stages of infancy - one with an atmosphere brimming with dusty clouds and the other encircled by a disk of material - orbiting a young sun-like star in a discovery that illustrates the complex nature of how planetary systems develop. The two gas giant planets, both more massive than our solar system's largest planet Jupiter, were directly imaged by Webb in a planetary system located in the Milky Way galaxy about 310 light years from Earth in the direction of the constellation Musca. A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). Astronomers have detected more than 5,900 planets beyond our solar system - called exoplanets - since the 1990s, with less than 2% of these directly imaged like these two. It is rare to find exoplanets in their early developmental stages. The birth of a planetary system begins with a large cloud of gas and dust - called a molecular cloud - that collapses under its own gravity to form a central star. Leftover material spinning around the star in what is called a protoplanetary disk forms planets. This planetary system was observed by Webb very early in its developmental history. The star, named YSES-1, is about the same mass as the sun. The two planets orbit a long distance from the star, each probably needing thousands of years to complete a single orbit. While the sun is roughly 4.5 billion years old, this star is approximately 16 million years old, a veritable newborn. The researchers were surprised to find that the two neonatal planets observed by Webb appeared to be at different stages of development. The innermost of the two has a mass about 14 times greater than Jupiter and orbits the star at a distance 160 times greater than Earth orbits the sun and more than five times as far as our solar system's outermost planet Neptune. The planet is surrounded by a disk of small-grained dust, a state one might expect in a very early stage of formation when it is still coalescing, or perhaps if there has been a collision of some kind or a moon is in the process of taking shape. Webb spotted water and carbon monoxide in its atmosphere. The outermost planet has a mass about six times greater than that of Jupiter and orbits the star at 320 times the distance of Earth to the sun. Its atmosphere is loaded with silicate clouds, differing from our solar system's gas giants. Webb also detected methane, water, carbon monoxide and carbon dioxide in the atmosphere. It has no disk of material around it. The puzzling combination of traits presented by these two planets in the same system illustrates "the complex landscape that is planet formation and shows how much we truly don't know about how planetary systems came to be, including our own," said astrophysicist Kielan Hoch of the Space Telescope Science Institute in Baltimore, who led the study published this week in the journal Nature. "Theoretically, the planets should be forming around the same time, as planet formation happens fairly quickly, within about one million years," Hoch said. A real mystery is the location where the planets formed, Hoch added, noting that their orbital distance from the host star is greater than would be expected if they formed in the protoplanetary disk. "Furthermore, why one planet still retains material around it and one has distinct silicate clouds remains a big question. Do we expect all giant planets to form the same way and look the same if they formed in the same environment? These are questions we have been investigating for ages to place the formation of our own solar system into context," Hoch said. In addition to amassing a trove of discoveries about the early universe since becoming operational in 2022, Webb has made a major contribution to the study of exoplanets with its observations at near- and mid-infrared wavelengths. "Webb is revealing all sorts of atmospheric physics and chemistry happening in exoplanets that we didn't know before, and is currently challenging every atmospheric model we used pre-Webb," Hoch said. — Reuters

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