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Time of India
10 hours ago
- Science
- Time of India
Kepler-139f: The massive planet that remained 'invisible' to scientists for years
Astronomers have recently discovered a massive exoplanet, Kepler-139f, hidden within a known star system. This Neptune-sized planet, 36 times the mass of Earth, eluded detection until 2025 due to its inclined orbit, which prevents it from transiting its star from Earth's perspective. It is well known that the universe still hides millions of secrets that remain to be discovered from the dark silences of space Recently, astronomers made a discovery hidden in plain sight. Despite orbiting a star system already known to host several planets, this giant exoplanet somehow evaded detection for years. Astronomers announced the discovery of Kepler‑139f, which is a massive exoplanet approximately 36 times the mass of Earth, around twice as large as Neptune, yet it stayed invisible until 2025. Orbiting a G‑type star similar to our Sun, Kepler‑139f completes one orbit in about 355 days, roughly at 1 AU distance, as reported in a study published in The Astrophysical Journal Letters. So, why was such a large planet missed for so long The key to its secret lies in its unusual orbit. NASA's Kepler Space Telescope, which discovered thousands of exoplanets through the transit method, only detects planets that pass directly between the star and Earth, causing slight dips in starlight. Kepler‑139f's orbit is inclined, so it never transits from our vantage point, remaining invisible to the primary detection method. What method did scientists use this time To find out Kepler‑139f, scientists used a combination of radial velocity (RV) and transit timing variations (TTVs). by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Passive Income Ideas Sitting at Home Mone Undo RV measures how a star wobbles due to gravitational pull from orbiting planets, while TTVs capture irregularities in known planets' transit timings caused by unseen companions. As Caleb Lammers, a graduate student in the Department of Astrophysical Science at Princeton and co-author of the study, told 'When you observe TTVs that cannot be attributed to the known planets, you can be fairly confident that there is an unseen body in the system'. After the 2023 discovery of Kepler‑139e, scientists went back and rechecked earlier data using RV and TTV methods. This helped them spot Kepler‑139f, hidden between the smaller planet Kepler‑139c and the gas giant Kepler‑139e. According to Lammers, 'Many planetary systems likely host invisible worlds—particularly in their distant orbits.' Since traditional planet-hunting methods rely on perfect orbital alignment with Earth, many such planets can go unnoticed. That's why using a mix of techniques like RV, TTV, and upcoming missions like ESA's PLATO, launching in 2026, will be important in finding more of these hidden, massive worlds.
Scottish Sun
a day ago
- Science
- Scottish Sun
Breakthrough in hunt for ALIENS as scientists find treasure trove of ‘ingredients for life' near distant baby star
The birth of stars is violent, emitting such a huge amount of energy that astronomers assumed these seeds of life would be obliterated SPACE TRACE Breakthrough in hunt for ALIENS as scientists find treasure trove of 'ingredients for life' near distant baby star Click to share on X/Twitter (Opens in new window) Click to share on Facebook (Opens in new window) THE key ingredients for life may be scattered across the universe in more places than first thought, according to a new study. From prebiotic molecules in comets, to chemicals floating in the dust of interstellar space, scientists have traced the building blocks of life all across space. Sign up for Scottish Sun newsletter Sign up 1 Instead of destroying these precious organic compounds, the star may actually be freeing them from these icy surfaces Astronomers have recently discovered the key components to life swirling around a remote baby star roughly 1,300 light-years from Earth. A protostar called V883 Orionis, tucked away in the constellation Orion, contains 17 complex organic molecules, including ethylene glycol and glycolonitrile. These are the precursors to components found in DNA and RNA - which build all living things. The study, published in the The Astrophysical Journal Letters, suggests the key components for life are far more common throughout the universe - offering a glimpse of hope for Earth's alien hunters. While similar compounds have been discovered elsewhere in the cosmos, astronomers assumed it wouldn't be possible so close to a star. The birth of stars is violent, emitting such a huge amount of energy that astronomers assumed these seeds of life would be obliterated. It was thought that only the rare planetary systems - like Earth - would be capable of reproducing them. "Now it appears the opposite is true," study co-author Kamber Schwarz, an astrochemist at the Max Planck Institute for Astronomy in Heidelberg, Germany, said in a statement. "Our results suggest that protoplanetary discs inherit complex molecules from earlier stages, and the formation of complex molecules can continue during the protoplanetary disc stage." Huge leap in search for aliens after 'building blocks for LIFE' found on ancient asteroid Bennu from lost watery world Using the Atacama Large Millimeter/submillimeter Array (ALMA) in northern Chile, scientists spotted emission lines from a cluster of organic molecules inside a debris and gas rich disk encircling V883 Orionis. This is in spite of the baby star pumping out powerful bursts of radiation. "These outbursts are strong enough to heat the surrounding disc as far as otherwise icy environments, releasing the chemicals we have detected," study first author Abubakar Fadul, a graduate student at the Max Planck Institute for Astronomy, added. The organic compounds form on specks of ice in the debris and gas disk. Instead of destroying these precious organic compounds, the star may actually be freeing them from these icy surfaces. The researchers still need more data to see how well these compounds hold up as their host star grows. "Perhaps we also need to look at other regions of the electromagnetic spectrum to find even more evolved molecules," Fadul said. "Who knows what else we might discover?" All you need to know about planets in our solar system Our solar system is made up of nine planets with Earth the third closest to the Sun. But each planet has its own quirks, so find out more about them all... How old is Earth? Plus other facts on our planet How many moons does Mercury have? What colour is Venus? How far away is Mars to Earth? And other facts on the red planet How big is Jupiter? How many moons does Saturn have? Does Uranus have rings? How many moons does Neptune have? How big is Pluto? How hot is the Sun?
Time of India
6 days ago
- Science
- Time of India
Astronomers discover blazing Betelgeuse has companion star
This is an AI generated image. Used for representation purpose only. Since at least the time of the ancient Egyptians, people across the world have gazed up in awe at Betelgeuse , one of the brightest stars blazing in the night sky. Now astronomers have discovered that this red supergiant , known to many as the hunter's shoulder in the Orion constellation , is being orbited by a much smaller companion star , a study said on Monday. It is not the first time Betelgeuse has surprised stargazers. Seemingly out of nowhere, the giant star dramatically dimmed for five months between 2019 and 2020, leading some scientists to suggest it could soon die in an epic supernova explosion. Further observations revealed that this event -- known as the " Great Dimming " -- was actually caused by material ejected from the surface that cooled part of the star, creating a dust cloud that blocked its light. by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Swelling and internal bleeding in the brain, help this baby Donate For Health Donate Now Undo But scientists could still not explain why Betelgeuse's brightness changes regularly, both on a 400-day cycle and another that lasts nearly six years. In a paper titled "A Buddy for Betelgeuse" published in December, some researchers theorised that the longer variation could be caused by a hidden small star orbiting the behemoth. Astronomers using the Gemini North telescope in Hawaii have now discovered this elusive companion, according to a new study in The Astrophysical Journal Letters. - Little buddy - This companion has a mass around 1.5 times greater than our Sun, the research estimated. That means it is dwarfed by Betelgeuse, which is 1,000 times bigger than the Sun. The companion star is around four times the distance from Betelgeuse as the Earth is from the Sun, which is quite close for a stellar companion. The discovery is the first time such a close companion star has been detected orbiting a supergiant, according to a statement from the US research centre NOIRLab, which operates the Gemini Observatory. Betelgeuse is more than 10,000 times brighter than the Sun, its blinding light making spotting anything nearby difficult. Steve Howell, a NASA scientist who led the research team, said previous "papers that predicted Betelgeuse's companion believed that no one would likely ever be able to image it". However the Gemini North telescope was able to spot the much smaller, dimmer star using a technique called speckle imaging. This involves assembling many images taken with short exposure times to overcome the distortions that Earth's atmosphere causes ground-bound telescopes. According to Greek myth, the giant hunter Orion claimed he would kill all the world's beasts, so Earth goddess Gaia sent a scorpion to kill him. God king Zeus then turned both Orion and the scorpion -- Scorpius -- into constellations. Earlier, ancient Egyptians included Betelgeuse in the constellation Osiris, their god of the dead. Even earlier, research has suggested that Indigenous Australians included Betelgeuse in their own constellations -- and had noticed the star's varying brightness.
The Hindu
17-07-2025
- Science
- The Hindu
IIST team discovers radio emission with circular polarisation near a massive young protostar
An international team led by astronomers from the Indian Institute of Space Science and Technology (IIST) here has discovered radio emission with a special property known as circular polarisation near a massive young protostar that is still forming about 4,500 light years from earth. [Protostar refers to the earliest known stage of a star when it is still accumulating gas and dust material from its surroundings.] The discovery linked to IRAS 18162-2048, a massive protostar in the Milky Way galaxy, opens an exciting window into scientists' understanding of how massive stars form, astronomers at the IIST said on Thursday. Circular polarisation occurs when electric and magnetic field vectors of electromagnetic waves—in this case radio waves—rotate in a circle about the direction in which the waves travel through space. This emission offers the first direct clue to the strength of magnetic fields in the immediate neighbourhood of a protostar, they said. The findings have been published in The Astrophysical Journal Letters under the title 'First Detection of Circular Polarization in Radio Continuum Toward a Massive Protostar.' In the early stage, the protostar can also eject high-velocity material in opposite directions, known as a bipolar jet. 'Massive protostars' evolve to have mass more than 8 to 10 times that of the Sun. Protostellar jets According to the astronomers, IRAS 18162-2048 powers one of the largest and brightest known protostellar jets in the Milky Way, the HH80-81 jet. It is believed that the magnetic field and rotation in the protostellar system are responsible for the ejection of the jet. While a magnetic field has been imaged from the jet earlier, this is the first time that hints of it have been detected directly from this massive protostar, according to the IIST. Strong magnetic fields have been observed earlier in low-mass protostars that go on to form stars like the Sun. But measuring such fields around massive protostars has remained elusive, until now. Much harder to study 'Massive protostars are much harder to study. The circular polarisation we are looking for is very faint and sporadic, making such measurements very challenging,' Amal George Cheriyan from the IIST, lead author of the paper, said in a statement. The radio observations were carried out using the National Radio Astronomy Observatory's (NRAO) Karl G. Jansky Very Large Array (VLA) in the U.S. 'This is the first inference of the magnetic field strength using circular polarisation in radio waves from a massive protostar,' said Sarita Vig of the IIST who conceptualised the work. Remarkable result 'The detection of circular polarisation is an exceptionally rare and challenging feat even in active galactic nuclei (AGNs), where conditions are extreme, but better investigated,' Nirupam Roy from the Indian Institute of Science (IISc), Bengaluru, said. Samir Mandal of the IIST noted that observing the phenomenon in the environment of a massive protostar, which lies buried in dense gas and dust, is even more difficult, making this result remarkable. The new data has allowed researchers to infer that the magnetic field near the protostar is roughly 100 times stronger than the Earth's magnetic field. They also support a long-standing theory that powerful jets from stars and black holes are driven by the same magnetic engine.
Arab Times
16-07-2025
- Science
- Arab Times
Astronomers discover hidden alien planet 35 times heavier than Earth
NEW YORK, July 16: Astronomers have uncovered a previously undetected alien planet, Kepler-139f, by analyzing the orbits of known planets within the Kepler-139 star system. This hidden exoplanet is about twice the mass of Neptune and 35 times the mass of Earth, taking approximately 355 days to orbit its host star. The discovery was published on May 2, 2025, in The Astrophysical Journal Letters. Kepler-139f had managed to remain elusive due to limitations in early detection methods used by NASA's Kepler Space Telescope. Kepler, which identified nearly 3,000 exoplanets over its nine-year mission, primarily detected planets that passed directly between their star and Earth, causing a brief dimming of the star's light. This allowed scientists to identify the size of these planets. However, Kepler could not detect planets that were positioned above or below the line of sight of the telescope, meaning some planets remained hidden. However, because Kepler-139 is home to multiple planets, astronomers had the opportunity to search for worlds outside of Kepler's original detection range. The system was known to contain three rocky super-Earths that transit their star, and later, a fourth gas giant was discovered. Astronomers observed gaps in the orbits of these planets, suggesting the presence of an additional, unseen world. By studying these orbital gaps in detail, scientists were able to infer the existence of Kepler-139f. "The challenge isn't in finding non-transiting planets but in identifying situations where we can deduce the location of these hidden worlds," explained Caleb Lammers, a graduate student at Princeton University and co-author of the study. "It was through precise measurements of the known planets' orbits, including radial velocity (RV) and transit timing variations (TTVs), that we could infer the existence of Kepler-139f." The RV technique measures the gravitational pull a planet exerts on its host star, helping astronomers determine the planet's mass. Additionally, TTVs—subtle variations in the timing of transits of known planets—can indicate the presence of other planets that don't transit the star themselves. Lammers and his colleague, Joshua Winn, an astrophysicist at Princeton and participating scientist on the Kepler mission, worked together to identify these gaps in the system. Using a combination of RV and TTV measurements, the pair discovered Kepler-139f nestled between the outermost super-Earth and a gas giant in the system. Kepler-139f's discovery also provided clarity on the previously puzzling density of Kepler-139c, the outermost super-Earth in the system. The earlier density readings were incorrectly influenced by the pull of the hidden planet, but with Kepler-139f identified, the team revised the data, providing more typical density values for Kepler-139c. The discovery raises the possibility that other unseen planets may be lurking in the Kepler-139 system. "There may still be other undiscovered planets in the system, especially given the prominent gap between planets b and c," said Lammers. "The challenge now is to find them." While the Kepler and TESS (Transiting Exoplanet Survey Satellite) missions have been adept at detecting planets closer to their stars—where transits are more frequent and easier to observe—planets further away with wider orbits present more difficulties. Additionally, the RV method is more effective for detecting larger, more massive planets due to their stronger gravitational influence. This bias toward larger worlds has made it harder to detect smaller, more distant planets, particularly those that don't transit their stars. To combat these challenges, astronomers are combining multiple methods—transits, RVs, and TTVs—to identify smaller, hidden planets. "It's likely that many planetary systems host unseen worlds, particularly in their outer regions," Lammers added. Looking ahead, the European Space Agency's upcoming PLATO mission, launching in 2026, will provide an even more powerful tool for detecting these hidden planets. PLATO will survey transiting planets and revisit the Kepler field, refining TTV measurements and boosting the potential for discovering more misaligned and hidden worlds. "In the near future, TTV-based planet detection is expected to accelerate significantly with the PLATO mission," Lammers concluded.
