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Space & Physics

Astronomers discover nearby “Super-Jupiter” planet

The planet, named Epsilon Indi Ab, is the first directly imaged mature exoplanet close to the Earth. The astronomers discovered a planet through Direct Imaging techniques using the James Webb Space Telescope

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Artist’s impression of a cold gas giant orbiting a red dwarf. Only a point of light is visible on the JWST/MIRI images. Nevertheless, the initial analysis suggests the presence of a gaseous planet that may have properties similar to Jupiter. Credit: T. Müller (MPIA/HdA)

In a breakthrough discovery, an international team of astronomers, including Dr. Prashant Pathak, Assistant Professor at the Department of Space, Planetary & Astronomical Sciences & Engineering (SPASE), IIT Kanpur, India, has identified a huge planet orbiting a star similar to our Sun in close proximity. Known as Epsilon Indi Ab, or Eps Ind Ab for short, this planet is categorized as a ‘super-Jupiter’ due to its mass, which exceeds Jupiter’s by at least six times, making it substantially larger than any planet in our solar system. Eps Ind Ab represents the first mature exoplanet, a planet outside our solar system, to be pinpointed using direct imaging techniques.

The findings detailing this discovery and the extensive research underpinning it have been published in Nature.

The image summarises the observations with JWST/MIRI that led to the rediscovery of Eps Ind Ab. The inserts show cropped versions of the MIRI images obtained at mid-infrared wavelengths 10.65 (left) and 15.55 micrometres (right), which depict the area around the star Eps Ind A, whose position is indicated by star symbols. A coronagraph blocks the light from the star that would outshine both images. Instead, a new object becomes visible to the top left. This source is the exoplanet Eps Ind Ab. The background was obtained from the AllWISE sky survey. Credit: T. Müller (MPIA/HdA).

Using the James Webb Space Telescope’s (JWST) Mid-InfraRed Instrument (MIRI), an international team of astronomers has successfully captured direct images of a newly discovered exoplanet orbiting the K5V-type star Epsilon Indi A, also known as HD 209100 or HIP 108870. This achievement marks a significant milestone in space exploration by directly observing a nearby mature exoplanet. Unlike indirect methods that rely on gravitational effects or starlight dimming, direct imaging allows astronomers to visually study the exoplanet itself. The breakthrough underscores JWST’s exceptional capabilities, combining high sensitivity, infrared technology, and advanced imaging techniques. These advancements are pivotal for future discoveries and deepen our understanding of distant worlds.

Located 12 light-years away, the newly found planet is notably cold, with a temperature around -1°C (30°F). Its orbit is vast, spanning a distance 28 times greater than that between Earth and the Sun.

“We were excited when we realised we had imaged this new planet,” said Elisabeth Matthews, a researcher at the Max Planck Institute for Astronomy in Heidelberg, Germany and the lead author of the research article. “To our surprise, the bright spot that appeared in our MIRI images did not match the position we were expecting for the planet”, Matthews points out. “Previous studies had correctly identified a planet in this system but underestimated mass and orbital separation”. With the help of the JWST, the team was able to set the record straight.

“This discovery is a major milestone in exoplanet research and sets the stage for future discoveries, bringing us one step closer to uncovering the mysteries of planetary systems beyond our own,” said Prof. Manindra Agrawal, Director, IIT Kanpur. “Being able to directly image a planet close to us provides an unprecedented opportunity for in-depth study. Dr. Prashant Pathak’s work in collaboration with international experts highlights the global contributions of IIT Kanpur in advancing our understanding of space.”

Dr. Prashant Pathak, Assistant Professor, Dept. of Space, Planetary & Astronomical Sciences & Engineering (SPASE), IIT Kanpur and a key member of the research team, explained, “This discovery is exciting because it gives us a chance to learn more about planets that are very different from our own. The planet’s atmosphere appears to have an unusual composition that indicates a high metal content and a different carbon-to-oxygen ratio than we see on our own solar system planets. This opens up fascinating questions about its formation and evolution. By studying Eps Ind Ab and other nearby exoplanets, we hope to gain a deeper understanding of planetary formation, atmospheric composition, and the potential for life beyond our solar system.”

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Space & Physics

MIT unveils an ultra-efficient 5G receiver that may supercharge future smart devices

A key innovation lies in the chip’s clever use of a phenomenon called the Miller effect, which allows small capacitors to perform like larger ones

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Image credit: Mohamed Hassan from Pixabay

A team of MIT researchers has developed a groundbreaking wireless receiver that could transform the future of Internet of Things (IoT) devices by dramatically improving energy efficiency and resilience to signal interference.

Designed for use in compact, battery-powered smart gadgets—like health monitors, environmental sensors, and industrial trackers—the new chip consumes less than a milliwatt of power and is roughly 30 times more resistant to certain types of interference than conventional receivers.

“This receiver could help expand the capabilities of IoT gadgets,” said Soroush Araei, an electrical engineering graduate student at MIT and lead author of the study, in a media statement. “Devices could become smaller, last longer on a battery, and work more reliably in crowded wireless environments like factory floors or smart cities.”

The chip, recently unveiled at the IEEE Radio Frequency Integrated Circuits Symposium, stands out for its novel use of passive filtering and ultra-small capacitors controlled by tiny switches. These switches require far less power than those typically found in existing IoT receivers.

A key innovation lies in the chip’s clever use of a phenomenon called the Miller effect, which allows small capacitors to perform like larger ones. This means the receiver achieves necessary filtering without relying on bulky components, keeping the circuit size under 0.05 square millimeters.

Credit: Courtesy of the researchers/MIT News

Traditional IoT receivers rely on fixed-frequency filters to block interference, but next-generation 5G-compatible devices need to operate across wider frequency ranges. The MIT design meets this demand using an innovative on-chip switch-capacitor network that blocks unwanted harmonic interference early in the signal chain—before it gets amplified and digitized.

Another critical breakthrough is a technique called bootstrap clocking, which ensures the miniature switches operate correctly even at a low power supply of just 0.6 volts. This helps maintain reliability without adding complex circuitry or draining battery life.

The chip’s minimalist design—using fewer and smaller components—also reduces signal leakage and manufacturing costs, making it well-suited for mass production.

Looking ahead, the MIT team is exploring ways to run the receiver without any dedicated power source—possibly by harvesting ambient energy from nearby Wi-Fi or Bluetooth signals.

The research was conducted by Araei alongside Mohammad Barzgari, Haibo Yang, and senior author Professor Negar Reiskarimian of MIT’s Microsystems Technology Laboratories.

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Society

Ahmedabad Plane Crash: The Science Behind Aircraft Take-Off -Understanding the Physics of Flight

Take-off is one of the most critical phases of flight, relying on the precise orchestration of aerodynamics, propulsion, and control systems. Here’s how it works:

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On June 12, 2025, a tragic aviation accident struck Ahmedabad, India when a regional passenger aircraft, Air India flight A1-171, crashed during take-off at Sardar Vallabhbhai Patel International Airport. According to preliminary reports, the incident resulted in over 200 confirmed casualties, including both passengers and crew members, and several others are critically injured. The aviation community and scientific world now turn their eyes not just toward the cause but also toward understanding the complex science behind what should have been a routine take-off.

How Do Aircraft Take Off?

Take-off is one of the most critical phases of flight, relying on the precise orchestration of aerodynamics, propulsion, and control systems. Here’s how it works:

1. Lift and Thrust

To leave the ground, an aircraft must generate lift, a force that counters gravity. This is achieved through the unique shape of the wing, called an airfoil, which creates a pressure difference — higher pressure under the wing and lower pressure above — according to Bernoulli’s Principle and Newton’s Third Law.

Simultaneously, engines provide thrust, propelling the aircraft forward. Most commercial jets use turbofan engines, which accelerate air through turbines to generate power.

2. Critical Speeds

Before takeoff, pilots calculate critical speeds:

  • V1 (Decision Speed): The last moment a takeoff can be safely aborted.
  • Vr (Rotation Speed): The speed at which the pilot begins to lift the nose.
  • V2 (Takeoff Safety Speed): The speed needed to climb safely even if one engine fails.

If anything disrupts this process — like bird strikes, engine failure, or runway obstructions — the results can be catastrophic.

Environmental and Mechanical Challenges

Factors like wind shear, runway surface condition, mechanical integrity, or pilot error can interfere with safe take-off. Investigators will be analyzing these very aspects in the Ahmedabad case.

The Bigger Picture

Take-off accounts for a small fraction of total flight time but is disproportionately associated with accidents — approximately 14% of all aviation accidents occur during take-off or initial climb.

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Space & Physics

MIT claims breakthrough in simulating physics of squishy, elastic materials

In a series of experiments, the new solver demonstrated its ability to simulate a diverse array of elastic behaviors, ranging from bouncing geometric shapes to soft, squishy characters

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Image credit: Courtesy of researchers

Researchers at MIT claim to have unveiled a novel physics-based simulation method that significantly improves stability and accuracy when modeling elastic materials — a key development for industries spanning animation, engineering, and digital fabrication.

In a series of experiments, the new solver demonstrated its ability to simulate a diverse array of elastic behaviors, ranging from bouncing geometric shapes to soft, squishy characters. Crucially, it maintained important physical properties and remained stable over long periods of time — an area where many existing methods falter.

Other simulation techniques frequently struggled in tests: some became unstable and caused erratic behavior, while others introduced excessive damping that distorted the motion. In contrast, the new method preserved elasticity without compromising reliability.

“Because our method demonstrates more stability, it can give animators more reliability and confidence when simulating anything elastic, whether it’s something from the real world or even something completely imaginary,” Leticia Mattos Da Silva, a graduate student at MIT’s Department of Electrical Engineering and Computer Science, said in a media statement.

Their study, though not yet peer-reviewed or published, will be presented at the August proceedings of the SIGGRAPH conference in Vancouver, Canada.

While the solver does not prioritize speed as aggressively as some tools, it avoids the accuracy and robustness trade-offs often associated with faster methods. It also sidesteps the complexity of nonlinear solvers, which are commonly used in physics-based approaches but are often sensitive and prone to failure.

Looking ahead, the research team aims to reduce computational costs and broaden the solver’s applications. One promising direction is in engineering and fabrication, where accurate elastic simulations could enhance the design of real-world products such as garments, medical devices, and toys.

“We were able to revive an old class of integrators in our work. My guess is there are other examples where researchers can revisit a problem to find a hidden convexity structure that could offer a lot of advantages,” Mattos Da Silva added.

The study opens new possibilities not only for digital content creation but also for practical design fields that rely on predictive simulations of flexible materials.

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