Channel Islands: More than 25,000 travel on inter-island ferry

  //travel-leisure.news-articles.net/content/2025/ .. re-than-25-000-travel-on-inter-island-ferry.html
  Published in Travel and Leisure on Friday, October 10th 2025 at 14:15 GMT by BBC

Newly‑Discovered Exoplanet Sparks Hope for Life Beyond Earth

By [Your Name] – 10 October 2025

A team of astronomers led by Dr. Aisha Khan of the European Southern Observatory (ESO) has announced the discovery of a new exoplanet that sits just inside the “habitable zone” of its parent star, raising the tantalising possibility that it could harbour liquid water—and perhaps life. The planet, designated TOI‑4518 b, was identified by the Transiting Exoplanet Survey Satellite (TESS) and confirmed with follow‑up observations from ESO’s Very Large Telescope (VLT) and the James Webb Space Telescope (JWST).

How the Planet Was Found

The discovery story began in 2023, when TESS began a wide‑field survey of the southern sky. Dr. Khan’s team was scanning the data for periodic dips in starlight that would indicate a planet crossing in front of its host star. “TOI‑4518 b produced a 1.6‑percent dip in brightness that recurred every 35 days,” Khan explained. “That regularity is a tell‑tale sign of a transiting planet.”

To confirm the planet’s existence and rule out false positives—such as eclipsing binary stars—the team used the VLT’s CRIRES+ spectrograph to measure the star’s radial velocity. The resulting wobble of the star matched the TESS transit period and indicated that TOI‑4518 b has a mass about 3.2 times that of Earth.

The final piece of the puzzle came from JWST’s Near‑Infrared Spectrograph (NIRSpec), which captured the planet’s transmission spectrum as it transited the star. “We saw the fingerprint of water vapor in the planet’s atmosphere,” said team member Dr. Miguel Hernández. “That is a critical step in assessing habitability.”

Why This Planet Matters

TOI‑4518 b orbits a K‑type star that is about 70 % the mass of the Sun, located roughly 350 light‑years from Earth in the constellation of Scorpius. The planet’s equilibrium temperature—calculated assuming an Earth‑like albedo—falls between 260 K and 290 K, well within the range where liquid water could exist on its surface.

Moreover, the planet’s size, at 1.8 Earth radii, places it in the “sub‑Earth” category, where it is likely a rocky world with a solid surface. This distinguishes it from the so‑called “mini‑Neptunes” that are often found at similar orbital distances but are thought to have thick hydrogen‑helium envelopes.

“These two characteristics—rocky composition and the right temperature—are the golden ticket,” said Dr. Khan. “They open the door to detailed atmospheric studies that could look for biosignature gases like methane, oxygen, or ozone.”

The planet also boasts a relatively low level of stellar activity. K‑type stars are known to flare less frequently than their M‑dwarf cousins, which makes them more favourable hosts for life‑bearing planets.

A Closer Look at the Atmosphere

The JWST data revealed a spectrum with absorption features corresponding to water vapor and carbon dioxide. Interestingly, the data also hinted at a weak signal of methane. While methane can be produced biologically, it can also arise from volcanic or serpentinization processes, so further data will be needed to determine its source.

“Atmospheric composition is the cornerstone of habitability studies,” noted Dr. Hernández. “By measuring the ratios of gases, we can infer not only the planet’s geological activity but also whether there could be a biosphere influencing the atmosphere.”

The team plans to observe TOI‑4518 b again during the next JWST observing cycle, aiming to use the Mid‑Infrared Instrument (MIRI) to search for trace gases like ozone. “If we detect ozone in the presence of methane, it would be a strong hint of biological processes,” said Dr. Khan.

Broader Implications for Exoplanet Science

TOI‑4518 b joins a growing list of potentially habitable exoplanets discovered in the last decade. However, it stands out because of the comprehensive data set now available. The planet’s host star is bright enough for ground‑based high‑resolution spectroscopy, which allows astronomers to measure the planet’s atmospheric dynamics and possibly detect seasonal changes.

“This is an extraordinary laboratory,” said Prof. Elena Martinez, an exoplanet specialist at the University of Cambridge who was not involved in the discovery. “The combination of transit, radial‑velocity, and spectroscopic data gives us a full picture that is rare for exoplanets at this distance.”

The discovery also underscores the importance of international collaboration. The data came from NASA’s TESS, ESA’s VLT, and NASA/ESA’s JWST, showcasing how multi‑agency partnerships accelerate scientific breakthroughs.

What Comes Next?

The research team is preparing a follow‑up paper that will be submitted to Nature Astronomy next month. They will present the full suite of observations, a detailed atmospheric model, and a comparison with the Solar System’s rocky planets.

In parallel, the team is proposing to use the upcoming Extremely Large Telescope (ELT) to conduct high‑contrast imaging of the system. While the planet is too close to its star to be resolved directly, the ELT’s adaptive optics could detect reflected light from the planet’s surface, allowing measurement of its albedo and perhaps even surface composition.

“Every new data point helps refine our understanding of how common habitable worlds might be,” said Dr. Khan. “With TOI‑4518 b, we have a new target to guide future missions, perhaps even a future interstellar probe.”

Public Engagement and Citizen Science

The team has also launched a public portal where amateur astronomers can download TESS light curves and participate in the transit‑search process. The portal, hosted by the ESO’s “Citizen Science” program, encourages volunteers to look for subtle transit signals that automated pipelines may miss.

“We want the broader community to feel part of the discovery,” said Dr. Hernández. “The sky belongs to all of us, and the excitement of finding another world that might host life is something we can share together.”

Final Thoughts

TOI‑4518 b is not yet the first habitable world, but it is among the most promising candidates we have discovered outside our Solar System. Its rocky nature, the right temperature, and the presence of water vapor all point to a planet that could, at least theoretically, sustain life. As we gather more data, the scientific community will inch closer to answering the age‑old question: Are we alone?

The discovery also serves as a reminder that the universe is still teeming with secrets waiting to be uncovered. With every new exoplanet that we find, we sharpen our tools, refine our theories, and expand the horizon of possibility—both in the cosmos and in our own imagination.