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Astronomers have analysed the atmosphere of WASP-166 b, a hot super-Neptune exoplanet, revealing the presence of water and carbon dioxide. Using data from the James Webb Space Telescope (JWST), the observations also detected ammonia in smaller quantities. WASP-166 b is situated approximately 368 light-years away and is about seven times larger and 32 times heavier than Earth. The planet, orbiting its host star every 5.44 days at a distance of 0.067 AU, has an estimated equilibrium temperature of 1,270 K, placing it within the hot Neptune desert.

Findings from JWST Observations

As reported by phys.org, the JWST employed its Near Infrared Imager and Slitless Spectrograph (NIRISS) and Near Infrared Camera (NIRCam) to study WASP-166 b’s atmosphere. These observations highlighted water and carbon dioxide as dominant elements in the spectrum, alongside weak traces of ammonia and cloud deck pressure. Helium and hydrogen, in a primordial solar ratio, are believed to compose the remaining atmosphere. Searches for compounds like carbon monoxide yielded no significant results.

Characteristics of WASP-166 and Its Planet

WASP-166, the host star of this exoplanet, belongs to the F9V spectral type and is approximately 20 percent larger and more massive than the sun. It is 2.1 billion years old, with a surface temperature of 6,050 K and a metallicity of 0.19 dex. The planetary carbon-to-oxygen ratio of WASP-166 b was calculated to be 0.282, significantly lower than both the host star (0.41) and the sun (0.55). Additionally, the planet’s high atmospheric metallicity of 1.57 was reported.

Explanations for Atmospheric Composition

It was suggested that the atmospheric composition could be linked to planetesimal accretion, core erosion, or photoevaporation. Such findings contribute to understanding planetary formation and evolution, particularly within regions like the hot Neptune desert. The study provides insights into the diversity of exoplanetary systems and their unique characteristics.

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Amateur Astronomer Discovers Unexpected Composition of Jupiter’s Clouds

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Amateur Astronomer Discovers Unexpected Composition of Jupiter’s Clouds

Jupiter’s atmospheric composition has been called into question through observations made using an old technique by an amateur astronomer, Steve Hill. The findings have indicated that the planet’s iconic swirling clouds may not be composed of ammonia ice, as previously assumed. This revelation stems from data collected with commercial telescopes and spectral filters, presenting new perspectives on the gas giant’s atmospheric dynamics and chemistry. The observations have sparked further investigation into the structure of Jupiter‘s cloud layers.

Findings from Observational Studies

According to research published in Earth and Space Science, Hill applied a method known as band-depth analysis. This technique measures light absorption at specific wavelengths to map the abundance of gases like ammonia and methane in Jupiter’s atmosphere. As reported by space.com, the data revealed that reflective cloud layers are located at pressure levels of 2-3 bar, far deeper than where ammonia ice was expected to condense at 0.7 bar.

Patrick Irwin, a planetary physicist at the University of Oxford, reviewed Hill’s results and confirmed their accuracy through comparisons with data from instruments such as NASA’s Juno spacecraft and ESO’s Very Large Telescope (VLT). He noted to space.com that the main reflection appears to stem from ammonium hydrosulfide clouds or photochemical products, rather than pure ammonia ice.

Implications and Future Research

Reports indicate that these findings underline the role of photochemistry in shaping Jupiter’s atmosphere, where ammonia is often destroyed faster than it can rise to the upper layers. Similar processes have been observed on Saturn, where cloud layers are also deeper than predicted. Researchers aim to refine models by integrating additional data from the VLT, Juno, and other observatories to better understand ammonia’s vertical distribution.

Hill’s approach demonstrates the potential of collaborative efforts between amateur and professional astronomers. These findings not only challenge existing models but also open new pathways for studying atmospheric dynamics on gas giants.

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Blue Origin Delays New Glenn Launch to January 12 Due to Adverse Weather in Atlantic

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Blue Origin Delays New Glenn Launch to January 12 Due to Adverse Weather in Atlantic

The launch of Blue Origin’s highly anticipated New Glenn rocket has been delayed due to adverse weather conditions. Initially planned for Friday, January 10, the liftoff was rescheduled to Sunday, January 12, at 1:00 a.m. EST (0600 GMT). This decision was taken because rough seas in the Atlantic Ocean could jeopardise the landing of the rocket’s reusable first stage. The launch will proceed from the Cape Canaveral Space Force Station in Florida, with the same three-hour launch window.

Weather Challenges Force Delay

According to a statement by Blue Origin, as reported by Space.com, the high sea state in the Atlantic presented risks to the landing operation of the rocket booster, which is designed to return to Earth and land on a barge named Jacklyn. Named after Jeff Bezos’ mother, the barge is critical to the company’s plans to achieve reusability. Blue Origin acknowledged the ambitious nature of attempting a first-time booster landing, emphasising their determination to succeed despite the challenges.

Technical Details of New Glenn

Standing at an impressive height of 320 feet (98 meters), the New Glenn rocket marks Blue Origin’s entry into orbital-class missions. It is equipped with a reusable first stage that is intended to endure at least 25 flights, reducing the cost of space missions. This design mirrors the reusable model successfully employed by rival company SpaceX, which regularly recovers its Falcon 9 and Falcon Heavy boosters for reuse.

Future Missions and Contracts

Blue Origin has already secured several contracts for its New Glenn rocket. Among them are NASA’s ESCAPADE mission to Mars and the deployment of Amazon’s Kuiper internet satellites. If the launch does not proceed on Sunday, notices from the Federal Aviation Administration indicate that the company may attempt additional launches through January 16.

The mission represents a significant step for Blue Origin in advancing reusable space technology, with the industry closely monitoring the outcome of its maiden voyage.

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New Link Found Between Ferroelectric Domain Walls and Superconductivity in 2D Materials

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New Link Found Between Ferroelectric Domain Walls and Superconductivity in 2D Materials

Scientists have discovered a unique link between ferroelectric domain walls and superconductivity in two-dimensional van der Waals materials. This breakthrough, credited to research by Gaurav Chaudhary from the University of Cambridge and Ivar Martin from Argonne National Laboratory, sheds light on how specific structural features in these materials enable strong electron interactions. The findings are expected to pave the way for new superconducting devices and innovative applications in the field of condensed matter physics.

Sliding Ferroelectricity and Polarisation Reversal

According to reports by phys.org, sliding ferroelectricity in certain 2D van der Waals materials, including boron nitride and transition metal dichalcogenides (TMDs), facilitates polarisation reversal under moderate electric fields. This phenomenon allows for large-scale manipulation of layer stacking, significantly impacting the material’s electronic properties. Researchers noted that domain walls—boundaries separating regions with differing orientations of ferroelectric polarisation—exhibit unique characteristics that enhance electron-phonon coupling.

Superconductivity Observed at Domain Walls

The study revealed that in materials like molybdenum ditelluride (MoTe₂), superconductivity is transiently enhanced near ferroelectric reversal transitions. This enhancement occurs within hysteresis loops where domains of varying polarisation coexist. The dynamic fluctuations in domain walls were identified as the driving mechanism for the pairing interactions required for superconductivity. It was highlighted that these conditions are exclusive to 2D TMDs, which support interlayer ferroelectricity while remaining conductive within their planes.

Future Research and Applications

Chaudhary and Martin indicated to phys.org that their findings hold potential for developing highly controllable superconducting devices. Efforts are underway to explore the systematic design of new superconductors by layering polar materials and leveraging domain wall networks in moiré systems. They also emphasised the need for further investigations to validate their theoretical models using advanced microscopic simulations.
The study has generated interest among scientists aiming to uncover unconventional mechanisms of superconductivity, marking an important step forward in understanding and utilising the properties of 2D materials.

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