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Uranus, the seventh planet from the Sun, is usually known as a frozen “ice giant.” But in July 2025 astronomers announced a big surprise: Uranus is actually emitting more heat than it receives from sunlight. Decades of data and new models show Uranus emits about 12% more internal heat than it gets from the Sun. This contradicts measurements from NASA’s Voyager 2 flyby in 1986, which had found almost no internal warmth. The finding suggests Uranus is still cooling off from its formation. For scientists, this warm surprise has revived interest in exploring the distant world. An internal heat source could help explain Uranus’s tilt. Internal heat is really key to understanding Uranus’s mysteries.

Surprising Internal Warmth

According to the study, published in the journal Geophysical Research Letters, scientists used computer models and archival telescope and spacecraft data to reanalyze Uranus’s energy budget. They found the distant planet emits noticeably more heat from inside than expected. The team concludes this heat likely comes from leftover energy deep inside Uranus’s core, slowly escaping into space. One reason this wasn’t seen before could be timing: a solar storm during Voyager’s flyby might have masked some heat. The new results hint that Uranus’s deep interior could be arranged differently than scientists assumed.

Renewed Mission Push

Almost everything we know about Uranus comes from that one Voyager 2 flyby, and no spacecraft has ever orbited Uranus; dedicated missions have only been proposals. For decades, scientists have argued for a mission to Uranus, and in fact the latest decadal survey named it a flagship mission idea. Such a mission could send an atmospheric probe into Uranus and then spend years circling the planet, measuring its composition, winds and magnetic field, and studying its faint rings and many moons.
Scientists note that ice giants are among the most common planets in other star systems. The warmth finding adds urgency: one researcher said it “strengthens the case for a mission to Uranus”, and others note it could help NASA plan an expedition to this distant ice giant.

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Century-Old Thermoelectric Effect Finally Observed – Transverse Thomson Effect Discovery Explained

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Century-Old Thermoelectric Effect Finally Observed – Transverse Thomson Effect Discovery Explained

In a recent paper published online, researchers have reported the transverse Thomson effect’s first experimental observation. It is a key thermoelectric phenomenon that has made scientists avoid it since it was predicted almost a century ago. Physicists have observed thermoelectric effects to understand the connection between heat and electricity on the basis of the Peltier, Seebeck and Thomson effects studied during the 1800s. The Thomson effect includes heating or cooling during the flow of electric current and a temperature gradient towards the same direction through a conductor.

How Scientists Isolated the Elusive Transverse Thomson Effect

As per phys org, Scientists found the transverse version of the effect that exists when the electric current, magnetic field and temperature gradient interact. A team led by Atsushi Takahagi experimentally demonstrated the higher order effect of thermoelectricity. The researchers isolated the signals by applying extracted temperature modulations that oscillates at the same frequency and applying periodic electric currents. Through two sets of measurements, the team successfully isolated the Thomson effect from overlapping signals.

The Role of Bismuth Antimony Alloy in Demonstrating the Effect

For their experiments, the team picked a bismuth antimony alloy, which shows a strong Nernst effect at room temperature. This effect occurs when the temperature gradient and magnetic field are applied orthogonally and generate an electric field perpendicularly. The Ettingshausen effect, on the reverse, creates a temperature gradient from the magnetic and electric field. The researchers found that the transverse Thomson effect is dependent on the temperature derivative of the Nernst coefficient itself, which is different from the conventional one.

Switching Between Heating and Cooling Using Magnetic Fields

A surprising finding was the ability to switch between the cooling and heating simply by changing the direction of the magnetic field. This interplay led to the reversal sign in the effect at the magnetic field strengths, and was confirmed through experiments and numerical simulations.

New Possibilities for Thermal Management and Future Research Directions

The discovery made its way for these different thermal management applications, especially where controlled heat is required. The future research might focus on finding new materials where both the gradients of the transverse Thomson coefficient amplify each other and do not cancel out, which signals the high performance of thermoelectric materials.

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Young Exoplanet Spotted Shedding Atmosphere Under Stellar Radiation

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Young Exoplanet Spotted Shedding Atmosphere Under Stellar Radiation

NASA’s Chandra X-ray Observatory, together with data from the Hubble Space Telescope, has revealed a “baby” exoplanet rapidly losing its atmosphere. The planet, named TOI 1227 b, orbits a faint red dwarf star and is only about 8 million years old. Powerful X-ray blasts from the star are stripping away the planet’s thick gas envelope. Models indicate TOI 1227 b is shedding an amount of gas equal to Earth’s entire atmosphere every ~200 years. The team notes the planet’s atmosphere “simply cannot withstand the high X-ray dose it’s receiving”. This finding offers a rare, real-time look at atmospheric erosion, showing how a young world can be dramatically reshaped by its star early on.

Observations of an Eroding Planet

According to the study, astronomers used Chandra’s X-ray data (and earlier Hubble observations of the planet’s transit) to study TOI 1227 b. This Jupiter-sized world orbits extremely close to its star – much closer than Mercury is to the Sun – and is about a thousand times younger than Earth. The host star is unleashing intense X-rays on the planet.

In artist’s illustrations and models, this appears as a blue tail of gas streaming off TOI 1227 b as its atmosphere is ripped away. Computer simulations show the radiation will “rapidly” strip off the gas. Remarkably, the planet is already losing the equivalent of an Earth’s atmosphere about every 200 years. If conditions persist, TOI 1227 b could ultimately shrink from a gas giant to “a small, barren world”.

Implications for Planetary Evolution

This discovery highlights the key role of stellar radiation in young planetary systems. High-energy X-rays (and ultraviolet light) from an active young star can heat and blow away a planet’s atmosphere. As co-author of the study Joel Kastner explains, understanding exoplanets requires that scientists “account for high-energy radiation like X-rays”. In this case, the star’s output acts like “a hair dryer on an ice cube,” gradually blowing the gas off the planet. Such photoevaporation is thought to explain why many intermediate-size exoplanets end up smaller or stripped to their cores.

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China Launches Advanced Spacesuits and 7.2 Tons of Supplies to Tiangong Space Station

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China Launches Advanced Spacesuits and 7.2 Tons of Supplies to Tiangong Space Station

China has launched a new resupply mission to its module and the astronauts and space station to which it is connected in orbit above the Earth, sending food, fuel, scientific gear, and updated spacesuits. The Long March 7 rocket, taking it aloft, took off from the Wenchang Satellite Launch Centre on Hainan Island at 5:34 p.m. EDT July 14 (5:34 a.m. China Standard Time July 15), carrying the Tianzhou 9 cargo spacecraft. The vehicle is carrying about 7.2 tons (6.5 metric tons) of supplies to support the three taikonauts currently on the station for the ongoing Shenzhou 20 crewed mission.

China Enhances Tiangong Station with New Spacesuits and Fitness Gear in Tianzhou 9 Mission

As per a report by China Global Television Network (CGTN), the cargo includes two new spacesuits that should last three to four years and allow for up to 20 spacewalks, rather than 15 for the old generation. Also along for the ride is a core muscle training device meant to boost the station’s gym for astronauts with better tools to fight muscle atrophy in microgravity conditions. The report emphasised that these improvements are key to ensuring crew health during long-duration missions.

Tianzhou 9 marks the ninth cargo launch China has executed for its human spaceflight program since 2017. The first such spacecraft docked with Tiangong 2, a prototype lab that tested critical technologies ahead of the current space station’s development. Subsequent missions have supplied either the fully assembled Tiangong station or its core module, Tianhe, which was launched in April 2021.

Launched in October 2022, the Tiangong space station, a 3-module space station, is a significant step in China’s independent space ambitions. And while its mass is but 20 percent of what the International Space Station allotted to its construction, Chinese officials have signalled plans for growing the outpost, possibly boosting its stature in low Earth orbit activities worldwide.

Cargo deliveries like Tianzhou 9 are essential to keeping Tiangong in business and the Chinese space program’s long-term human presence in space running. Thanks to improvements in equipment, preparations, and life support, the nation looks prepared to further cement its place in orbital science and discovery.

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