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One-third of the planets orbiting the most common stars across the Milky Way galaxy may hold onto liquid water and possibly harbour life, according to a study based on latest telescope data.

The most common stars in our galaxy are considerably smaller and cooler, sporting just half the mass of the Sun at most. Billions of planets orbit these common dwarf stars.

The analysis, published in the journal Proceedings of the National Academy of Sciences, shows that two-thirds of the planets around these ubiquitous small stars could be roasted by tidal extremes, sterilising them.

However, that leaves one-third of the planets—hundreds of millions across the galaxy—that could be in a goldilocks orbit close enough, and gentle enough, to be possibly habitable.

“I think this result is really important for the next decade of exoplanet research, because eyes are shifting towards this population of stars,” said Sheila Sagear, a doctoral student at the University of Florida (UF) in the US.

“These stars are excellent targets to look for small planets in an orbit where it’s conceivable that water might be liquid and therefore the planet might be habitable,” Sagear said in a statement.

Sagear and UF astronomy professor Sarah Ballard measured the eccentricity of a sample of more than 150 planets around M dwarf stars, which are about the size of Jupiter.

The more oval shaped an orbit, the more eccentric it is. If a planet orbits close enough to its star, at about the distance that Mercury orbits the Sun, an eccentric orbit can subject it to a process known as tidal heating.

As the planet is stretched and deformed by changing gravitational forces on its irregular orbit, friction heats it up. At the extreme end, this could bake the planet, removing all chance for liquid water.

“It’s only for these small stars that the zone of habitability is close enough for these tidal forces to be relevant,” Ballard said.

The researchers used data from NASA’s Kepler telescope, which captures information about exoplanets as they move in front of their host stars.

To measure the planets’ orbits, they focused especially on how long the planets took to move across the face of the stars. Their study also relied on new data from the Gaia telescope, which has measured the distance to billions of stars in the galaxy.

“The distance is really the key piece of information we were missing before that allows us to do this analysis now,” Sagear said.

The team found that stars with multiple planets were the most likely to have the kind of circular orbits that allow them to retain liquid water.

Stars with only one planet were the most likely to see tidal extremes that would sterilise the surface, according to the researchers.

Since one-third of the planets in this small sample had gentle enough orbits to potentially host liquid water, that likely means that the Milky Way has hundreds of millions of promising targets to probe for signs of life outside our solar system, they added.


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Astronaut Captures Rare ‘Gigantic Jet’ Lightning Extending 50 Miles Above Earth

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Astronaut Captures Rare ‘Gigantic Jet’ Lightning Extending 50 Miles Above Earth

A rare ‘gigantic jet’ of lightning has been photographed from space, extending nearly 50 miles above the U.S. coastline. The image was taken by an astronaut aboard the International Space Station (ISS) on November 19, 2024, but was not immediately shared by space agencies. The phenomenon was later discovered on NASA’s Gateway to Astronaut Photography of Earth website by photographer Frankie Lucena, who specialises in capturing rare lightning events. The images were subsequently highlighted by Spaceweather.com on February 26.

Jet Likely Originated Over Louisiana

According to Spaceweather.com, the ISS was positioned over the Gulf of Mexico at the time of the capture, suggesting that the lightning jet likely originated from a thunderstorm near New Orleans. Due to dense cloud cover in the image, the precise location could not be determined. Four images of lightning were identified in the astronaut’s photography sequence, but only one captured the distinct upward-shooting jet.

Understanding Gigantic Jets

Gigantic jets are powerful electrical discharges that travel upward from thunderstorms when charge layers within the clouds become inverted. Unlike conventional lightning that strikes downward, these jets extend into the ionosphere, the atmospheric layer beginning around 50 miles above the Earth’s surface. As per Spaceweather.com, these jets emit a blue glow due to interactions with nitrogen in the upper atmosphere and last for less than a second.

Uncommon but Extremely Powerful

Reports indicate that while gigantic jets were first documented in 2001, scientists estimate that around 1,000 could occur annually, though most go undetected. The most powerful recorded jet was observed in May 2018 over Oklahoma, carrying nearly 60 times the energy of a typical lightning strike. These events often conclude with red branching tendrils, similar to lightning phenomena known as sprites, but classified as separate occurrences.

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Solar Storm to Trigger Northern Lights in US: Visibility, Timing & Impact



Infinix GT 30 Pro Key Features Surface Online; Tipped to Get Gaming Trigger Buttons

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Solar Storm to Trigger Northern Lights in US: Visibility, Timing & Impact

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Solar Storm to Trigger Northern Lights in US: Visibility, Timing & Impact

A solar storm is set to reach Earth tonight, with potential geomagnetic activity that could make the northern lights visible as far south as New York and Idaho. The event is the result of a coronal mass ejection (CME) from the Sun, which was recorded on March 1. The Space Weather Prediction Center (SWPC) of the National Oceanic and Atmospheric Administration (NOAA) has classified this as a G1-level geomagnetic storm, with a possibility of stronger G2 conditions. As a result, skywatchers in mid-latitudes may witness the aurora borealis in areas where the skies remain clear.

Geomagnetic Storm Forecast and Impact

According to NOAA’s Space Weather Prediction Center, the CME is expected to make contact with Earth’s magnetic field between March 4 and March 5. The intensity of the storm is predicted to peak between 7:00 p.m. EST and 10:00 p.m. EST on March 5. While a G1 storm is considered minor, space weather physicist Tamitha Skov has indicated that G2 storm conditions remain a possibility, increasing the chances of a more widespread auroral display.

Geomagnetic storms occur when charged particles from the Sun interact with Earth’s magnetosphere, potentially affecting satellite communications, power grids, and GPS accuracy. Experts have advised that radio operators, GPS users, and drone pilots may experience signal disruptions, especially during nighttime hours when such interference is more pronounced.

Visibility and Viewing Conditions

As per reports, aurora visibility will largely depend on atmospheric clarity and light pollution levels. NOAA’s storm classification system places G1 storms as minor, meaning that the northern lights will likely be seen closer to high-latitude regions. If G2 storm conditions occur, visibility could extend further south. Observers are advised to find dark locations away from city lights for the best viewing experience.

For real-time updates and forecasts, space weather monitoring agencies continue to track the storm’s progression.

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NASA Tests Advanced Infrared Technology to Improve Wildfire Monitoring

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NASA Tests Advanced Infrared Technology to Improve Wildfire Monitoring

Wildfires in California during January caused widespread destruction, affecting communities and ecosystems. To improve wildfire monitoring and response, NASA deployed a new scientific instrument capable of capturing high-resolution thermal infrared images. The Compact Fire Infrared Radiance Spectral Tracker (c-FIRST) was tested aboard NASA’s B200 King Air aircraft over fire-hit areas in Pacific Palisades and Altadena. The instrument, developed for satellite-based missions, was assessed for its ability to provide real-time data on active and smoldering fires. Scientists aim to use this technology to enhance understanding of wildfire behavior and improve mitigation strategies.

Enhanced Fire Detection and Data Collection

According to reports, the c-FIRST instrument was developed and is managed by NASA’s Jet Propulsion Laboratory (JPL), with support from NASA’s Earth Science Technology Office. The compact design allows it to be deployed on airborne platforms, simulating satellite missions while providing near-instantaneous observations. The system captures a wide range of fire characteristics, including temperature variations across large areas. Unlike previous infrared imaging systems, c-FIRST can detect extremely high temperatures exceeding 1,000 degrees Fahrenheit (550 degrees Celsius) with improved clarity.

In a statement, Sarath Gunapala, principal investigator for c-FIRST at NASA JPL, noted that current fire observation instruments do not fully capture fire attributes across the Earth system. He explained that limitations in past imaging technologies have resulted in gaps in data concerning wildfire frequency, size, and intensity.

Potential Benefits for Fire Management

As per sources, c-FIRST is expected to provide critical insights for firefighting agencies by identifying smoldering fires that could reignite under changing wind conditions. In a report, Gunapala stated that the instrument’s ability to distinguish such fires in near real-time could support more effective wildfire management efforts.

KC Sujan, operations engineer for the B200 King Air, told that the aircraft’s flight characteristics made it ideal for testing the instrument. With further evaluation, c-FIRST is expected to be integrated into future satellite missions, potentially improving global wildfire monitoring capabilities.

For details of the latest launches and news from Samsung, Xiaomi, Realme, OnePlus, Oppo and other companies at the Mobile World Congress in Barcelona, visit our MWC 2025 hub.

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