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The Sun, during its solar maximum phase in 2024, emitted over 50 X-class solar flares—the most powerful category of solar flares. These intense bursts of energy, capable of disrupting satellites and communications on Earth, marked a highly active year for solar phenomena. According to reports, these flares varied in magnitude and impact, with the strongest measured at X9.0 on October 3. Below is a countdown of the ten most notable solar flares recorded this year.

February 9 – X3.38

A solar flare rated X3.38 was observed near the southwestern edge of the Sun. According to researchers, the full intensity might have been obscured due to its position. The flare showcased a “coronal wave,” with solar material visibly displaced across the Sun’s surface.

February 22 – X6.37

This flare, while registering an impressive X6.37, lacked Earth-directed coronal mass ejections (CMEs) and had limited effects beyond its intense X-ray emissions. Data from NASA highlighted its scientific importance despite its minimal impact.

May 6 – X4.52

An eruption from Active Region AR 13663 in the northern hemisphere occurred early in May. This flare, documented by NASA’s Solar Dynamics Observatory, did not produce Earth-directed CMEs, though it highlighted the active state of the Sun during this period.

May 10 – X3.98

From Active Region AR 13664, this solar flare produced a strong Earth-directed CME. Reports indicated it was part of a series of events that caused a G5 geomagnetic storm, leading to widespread auroras visible at unusually low latitudes.

May 11 – X5.89

Another eruption from AR 13664 occurred just a day later. This flare, part of a chain of CMEs, contributed to the extreme geomagnetic activity documented during this period. Its position on the solar limb reduced its direct impact on Earth.

May 14 – X8.79

A confined flare from AR 13664 produced strong X-ray emissions without a major eruption. Despite its physical size, its intensity ranked among the highest of the year, as confirmed by ESA and NASA observations.

May 15 – X3.48

The final X-class flare from AR 13664 during its rotation was recorded on May 15. Observations revealed that its intensity was partly obscured as the active region moved out of Earth’s view. ESA reports noted continued activity from this region even when it was no longer visible from Earth.

September 14 – X4.54

A strong CME directed over the Sun’s eastern limb accompanied this flare. Observers noted pixel saturation in images, a common occurrence in high-energy flares of this magnitude.

October 1 – X7.10

This flare originated from Active Region AR 13842. Despite its size, it did not produce significant geomagnetic storms. Experts observed that smaller flares from this active region later contributed to strong auroras seen worldwide.

October 3 – X9.0

The largest solar flare of 2024, and one of the strongest in recent years, was recorded at X9.0. As per data from the Solar and Heliospheric Observatory, it unleashed energy nine times the X-class threshold, cementing its place as a standout event of Solar Cycle 25.

The Sun’s activity continues to be closely monitored as solar maximum extends into 2025.

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Algae-Grown Bioplastic Passes Mars Pressure Test, Boosting Hopes for Red Planet Habitats

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Algae-Grown Bioplastic Passes Mars Pressure Test, Boosting Hopes for Red Planet Habitats

In a major step forward for sustainable space travel, researchers have been able to successfully grow algae inside biodegradable bioplastic, which mimics the conditions of the extreme Martian environment. The experiment was intended to see how well materials made of polylactic acid could keep conditions habitable on Mars, where the surface pressure is less than 1 percent that of the Earth’s. It’s an important step toward the development of self-sustaining habitats for the human portion of the expeditionary force that require regenerative biological systems instead of expensive resupply missions from Earth.

Algae Thrive in Bioplastic Chambers Under Mars-Like Conditions, Paving Way for Space Habitats

As per a study published in Science Advances, a research team led by Robin Wordsworth of Harvard University demonstrated that the green algae Dunaliella tertiolecta could not only survive but perform photosynthesis inside 3D-printed chambers engineered to replicate Mars’s thin, carbon dioxide–rich atmosphere. The bioplastic chamber also protected the algae from ultraviolet radiation while allowing enough light for biological activity. Liquid water was stabilised using a pressure gradient within the chamber.

The researchers highlighted that bioplastics offer distinct advantages over traditional industrial

materials, which are difficult to recycle or transport in space. Since polylactic acid is derived from natural sources, it could potentially be manufactured or regenerated on-site using algae—establishing a self-sustaining loop. “If you have a habitat that is composed of bioplastic and it grows algae within it, that algae could produce more bioplastic,” Wordsworth noted in a statement.

This latest experiment builds on the team’s earlier work involving silica aerogels that replicated Earth’s greenhouse conditions. By combining algae-based bioplastic systems for material regeneration with aerogels for thermal and atmospheric control, the team sees a viable path forward to long-term extraterrestrial habitation. The chambers’ success under Mars-like conditions reinforces the possibility of using biologically sourced materials to support life beyond Earth.

In future experiments, those systems are to be tested in harsher vacuum conditions, eventually for the benefit of human spaceflight and with spinoff applications on Earth, said Wordsworth, who contends such technology can have spinoff benefits.

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NASA’s Twin TRACERS Satellites Will Monitor Space Weather to Shield Earth from Solar Storms

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NASA Tests Modular Satellite Tech to Cut Launch Costs and Speed Missions

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NASA Tests Modular Satellite Tech to Cut Launch Costs and Speed Missions

NASA is testing new scalable satellite technology to integrate and launch scientific sensors faster and at lower cost. NASA’s Athena EPIC (Economical Payload Integration Cost) mission uses a compact, modular spacecraft platform that “shares resources among the payloads onboard” so each instrument doesn’t need its own control system. By offloading routine functions to the bus, this architecture promises “lower costs to taxpayers and a quicker path to launch”. Langley leads the project, which will fly as a SpaceX rideshare in mid-2025 to test the concept in orbit. It could expedite deployment of climate and weather sensors and accelerate future missions.

Scalable Satellite Platforms and Demonstration Missions

According to official site, NASA and industry partners are developing modular small satellite platforms. The Athena EPIC spacecraft is built from eight interlocking Hyper-Integrated Satlet (HISat) modules that form a “SensorCraft” bus, simplifying integration of multiple instruments. In parallel, NASA’s Pathfinder Technology Demonstrator (PTD) series uses a standard six-unit (6U) CubeSat bus (by Terran Orbital) that can be reconfigured quickly. The PTD-3 mission, launched in 2022, carried MIT Lincoln Laboratory’s TBIRD optical-communications payload and achieved a record 200 gigabits-per-second laser downlink from orbit.

Commercial partners are involved as well: Blue Canyon Technologies built the two CubeSats for NASA’s CubeSat Laser Infrared Crosslink (CLICK) mission, and will supply four for the forthcoming Starling formation-flying demo. These standardized buses and partnerships speed integration and testing of new satellite systems.

Faster Deployments, Lower Costs, and Scientific Gains

These scalable satellite buses promise to cut mission costs and cycle times. Instead of the billion-dollar platforms of old, the new “SensorCraft” design can slash costs to the single-digit millions per mission. Smaller satellites are cheaper to build and easier to replace if failures occur. Moreover, by reusing existing parts, teams can accelerate development – for example, Athena’s optical sensor was assembled from spare components of NASA’s CERES climate-observation satellites. NASA officials note that, “as satellites become smaller, a less traditional, more efficient path to launch is needed” to maximize science return.

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NASA’s Twin TRACERS Satellites Will Monitor Space Weather to Shield Earth from Solar Storms

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NASA’s Twin TRACERS Satellites Will Monitor Space Weather to Shield Earth from Solar Storms

Two NASA satellites are scheduled to be launched into low-Earth orbit in a mission designed to do nothing less than study magnetic storms that imperil the Earth’s atmosphere, communication, and orbital systems. Travelling together in sun-synchronous orbit, the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) will keep watch over Earth’s polar cusps — a pair of funnel-shaped regions in Earth’s magnetosphere where solar particles and energy flow in. By observing these regions, TRACERS will continue to learn how magnetic reconnection works throughout space, powering the giant explosions on the sun as well as the solar wind that spreads throughout the solar system, leading to space weather.

NASA’s $170M TRACERS Mission to Track Solar Wind and Shield Earth from Space Weather Threats

As per NASA’s briefing, TRACERS will explore how solar wind triggers disruptions in Earth’s magnetic field, helping researchers better predict when and where such activity might occur. The spacecraft will fly closely behind one another, allowing for nearly real-time comparison of plasma and magnetic conditions—an improvement over previous single-satellite studies. Joe Westlake, NASA’s Heliophysics Division Director, stated the mission will help protect GPS, power grids, and astronauts by enabling earlier forecasts of solar storm activity.

The mission tackles a major challenge in heliophysics, our understanding of dynamic magnetic reconnection phenomena that vary on short timescales. TRACERS dual approach also enables scientists to discern between environmental shifts due to the travelling stars or to inherent magnetic variations. “These findings are crucial for basic studies of how the Earth’s magnetosphere interacts with solar energy,” said principal investigator David Miles.

TRACERS, a spacecraft located 590 kilometers above Earth, will collaborate with other missions to observe the Sun-Earth connection from various vantage points, providing unique low-orbit data to complement broader heliophysics observations.

The $170 million TRACERS mission, set to launch later in July, has been created to bolster readiness for such solar weather and keep space-dependent modern societies resilient and safe in a space-dependent world.

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