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The National Oceanic and Atmospheric Administration (NOAA) has released footage from its latest solar telescope, the Compact Coronagraph (CCOR-1). Launched with the GOES-19 weather satellite this past summer, CCOR-1 has already offered a detailed glimpse of charged particles exploding from the Sun’s corona, showcasing its ability to capture high-energy solar events. Positioned aboard the GOES-19 satellite, this telescope will help NOAA monitor solar activity as the Sun nears the peak of its 11-year cycle, expected in 2025.

Unveiling the Corona’s Activity

NOAA’s footage, released on October 22, highlights the power of the CCOR-1 telescope. This coronagraph blocks intense sunlight from the Sun’s central disk, allowing scientists to observe the corona — the Sun’s outermost layer — where extreme solar activity occurs. The telescope’s design enables researchers to watch as streams of solar plasma radiate outwards, providing insights into coronal mass ejections (CMEs) and other events crucial to understanding solar behavior.

Impact of Solar Ejections on Earth

These intense CMEs, driven at speeds ranging from hundreds to thousands of miles per second, pose significant risks to satellites, astronauts and even terrestrial technology. The Earth’s magnetic field offers some protection, but powerful solar eruptions can interfere with aviation communications, disrupt power grids and create vivid auroras. When we observe these solar storms in real-time, NOAA can better predict potential impacts, helping to safeguard infrastructure and ensure rapid responses to solar disruptions.

GOES-19’s Role in Space Weather Monitoring

The GOES-19 satellite sits 22,236 miles above the equator, orbits at a pace synchronised with Earth’s rotation, enabling constant observation of the same geographical area. While the satellite is still undergoing final testing and calibrations, NOAA plans to activate its full capabilities by spring 2025, just ahead of the Sun’s anticipated activity peak in July 2025. Through CCOR-1, NOAA’s mission to observe and understand the Sun’s dynamic corona will enhance forecasting for space weather, benefiting various sectors reliant on space-based technology.

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Supernova Remnant G278.94+1.35 is Closer to Earth, Claims New Study

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January 10, 2025

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Supernova Remnant G278.94+1.35 is Closer to Earth, Claims New Study

A significant discovery involving a supernova remnant in the Milky Way, identified as G278.94+1.35, has been made by a team of international astronomers. This structure, resulting from a massive stellar explosion, was initially thought to be approximately 8,800 light years away. New findings have revised this distance to about 3,300 light years, making it closer than previously calculated. The remnant’s estimated physical dimensions have also been adjusted to around 189 by 182 light years, contrary to earlier assessments of over 500 light years.

Insights from the Study

According to the study published December 30 on the pre-print server arXiv, highlighted the properties of this remnant. The research team, led by Miroslav D. Filipović, Professor at Western Sydney University, observations were conducted using the Australian Square Kilometer Array Pathfinder (ASKAP) as part of the ASKAP-Evolutionary Map of the Universe project. These observations revealed the nearly circular shape and expansive nature of the remnant, now named “Diprotodon,” in homage to an extinct giant marsupial native to Australia.

The research team attributed the name to raise awareness about the prehistoric megafauna of Australia and ongoing extinction challenges. The findings, as reported by phys.org indicate that the supernova remnant is in a radiative evolutionary phase, suggesting continued expansion.

Characteristics and Significance

Diprotodon’s progenitor star is estimated to have been about 15 times the mass of the Sun. The kinetic energy released during the explosion is approximated at 500 quindecillion ergs. The spectral index of the remnant, measured at around -0.55, aligns with typical shell-type remnants observed in the galaxy. These characteristics place it among the largest supernova remnants known, providing valuable insights into the dynamics of such structures.

The study has offered critical data regarding the formation, expansion, and current state of Diprotodon, contributing to the broader understanding of supernova remnants within the Milky Way.

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PFAS Chemicals Harm Freshwater Turtles in Australia, New Research Finds



NISAR Satellite by NASA and ISRO to Monitor Earth Like Never Before

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NISAR: NASA & ISRO’s joint satellite to monitor Earth like never before

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January 10, 2025

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NISAR: NASA & ISRO’s joint satellite to monitor Earth like never before

A collaboration between NASA and the Indian Space Research Organisation (ISRO) has resulted in the NISAR (NASA-ISRO Synthetic Aperture Radar) satellite, which is set to launch in a few months. This mission, designed to track and monitor Earth’s dynamic surface, will use synthetic aperture radar technology to measure changes in land and ice formations. Capable of delivering precise data down to centimetre-level accuracy, NISAR will contribute significantly to understanding natural disasters, ice-sheet movements, and global vegetation shifts.

Unique Dual-Band Technology

According to an official press release by NASA, NISAR is equipped with two radar systems: the L-band with a wavelength of 25 centimetres and the S-band with a 10-centimetre wavelength. This dual-band configuration enables detailed observations of various features, from small surface elements to larger structures. These advanced radars will collect data frequently, covering nearly all land and ice surfaces to provide a comprehensive view of Earth’s transformations.

Technology and Data Applications

As per reports, synthetic aperture radar technology, first utilised by NASA in the 1970s, has been refined for this mission. The data from NISAR will support ecosystem research, cryosphere studies, and disaster response initiatives. Stored and processed in the cloud, the data will be freely accessible to researchers, governments, and disaster management agencies.

Collaboration Between NASA and ISRO

The partnership between NASA and ISRO, formalised in 2014, brought together teams to create this dual-band radar satellite. Hardware was developed across continents, with final assembly in India. ISRO’s Space Applications Centre developed the S-band radar, while NASA’s Jet Propulsion Laboratory provided the L-band radar and other key components. The satellite will launch from ISRO’s Satish Dhawan Space Centre and will be operated by ISRO’s Telemetry Tracking and Command Network.

NISAR’s deployment highlights international collaboration in addressing global challenges, promising transformative insights into Earth’s changing landscapes.

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Velvet Ants Venom Affect Mammals and Insects Differently

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January 10, 2025

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Velvet Ants Venom Affect Mammals and Insects Differently

Velvet ants, despite their name, are not ants but parasitic wasps known for their painful stings. These insects, often called “cow killers” due to the intensity of their sting, possess a potent venom capable of acting on different molecular targets depending on the species they encounter. Their defensive mechanisms, which include venom, warning colours, tough exoskeletons, and unique sounds when threatened, have made them nearly invincible to predators. This versatility has intrigued researchers studying their venom’s effects on various creatures.

Study Highlights Dual Mechanisms in Velvet Ant Venom

According to a study published in Current Biology, velvet ant venom operates differently across species. Researchers, including Lydia Borjon, a sensory neurobiologist at Indiana University Bloomington, found that distinct peptides in the venom affect mammals and insects in unique ways. Experiments conducted on the venom of the scarlet velvet ant (Dasymutilla occidentalis) revealed that specific peptides target sensory neurons differently in insects and mammals.

As reported in Science News, in insects, a peptide called Do6a specifically activates neurons sensitive to harmful stimuli. However, in mammals such as mice, pain is triggered by two less abundant peptides, Do10a and Do13a. These peptides activate a broad range of sensory neurons, inducing a generalised pain response. The findings suggest that velvet ants’ venom tailors its effects based on the biology of the recipient, showcasing a rare example of multi-target venom.

Broader Implications of the Research

Joseph Wilson, an evolutionary ecologist at Utah State University, noted to Science News, that velvet ants’ extensive defensive arsenal could be linked to evolutionary pressures from unknown predators, particularly insects. He suggested that while their venom effectively deters a wide range of species, its evolution might have been influenced by specific ecological interactions. Sam Robinson, a toxinologist at the University of Queensland, highlighted that this type of broad-spectrum venom, though rare, may not be unique, as most venoms are tested on limited species.

The study provides new insights into venom evolution and raises questions about the ecological factors driving the development of such complex defensive strategies.

https://www.gadgets360.com/science/news/nasa-delays-artemis-2-and-artemis-3-missions-to-address-key-technical-challenges-7321848

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