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Recent research is shedding new light on how rainfall affects the ocean’s ability to absorb carbon dioxide (CO₂) from the atmosphere—a factor that scientists have often overlooked when assessing how well our oceans act as a “carbon sink.” This latest study finds that rainfall can boost the ocean’s CO₂ uptake by 5 percent to 7 percent, meaning an extra 140 to 190 million metric tons of CO₂ are absorbed by the ocean every year. The research, led by David Ho, an oceanographer from the University of Hawai’i at Manoa, builds on work he began almost 30 years ago. In those early days, Ho set up two children’s pools to study how rain impacted CO₂ transfer between air and water. His recent work now provides the first global estimate of rainfall’s influence on CO₂ levels at the ocean’s surface.

Traditionally, scientists have focused on measuring CO₂ in deeper ocean samples, collected from 5 to 7 meters below the surface. These measurements miss the rain’s direct impact on the surface layer, where gas exchange with the atmosphere occurs most intensively.

How Rain Boosts Ocean Carbon Absorption

The study identifies three main ways rainfall increases ocean CO₂ absorption: turbulence, dilution, and wet deposition. First, raindrops hitting the ocean surface create turbulence, which increases the interaction between seawater and the atmosphere. Secondly, rainwater dilutes salty ocean water, altering the CO₂ concentration gradient and helping more CO₂ move into the ocean. Lastly, rain can carry CO₂ from the atmosphere as it falls, a process called wet deposition, which directly deposits CO₂ into the ocean.

Laetitia Parc, who led this research as part of her doctoral studies at Sorbonne Université, stresses the importance of understanding this effect. Quantifying how rainfall impacts ocean carbon absorption can improve the accuracy of models that track carbon exchanges between the ocean and atmosphere.

Implications for Climate Models

The team developed a model to monitor how rainfall affects ocean salinity at the surface. They found that turbulence and dilution play major roles in tropical regions, where warm water absorbs more CO₂. Meanwhile, wet deposition is particularly significant in areas with heavy rainfall, such as storm tracks and the Southern Ocean.

Tatiana Ilyina, an Earth scientist at Universität Hamburg, notes that this study makes a valuable contribution to understanding the global carbon cycle. As climate change is expected to alter global rainfall patterns, the effect of rain on ocean carbon absorption may also shift, with important implications for climate models and predictions.

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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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