Study finds Irminger Sea key to Atlantic current’s stability
A new study highlights the critical role of the Irminger Sea, located off southeastern Greenland, in maintaining the strength of the Atlantic Meridional Overturning Circulation (AMOC). The AMOC, a global ocean conveyor belt, is crucial for regulating Earth’s climate, particularly in the Northern Hemisphere. According to research led by Dr Qiyun Ma, a postdoctoral researcher at the Alfred Wegener Institute for Polar and Marine Research in Germany, disruptions in this region could have far-reaching climate impacts.
Dr Ma emphasised that freshwater input into the Irminger Sea directly inhibits deep-water formation, a key process for sustaining the AMOC. This reduction in deep-water currents, caused by increasing Arctic meltwater, significantly alters atmospheric circulation and disrupts the broader ocean current system. The study underscores the urgent need for targeted monitoring of the Irminger Sea, as findings suggest its influence on the AMOC surpasses that of neighbouring regions, including the Labrador Sea and Nordic Seas.
Freshwater Flow Weakens Ocean Currents
The research simulated scenarios of increased freshwater in four regions of the North Atlantic and assessed the AMOC’s sensitivity. It was discovered that the Irminger Sea plays a unique role in regulating deep-water formation across adjacent seas, including the Labrador Sea. Freshwater input in this area also exacerbates climate extremes, such as altered precipitation patterns in North America and the Amazon Basin.
Wider Climate Implications
Findings from this study align with earlier predictions of Northern Hemisphere cooling and Arctic sea ice expansion due to a weakening AMOC. Additionally, slight warming in the Southern Hemisphere and disruptions to tropical monsoon systems were observed. Dr Ma pointed out that the location of freshwater input heavily influences these outcomes, making precise predictions more challenging.
The study, published in Science Advances on November 20, highlights the growing need for climate experts and policymakers to address AMOC vulnerabilities. Enhanced monitoring of sensitive areas like the Irminger Sea could aid in developing adaptive strategies to mitigate future climate disruptions.
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Bronze statues, including depictions of snakes and a child priest, have been uncovered from a hot spring at San Casciano dei Bagni in Italy, according to the Italian Ministry of Culture, as per reports. The site, located around 120 kilometres northwest of Rome, has been excavated since 2019 and is believed to have been used for sacred rituals dating back to the third century B.C. The spring, originally used by the Etruscans and later adopted by the Romans, was a place where votive offerings were made in hopes of divine protection or healing, as per reports.
Discovery of Snake Statues and Other Artefacts
Bronze snake statues, some measuring up to 90 centimetres in length, were among the latest findings during the 2024 excavation, as reported by the excavation team. These statues were discovered in the deeper layers of the spring and are thought to have symbolised protection for the sacred waters. Other artefacts include a nude male figure inscribed with the name “Gaius Roscius” and a child priest holding a ball, which may have been used in divination rituals.
Preserved Organic Remains Found
The excavation also revealed well-preserved organic remains, such as eggs with visible yolks, pine cones, and plant matter. According to the Italian Ministry of Culture, in a statement, these items may have been used in rituals symbolising rebirth and regeneration. The preservation of these items is attributed to their rapid burial in sediment.
Expert Perspective
Alexandra Carpino, an art history professor at Northern Arizona University, commented in an email to Live Science that these findings are among the most significant discoveries of the 21st century. The range of artefacts provides insights into the role of healing sanctuaries in ancient societies.
Ongoing Research at the Site
Research continues at San Casciano dei Bagni, with scholars examining the inscriptions and artefacts to uncover more about the Etruscan and Roman use of the spring.
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A new pulsar, PSR J1922+37, has been discovered with a spin period of 1.92 seconds using the Five-hundred-metre Aperture Spherical Radio Telescope (FAST) in China, according to a report. The finding was made in the direction of the open cluster NGC 6791. If confirmed as a member of this cluster, it would be the first pulsar identified in an open cluster, a breakthrough in pulsar and stellar cluster research, according to sources.
Key Details of PSR J1922+37
The finding was reported in a paper published Dec. 11 on the arXiv preprint server. As per reports, the pulsar PSR J1922+37 has been observed with a dispersion measure of 85 pc/cm³ and a flux density of approximately 7.0 µJy. Its position aligns closely with the location of NGC 6791, with an offset of 14 arcminutes from the cluster’s centre. The estimated distance of the pulsar, 15,600 light-years, is consistent with the cluster’s distance range, which is calculated to be between 13,100 and 16,000 light-years.
According to the study, led by Xiao-Jin Liu of Beijing Normal University, the dense stellar environment of NGC 6791 increases the likelihood of pulsars being present within the cluster. Researchers have suggested that precise measurements of PSR J1922+37’s distance and proper motion will be necessary to confirm its association with NGC 6791.
Potential for Further Discoveries
The researchers indicated that NGC 6791’s compact and high surface brightness environment could host additional pulsars. An estimate provided in the study predicts that as many as nine pulsars may exist within this cluster. The team noted that further observations using advanced techniques could help verify these predictions.
The report further highlights that the discovery has been described as a significant development in the understanding of pulsars within open clusters, an area of study previously limited due to low stellar density in such regions. Verification of PSR J1922+37’s cluster membership will require additional studies, including proper motion analysis to establish a definitive connection.
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