Connect with us

Published

on

Astronomers continue to monitor the Corona Borealis constellation for a rare celestial event — the expected eruption of T Coronae Borealis (T CrB), as per sources. This binary star system, home to a white dwarf and a red giant, is predicted to produce a nova, briefly illuminating the night sky with a brightness comparable to Polaris, the North Star. While initial predictions placed the event as imminent by September 2023, observations suggest the outburst could occur later than anticipated.

A History of Eruptions

According to a report by Space.com, T CrB has a history of dramatic eruptions, with confirmed events in May 1866 and February 1946. These outbursts occur when the white dwarf accumulates sufficient material from the red giant, triggering a nuclear explosion. Previous eruptions have followed an 80-year cycle, suggesting the next event might occur by 2026. However, brightness changes observed in 2015 and dimming patterns similar to those preceding the 1946 eruption have led to revised estimates, prompting predictions for 2023 or 2024.

Monitoring the System

As per the report, data is being gathered using an array of space and ground-based telescopes, including NASA’s Fermi Gamma-ray Space Telescope, the James Webb Space Telescope, and the Very Large Array in New Mexico. Elizabeth Hays, an astrophysicist monitoring T CrB with Fermi, indicated to Space.com that while signs point to an impending eruption, pinpointing the exact timeline remains elusive.

Edward Sion, professor of astronomy at Villanova University, highlighted the complexities of the accretion process. He told the publication that the challenges posed by fluctuating rates of material transfer between the stars, which add uncertainty to the prediction.

The Wait Continues

Until the eruption occurs, astronomers are using this opportunity to collect unprecedented data. Observations across multiple wavelengths are being conducted to better understand the behaviour of novae. Experts suggest these findings will enhance future predictive models and deepen insights into stellar phenomena.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


From iQOO 13 to Offline Expansion, and Whether AI Will Be a Differentiator for Consumers: CEO Nipun Marya Talks to Gadgets 360



Fruit Fly Experiment on Tiangong Space Station Explores Effects of Microgravity

Continue Reading

Science

Indian Ocean Anomaly Challenges Ekman’s Ocean Current Theory

Published

on

By

Indian Ocean Anomaly Challenges Ekman’s Ocean Current Theory

A study published in Science Advances has identified a significant anomaly to Vagn Walfrid Ekman’s widely-accepted theory on wind-driven ocean currents. Conducted by a team of researchers from NOAA, the Indian National Center for Ocean Information Services and the University of Zagreb, the study focused on the Bay of Bengal in the Indian Ocean. Data spanning several years from a buoy stationed off India’s eastern coast was examined, revealing that ocean currents in this region deflect leftward, contradicting the theory’s predictions for the Northern Hemisphere.

Ekman’s Theory and Its Longstanding Influence

The Ekman theory, developed in 1905 by Swedish oceanographer Vagn Walfrid Ekman, asserts that surface ocean currents are deflected 45 degrees to the right of wind direction in the Northern Hemisphere due to the Coriolis force. Successive layers beneath the surface exhibit similar patterns, forming the Ekman spiral. This mechanism, though robust, assumes idealised conditions, including uniform ocean depth and density. Variations such as those observed in the Bay of Bengal highlight its limitations.

Findings from the Bay of Bengal

As per the study, according to data collected over several years, currents in the Bay of Bengal were found to veer leftward despite prevailing winds, defying Ekman’s predictions. This anomaly underscores the need to reassess assumptions about global oceanic patterns. The researchers suggested that local factors, including unique regional wind patterns and oceanic dynamics, could play a significant role.

Implications for Climate Models

It was noted in a statement by the researchers that the findings could influence future climate modelling efforts. If exceptions to Ekman’s theory exist in the Bay of Bengal, others might also occur globally, underscoring the need for more detailed oceanographic studies. Discussions have also highlighted the potential deployment of a NASA satellite system to monitor wind and surface currents comprehensively.

This study has brought attention to gaps in understanding wind-driven currents, stressing the importance of revisiting established models as global warming continues to impact ocean behaviour.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


World Labs Unveils AI System That Can Generate 3D Interactive Worlds Using an Image



Samsung Galaxy Z Fold 7, Galaxy Z Flip 7 to Debut With Larger Displays: Report

Related Stories

Continue Reading

Science

ISRO’s PSLV-C59 to Launch ESA’s Proba-3 Mission for Sun Corona Study

Published

on

By

ISRO's PSLV-C59 to Launch ESA's Proba-3 Mission for Sun Corona Study

The Indian Space Research Organisation (ISRO) has scheduled the launch of the PSLV-C59 rocket carrying the Proba-3 spacecraft for December 4, 2024, at 4:08 PM IST, as per reports. The mission, a dedicated commercial venture of NewSpace India Limited (NSIL), will take off from the First Launch Pad at the Satish Dhawan Space Centre, Sriharikota. According to reports, this will mark the 61st mission of the Polar Satellite Launch Vehicle (PSLV) and the 21st use of its XL configuration.

Mission Overview

As per sources, Proba-3, a project developed by the European Space Agency (ESA), is an In-Orbit Demonstration (IOD) mission aimed at showcasing precision formation flying. The spacecraft consists of two components: the Coronagraph Spacecraft (CSC) and the Occulter Spacecraft (OSC). These satellites, launched in a stacked arrangement, will operate in tandem, maintaining a precise distance of 150 meters. The innovative configuration will enable the creation of artificial solar eclipses, allowing extended observation of the Sun’s corona.

Scientific Objectives

Reports indicate that the mission’s primary objective is to explore the Sun’s corona, the outermost layer of its atmosphere, to enhance understanding of solar dynamics and space weather. Instruments aboard the spacecraft have been designed to block the Sun’s intense light, facilitating detailed study of solar phenomena that are otherwise difficult to observe. Proba-3’s ability to continuously monitor the corona for up to six hours is expected to yield valuable scientific data.

Collaboration and Technology

The mission highlights significant collaboration between ISRO and ESA. Reportedly, the PSLV-XL rocket, equipped with additional strap-on boosters, will carry a payload weighing approximately 550 kg. The precision formation flying technology demonstrated by Proba-3 is expected to pave the way for advanced techniques in space exploration. The launch preparations at the Satish Dhawan Space Centre are underway, and all systems are reportedly on track for the scheduled liftoff.

Continue Reading

Science

Meet Homo juluensis: A newly discovered ancient human species

Published

on

By

Meet Homo juluensis: A newly discovered ancient human species

A new ancient human species, Homo juluensis, has been identified by researchers, marking a significant step in understanding human evolution in the Middle Pleistocene epoch. According to findings published in PaleoAnthropology in May 2024, the discovery is based on fossil evidence unearthed in China, with specimens dating between 220,000 and 100,000 years ago. The species, known as “big head people,” is characterised by large skulls, blending features seen in modern humans, Neanderthals and Denisovans.

Fossil Evidence and Characteristics

The fossils forming the basis of this new classification were recovered from sites in Xujiayao and Xuchang in northern and central China, as per reports. Excavations at Xujiayao in the 1970s yielded over 10,000 stone tools and 21 fossil fragments, representing at least 10 individuals. These fossils display large, wide crania with Neanderthal-like characteristics, yet also share traits with modern humans and Denisovans. Four additional ancient skulls discovered at Xuchang exhibit similar features.

The research team, led by Christopher Bae, an anthropologist at the University of Hawai’i and Xiujie Wu, a paleoanthropologist at the Chinese Academy of Sciences, concluded that these fossils represent a distinct hominin population. The findings indicate a likely continuity of hybridisation among Middle Pleistocene hominins, which shaped human evolution in eastern Asia.

Naming and Expert Perspectives

In a statement to Nature Communications, published in November 2024, the researchers advocated for using Homo juluensis to clarify eastern Asia’s complex fossil record. While some experts, such as Chris Stringer of the Natural History Museum in London, have suggested the fossils might align more closely with Homo longi, the designation of Homo juluensis has gained traction.

The name, according to Bae, in a statement, was introduced to improve scientific communication. Paleoanthropologist John Hawks of the University of Wisconsin–Madison noted in a blog post that such terminology allows clearer reference to this population’s place in the human evolutionary narrative. The discovery underscores the intricate relationships within ancient hominin groups and their evolutionary significance.

Continue Reading

Trending