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During the Diwali festival on October 25, there will be a partial solar eclipse which will be visible from the city as well as from most parts of the country, astrophysicist Debi Prasad Duari said. The eastern metropolis, however, will be able to witness the partial solar eclipse, the second in 2022, for a very small duration, the celestial phenomenon will be better observed in the northern and western regions of the country, he said.

The eclipse will not be observed from northeastern India as the celestial phenomenon will be occurring after sunset in those regions, Duari said.

Apart from India, the October 25 partial cosmic affair will be visible from most parts of Europe, northern Africa, the Middle East, and parts of Asia, Duari elaborated.

“The partial solar eclipse will begin in Iceland at around 2:29 pm IST and will be seen at its maximum from Russia at 4:30 hours IST. It will end at around 6:32pm IST over the Arabian Sea,” he told PTI while sharing information on the celestial event.

“The eastern part of the country will see the partial eclipse only marginally, that also during the sunset. The northern and western part of the country is a better location to observe the partial eclipse with a better view and for a longer period of time.

“During the new moon (Amavasya) the Sun, Moon, and Earth almost come in a linear configuration, whereby from the Earth we can see the Moon without any sunlight falling on it. But at times, as on October 25, the Sun, Moon, and Earth will almost be on the same plane resulting in the moon appearing to cover the Sun partially for a period of time causing a partial solar eclipse,” he explained.

In and around the metropolis, the partial eclipse will begin at around 4:52pm, the maximum occurring at 5:01pm, and will cease to be seen at 5:03pm at the sunset, Duari said.

“Even at the maximum eclipse, only 4 percent of the lighted disc of the setting Sun will be covered by the Moon,” he said.

In the north Bengal town of Siliguri, the celestial phenomenon will be occurring between 4:41pm and 4:59pm and during the maximum eclipse (at around 4:56pm) about 8.91 percent of the Sun will be covered by the Moon’s disc, Duari stated.

“In New Delhi, it will commence at around 4:29pm and end with the sunset at 6:09pm with the maximum eclipse to occur at 5:42pm when the Sun will be obscured by the Moon by an amount of only 24.5 percent,” Duari said.

Jaisalmer in Rajasthan will experience the eclipse from 4:26pm to 6:09pm with the maximum at around 5:30pm. when the disc of the Sun will be obscured by 42.5 percent.

“In Mumbai, the eclipse will begin at 4:49pm with the maximum occurring at around 5:42pm. It will end at 6:09pm, when the Sun appears to go down the Arabian Sea at sunset. Here, the Sun’s disc will be covered by about 24.5 percent,” he added.

In southern and central India, the eclipse will be again observed just before sunset with Nagpur experiencing the eclipse from 4:49pm to 5:42pm. In Bengaluru, the eclipse will begin at 5:12pm, reaching its maximum at 5:49pm and ending at 5:55pm during the sunset. Chennai will have the eclipse during 5:14pm to 5:44pm, the astrophysicist said.

The next major solar eclipse to be visible from India will be an annular eclipse on May 21, 2031 when the annularity can be observed from a narrow patch of land in south India, he said.

Three years later, on March 20, 2034, the next total solar eclipse will be visible from India and the totality will be observed from the northernmost part of Kashmir.

On both occasions, the whole country will observe a partial eclipse of varying magnitude depending upon its geographical location, Duari said.

Another partial eclipse can be seen from the northern part of India on June 1, 2030.

Referring to the harm caused to the eyes by Sun’s rays during an eclipse, Duari cautioned the sky enthusiasts to take “extreme precaution” while observing it.

“Even if the degree of the partial eclipse is not appreciable in most of the country, extreme precaution has to be taken by everybody who wants to observe this cosmic event. The Sun’s rays can be very harmful for the eye and can become critical,” he said.


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Newly Detected Seaborgium-257 Offers Critical Data on Fission and Quantum Shell Effects

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Newly Detected Seaborgium-257 Offers Critical Data on Fission and Quantum Shell Effects

German Scientists at GSI Helmholtzzentrum für Schwerionenforschung found a new superheavy isotope, 257Sg, named Seaborgium, which reveals unexpected details about the stability and nuclear fission. This study was published in Physical Review Letters and describes how this isotope, made by fusing chromium-52 with lead-206, survived for 12.6 milliseconds, longer than usual. The rare longevity and decay into 253Rf provide new indications of how K-quantum numbers or angular momentum impact the fission resistance. The findings fill in the gaps and give us an understanding of the effects of quantum shells in superheavy nuclei, which is crucial for preventing immediate disintegration.

Challenging Traditional Views on K-Quantum Numbers and Fission

As per the study by GSI, it challenges conservative views on how K-quantum numbers impact fission. Previously, it was found that the higher K values lead to greater fission hindrance, but after getting the findings from the GSI team, a more complex dynamic emerged. They found that K-quantum numbers offer hindrance to fission, but it is still ot known that it is how much, said Dr. Pavol Mosat, the study’s co-author.

Discovery of First K-Isomeric State in Seaborgium

An important milestone is the identification of the first K-isomeric state in seaborgium. In 259Sg, the scientists found that the conversion of the electron signal occurs 40 microseconds after the nuclear formation. This is clear evidence of the high angular momentum K-isomer. These states have longer lifetimes and friction in fission in a more effective way than their ground-state counterparts.

Implications for the Theorised Island of Stability

This discovery by the scientists provides key implications for the Island of stability, which has long been theorised. It is a region where superheavy elements could have comparatively long half-lives. If K-isomers are present in the still undiscovered elements such as 120, they can enable scientists in the detection of nuclei that would otherwise decay in just under one microsecond.

Synthesising 256Sg with Ultra-Fast Detection Systems

This team of German Scientists under GSI is now aiming to synthesise 256Sg, which might decay quicker than observed or predicted. Their success is dependent on the ultra-fast detection systems created by GSI, which are capable of capturing events within 100 nanoseconds. This continued research by the team may help in reshaping the search and studying the heaviest elements in the periodic table.

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NASA CODEX Telescope on ISS Reveals Hidden Secrets of the Sun’s Corona

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NASA CODEX Telescope on ISS Reveals Hidden Secrets of the Sun’s Corona

A mini solar telescope aboard the International Space Station caught the first-ever images, which reveal the subtle and never-seen changes in the outer atmosphere of the Sun. It is known as the Coronal Diagnostic Experiment (CODEX) and has been designed to understand the solar corona, the outer layer of the Sun, in depth. This mini telescope functions like a coronagraph, which blocks the Sun’s disk to imitate the total solar eclipse. CODEX was delivered through SpaceX Dragon on November 5, 2024. It was mounted on the ISS using the Canadarm2 robotic arm on November 9, 2025.

Revolutionising Solar Observation

According to the report by NASA, the unique design of CODEX consists of an occulting disk the size of a tennis ball held by three arms made up of metal. It allows it to block the intense sunlight when imaging the faint corona. The first images were revealed on June 10, 2025, at the time of the American Astronomical Society’s meeting in Alaska. These comprised pictures of coronal streamers and footage of the temperature fluctuations in the outer corona over many days. This offers a fresh perspective on solar dynamics.

Measuring Solar Wind Like Never Before

CODEX is unlike the previous coronagraphs as it is the first to measure both the speed and temperature of the solar wind. There is a constant flow of superhot particles from the Sun. With the help of four narrowband filters, in which two are used for determining the temperature and two for speed, astronomers compare brightness to decode these properties, which helps in solving the mystery of how the solar wind reaches 1.8 million degrees Fahrenheit.

Tackling the Solar Weather Challenge

To know the solar wind, it is crucial to predict the geomagnetic storms triggered by the coronal holes. Shortly, the storms observed on June 13, 2025 and June 25, 2025, caused auroras because of these events. After refining the analysis of solar wind, CODEX can help in mitigating and forecasting such kind of disturbances.

A Timely Launch Amid Solar Peak

NASA’s CODEX started operations at a suitable moment, just as the current solar maximum comes to its end. As the magnetic field of the Sun shifts during the solar battle zone, CODEX is ready to catch the critical data that can change our understanding of the weather in space.

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Rocket Lab Sets Record with ‘Symphony in the Stars’ Launch for Confidential Client

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Rocket Lab Sets Record with 'Symphony in the Stars' Launch for Confidential Client

Rocket Lab has launched the mysterious satellite on Saturday, June 28, 2025, making another milestone, as it is the first ever record of their missions. At 12:38 p.m. IST, the Electron rocket lifted from Launch Complex 1 in Mahia. The mission is known as “Symphony in the Stars,” and carried a single spacecraft above 650 kilometres above the Earth’s orbit. This satellite was deployed for a confidential commercial client, and the details are still not revealed. However, Rocket Lab has made a record by doing so.

Confidential Launch, Yet Revealed

As reported by Rocket Launch, it was the 68th Electron launch of Rocket Lab overall and the tenth mission of 2025. Even after its confidentiality, it was confirmed that it had successfully launched into space. Rocket Lab shared its news on social media regarding Mission Success and confirmed payload deployment. They further wrote, “Music to our ears for “Symphony in the stars.” It was one of the two missions dedicated to the same client, with the second launch to happen later in 2025.

This launch went through 48 hours after the “Get the Haw Outta Here mission.” This set a new record for the company. This different and every achievement highlights the reliability and ability of Electron Rocket Lab to offer responsive and repeatable access to space. It is a significant milestone, especially for the demand for fast satellite deployment continuity to arise.

Rocket Launch’s Occupied Month

It was a busy month for Rocket Launch as it went through the completion of four missions alone. Further, in the queue, after “Symphony in the Stars,” they launched “Full Stream Ahead,” then “The Mountain God Guards,” and “Get The Hawk Outta Here.” Every mission has supported commercial satellite operators, which demonstrates the versatility of Electron in rapid deployment schedules and handling.

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