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Technology

Massive Star WOH G64 Predicted to Die, Challenging Stellar Evolution Theories

by Rachel Kim – Technology Editor March 3, 2026
written by Rachel Kim – Technology Editor

Astronomers have observed an extraordinarily rare transformation in one of the largest known stars in the universe, WOH G64, signaling its imminent demise. The star, located in the Large Magellanic Cloud approximately 160,000 light-years from Earth, has rapidly shifted from a supergiant red star to a hypergiant yellow star, a change detected over the past decade.

The transition, noted as occurring on a cosmic timescale but remarkably swift in human terms, has baffled researchers due to the absence of typical accompanying phenomena like stellar flares or explosions. “Usually, stellar evolution happens on timescales of billions of years. On human timescales, we only observe more sudden and violent events, such as eruptions, the merging of two stars, or the explosive death of a star,” explained Gonzalo Muñoz-Sanchez, the lead author of a study published this week in the journal Nature Astronomy.

WOH G64 is estimated to have a mass roughly 28 times that of our Sun, but its diameter is approximately 1,500 times larger. If positioned at the center of our solar system, its surface would extend beyond the orbit of Saturn. The star is relatively young, at around 10 million years old, contrasting sharply with our Sun’s 4.5 billion-year age and projected lifespan of another 5 billion years.

Stars with masses between eight and 23 times that of the Sun are generally expected to evolve into red supergiants and eventually explode as supernovae. Yet, the fate of stars with masses between 23 and 30 solar masses, like WOH G64, remains uncertain. Scientists are currently unsure whether these massive stars will detonate as supernovae, collapse directly into black holes, or undergo a transition from a red supergiant phase to a yellow hypergiant phase before their final moments.

Adding to the complexity of studying WOH G64 is its existence within a binary star system, gravitationally bound to another star. Researchers have yet to determine the size or characteristics of the companion star, but speculate that the two stars may eventually merge. Recent observations from the James Webb Space Telescope have also uncovered details about former stars that have exploded as supernovae, providing further context to the study of stellar evolution [3].

The dramatic changes observed in WOH G64 are also occurring as scientists continue to monitor other massive stars in the universe, including observations of changes in one of the universe’s biggest stars [1]. Meanwhile, NASA is tracking a massive iceberg in the Southern Ocean that is predicted to completely disintegrate in the coming days [2], and researchers are even considering the possibility of using nuclear weapons to deflect potentially hazardous asteroids [4].

March 3, 2026 0 comments
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Health

New Giant Planet Discovered 271 Light-Years Away by Subaru Telescope & OASIS Project

by Dr. Michael Lee – Health Editor February 25, 2026
written by Dr. Michael Lee – Health Editor

Astronomers have announced the first discoveries from the Observing Accelerators with SCExAO Imaging Survey (OASIS), a new program utilizing the Subaru Telescope in Hawai’i to identify massive planets and brown dwarfs orbiting distant stars. The findings, detailed in a study published in The Astronomical Journal in December 2025, include the detection of a planet, HIP 54515 b, and a brown dwarf.

HIP 54515 b orbits a star located 271 light-years away in the constellation Leo. Researchers estimate the planet has a mass nearly 18 times that of Jupiter and orbits its star at a distance comparable to Neptune’s orbit around our sun. The proximity of the system to Earth – described by astronomers as being comparable to viewing a baseball from a distance of 100 kilometers – aided in the observation.

The OASIS program addresses a significant challenge in exoplanet detection: the extreme faintness of planets and brown dwarfs compared to their host stars. Only about 1% of stars are estimated to host massive planets and brown dwarfs bright enough to be directly imaged with current telescopes. Even in young planetary systems, where these objects retain heat from their formation, they remain difficult to distinguish from stellar glare.

OASIS, led by Thayne Currie and Masayuki Kuzuhara, employs a two-step process. First, it analyzes data from the European Space Agency’s Hipparcos and Gaia missions to identify stars exhibiting subtle movements caused by the gravitational pull of unseen companions. When a star shows evidence of being “tugged” or “wobbled,” the Subaru Telescope is then directed towards that target.

The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system is then used to capture high-resolution images, directly photographing these hidden objects. The system’s precision was crucial in observing HIP 54515 b despite the challenges of separating its light from the host star.

These discoveries also have implications for NASA’s upcoming Roman Space Telescope. The data gathered by OASIS will help test critical technologies for the Roman Space Telescope’s coronagraph, which is designed to directly image Earth-like planets around other stars.

Astronomers anticipate that the Subaru Telescope will continue to play a key role in astronomical discoveries as new, advanced telescopes come online.

February 25, 2026 0 comments
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Health

Mars Volcanoes: Complex Eruptions Reveal Planet’s Volcanic History

by Dr. Michael Lee – Health Editor February 24, 2026
written by Dr. Michael Lee – Health Editor

New orbital analysis of Pavonis Mons, one of the largest volcanoes on Mars, reveals a far more complex geological history than previously understood. The research, published in the journal Geology, indicates the volcano wasn’t formed by a single, massive eruption, but through multiple phases of activity powered by a long-lived and evolving magma system beneath the surface.

The findings challenge previous assumptions about the Red Planet’s volcanic activity and suggest Mars’ interior was more dynamic for a longer period than scientists believed. Researchers from Adam Mickiewicz University in Poland, the University of Iowa, and the Lancaster Environment Centre collaborated on the study, utilizing high-resolution images and mineral data collected from orbit.

“Our results show that even during Mars’ most recent volcanic period, magma systems beneath the surface remained active and complex,” said Bartosz Pieterek of Adam Mickiewicz University, who led the research. “The volcano did not erupt just once – it evolved over time as conditions in the subsurface changed.”

The team focused on a volcanic system south of Pavonis Mons, reconstructing its evolution in unprecedented detail by combining surface mapping with orbital mineral data. The analysis revealed a transition from early lava flows originating from fissures to later, point-source eruptions that created cone-shaped vents. These distinct phases are marked by variations in mineral composition, indicating shifts in the magma’s origin and storage depth.

“These mineral differences tell us that the magma itself was evolving,” Pieterek explained. The changing chemical signatures within the lava flows provide clues about the processes occurring within the subsurface magma reservoir.

The study highlights the difficulty of understanding subsurface processes on Mars without direct access to rock samples. Currently, scientists rely on remote sensing data to infer the hidden workings of Martian volcanoes. The new research demonstrates the value of this approach, providing rare insights into the planet’s interior and the long-term evolution of its volcanic systems.

According to a release from the Geological Society of America, the research builds on previous work suggesting that even seemingly recent volcanic features on Mars possess a more intricate history than initially thought. The findings contribute to a growing body of evidence indicating that Mars was geologically active for a considerable period, potentially influencing its climate and habitability.

The research team intends to continue analyzing data from Pavonis Mons and other Martian volcanic regions to further refine their understanding of the planet’s magmatic processes. No immediate follow-up missions to collect physical samples have been announced.

February 24, 2026 0 comments
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News

Ramadan 2026: Predicting the Start Date with Science & Hilal Criteria

by Emma Walker – News Editor February 14, 2026
written by Emma Walker – News Editor

Indonesia is bracing for a potential split in the start of Ramadan 2026, not due to observational challenges, but because of differing criteria used to determine the beginning of the Islamic holy month. The disagreement centers on the application of “local” versus “global” hilal (crescent moon) sighting standards, according to officials at the National Research and Innovation Agency (BRIN).

The Indonesian government, through the Ministry of Religious Affairs, and the majority of Islamic organizations in the country adhere to the “local” hilal criteria, known as MABIMS. This standard requires the hilal to be visible in Indonesia with a minimum height of 3 degrees and an elongation of 6.4 degrees. Muhammadiyah, one of Indonesia’s largest Islamic organizations, employs a “global” hilal criteria. This principle dictates that if the new moon meets visibility criteria anywhere on Earth, and the conjunction occurs before dawn in New Zealand, Ramadan has begun.

Astronomical data from the Meteorology, Climatology, and Geophysics Agency (BMKG) predicts the geosentric conjunction – when the Moon and Sun align – will occur on Tuesday, February 17, 2026, at 7:01 PM Western Indonesian Time (WIB). However, at that time across Indonesia, the hilal will remain below the horizon, with altitudes ranging from -2.41° in Jayapura to -0.93° in West Sumatra. The moon’s age will likewise be negative, indicating the hilal has not yet “born” at sunset.

those following the local hilal criteria are expected to complete the month of Sha’ban with 30 days, placing the first day of Ramadan 1447 H on February 19, 2026. Conversely, proponents of the global hilal criteria point to visibility in locations like Alaska, United States, on February 17th. Because the conjunction occurred before dawn in New Zealand and the hilal was considered “existent” globally, they are likely to commence Ramadan on February 18, 2026, according to BRIN’s Coordinator of Astronomy and the Center for Space Research, Professor Thomas Djamaluddin.

For those awaiting the Indonesian government’s official announcement following the isbat (confirmation) session, observation (rukyatul hilal) will be conducted on the evening of February 18, 2026. At that time, BMKG data indicates the hilal will be significantly more visible, reaching altitudes of 7.62° in Merauke to 10.03° in Sabang, well above the 3° requirement. Elongation will range from 10.7° to 12.21° (exceeding the 6.4° threshold), and the moon’s age will be 20 to 23 hours.

Despite the clarity provided by scientific calculations (hisab), the Indonesian government will still hold the isbat session on February 17, 2026. This session serves as a formal confirmation, reconciling mathematical calculations with observational data. Professor Djamaluddin emphasized that the purpose of the scientific data is not to create conflict, but to provide an objective understanding of the reasons for the potential differences. “Astronomically, there is no erroneous data; the differences arise solely from the different criteria believed,” he stated.

Consumer insights from YouGov, covering Indonesia, Malaysia, Saudi Arabia, Türkiye and the UAE, indicate a heightened focus on religious observance during Ramadan 2026, but do not address the potential divergence in start dates. The government has also set school learning policy for Ramadan 2026, but details of that policy were not available.

February 14, 2026 0 comments
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