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A recent study published in The Astronomical Journal has revealed the discovery of a fourth planet in the Kepler-51 system, an already remarkable planetary system known for hosting three ultra-low-density “super-puff” planets. This discovery was made by a research team led by Dr Jessica Libby-Roberts, a postdoctoral fellow at Penn State’s Centre for Exoplanets and Habitable Worlds, and Dr Kento Masuda, Associate Professor of Earth and Space Science at Osaka University. The finding suggests that the gravitational influence of the newly identified planet, named Kepler-51e, explains unexpected variations in the transit timings of the system’s known planets.

Unexpected Findings During Observations

As per a report by Phys.org, the researchers initially aimed to study Kepler-51d using NASA’s James Webb Space Telescope (JWST) but observed its transit occurring two hours earlier than predicted. This significant deviation prompted further analysis of data from NASA’s Kepler and TESS telescopes, Hubble Space Telescope and ground-based observatories such as the Apache Point Observatory (APO) and Palomar Observatory, as per reports. According to the team, only a four-planet model could account for the observed transit timing variations.

Insights Into the Kepler-51 System

Kepler-51e is believed to have a mass comparable to the existing planets in the system, following a relatively circular orbit of approximately 264 days. However, its classification as a “super-puff” remains uncertain due to the lack of transit data needed to calculate its radius and density. The inner three planets, known for their extremely low densities, continue to intrigue scientists. The team noted that accounting for the fourth planet alters previously estimated masses of the inner planets, slightly increasing their values while maintaining their status as super-puffs.

Future Implications of the Study

Dr Libby-Roberts, in a statement, indicated the potential for further exploration, stating that Kepler-51e’s orbit, located just inside the system’s habitable zone, suggests the possibility of additional planets or complex gravitational interactions. Continued observations may uncover planets farther from the star, contributing to the search for potentially habitable worlds. Researchers are also analysing data from JWST to study the atmospheric composition of Kepler-51d, which may shed light on the formation mechanisms of such unusual planets.

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Astronomers Spot Galaxy NGC 3640 With a Past of Consuming Smaller Galaxies

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Astronomers Spot Galaxy NGC 3640 With a Past of Consuming Smaller Galaxies

An elliptical galaxy located 88 million light-years from Earth has been observed displaying unusual characteristics, with astronomers identifying it as a cosmic predator. The latest images captured by the Very Large Telescope (VLT) at the European Southern Observatory (ESO) indicate that the galaxy, designated NGC 3640, has a history of consuming smaller galaxies and may soon engulf another. The galaxy’s distorted structure and the faint, diffused light surrounding it serve as evidence of its turbulent past, as per reports. Positioned just above a smaller galaxy, NGC 3641, the larger body appears to be on a trajectory that could lead to a future merger. The study of such interactions provides insights into the evolutionary patterns of galaxies.

Evidence of Past Galactic Mergers

According to research published in Astronomy & Astrophysics, signs of previous mergers have been detected within NGC 3640. The structural distortions observed, coupled with the presence of older stellar populations, suggest that remnants of previously absorbed galaxies are embedded within its formation. Astronomers at the Italian National Institute for Astrophysics have analysed the remnants, with findings indicating that ancient stars from the original galaxy serve as markers of past collisions. The faint glow surrounding NGC 3640 is attributed to these past interactions, demonstrating the lasting effects of galactic mergers.

Upcoming Galactic Collision

Reports suggest that while NGC 3641 remains intact, its eventual fate may align with the ongoing patterns of NGC 3640. As galaxies interact, their gravitational forces distort their structures, often leading to eventual mergers. Current observations indicate no immediate impact on NGC 3641, implying that significant interactions have yet to begin. ESO officials have stated that galaxies undergo structural changes over time due to the absorption of gas and stars from their surroundings. This process has been linked to the unique shape and features displayed by NGC 3640.

Gravitational Influence and Cosmic Evolution

The gravitational forces exerted by approaching galaxies can trigger large-scale changes in their structures. Astronomers have been closely monitoring such interactions to gain a deeper understanding of galactic evolution. The observations made using the VLT provide an opportunity to study these cosmic processes in detail, with researchers continuing to track the potential merger between NGC 3640 and its smaller companion. The findings contribute to broader studies on the dynamic nature of galaxies and their role in shaping the universe over billions of years.

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Scientists Discover Declining Global Ocean Evaporation Amid Rising Temperatures

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Scientists Discover Declining Global Ocean Evaporation Amid Rising Temperatures

A decline in global ocean evaporation has been identified over the past decade, despite rising sea surface temperatures. This shift challenges established climate models, which have long linked higher temperatures to increased evaporation. The unexpected trend was observed through satellite data analysis, revealing that evaporation rates started decreasing after 2008. Researchers suggest that changing atmospheric circulation patterns and reduced wind speeds may be influencing this reversal, highlighting the complexity of Earth’s climate system.

Study Reveals Key Climate Anomalies

According to the study published in Geophysical Research Letters, an assessment of ocean heat flux data was conducted by researchers from the Institute of Geographic Sciences and Natural Resources Research at the Chinese Academy of Sciences. It was found that while ocean evaporation had been rising from 1988 to 2008, a reversal occurred thereafter, leading to a decline between 2008 and 2017.

The study’s lead author, Dr. Ma Ning, told Phys.org that two-thirds of the global oceans have shown reduced evaporation rates since the late 2000s. This decline contradicts previous expectations that global warming would consistently drive higher evaporation levels. The research suggests that large-scale atmospheric circulation shifts, particularly in the Northern Oscillation Index, may be contributing to the changes.

Impact of Wind Stilling on Evaporation

A decline in wind speed, referred to as “wind stilling,” has been identified as a crucial factor in this unexpected trend. Lower wind speeds result in reduced surface turbulence, thereby limiting the exchange of moisture between the ocean and the atmosphere. The study indicates that this phenomenon may be linked to broader climate oscillations affecting atmospheric circulation.

Dr. Ma explained that while evaporation levels have declined, this should not necessarily be viewed as a weakening of the global hydrological cycle. Instead, it may be an indication of natural climate variability influencing regional and global weather patterns. Researchers continue to investigate how these findings may affect long-term climate predictions.

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Arabia Had Five Times More Rainfall 400 Years Ago, Study Finds

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Arabia Had Five Times More Rainfall 400 Years Ago, Study Finds

Extreme rainfall in Arabia was five times more intense 400 years ago, as indicated by recent climate reconstructions. The data suggests that the region, currently defined by arid desert, once had significantly higher precipitation levels, resembling a lush savannah. The findings highlight the necessity for improved climate preparedness as urbanisation expands in the region.

Study Reveals Significant Rainfall Variability Over Centuries

According to the study published in Science Advances, researchers from the University of Miami Rosenstiel School of Marine, Atmospheric, and Earth Science discovered that the Arabian Peninsula had significantly higher rainfall over the last 2,000 years. The landscape, now barren, was once covered with vegetation and inhabited by wildlife such as lions, leopards, and wolves. Findings indicate that 200 years ago, rainfall was still double what it is today.

Deep-Sea Brine Pools Provide Uninterrupted Climate Record

As per reports, sediment cores were extracted from a deep-sea brine pool in the Gulf of Aqaba using a remotely operated vehicle (ROV) deployed from the research vessel OceanXplorer. The brine’s chemistry enabled the preservation of undisturbed sediment layers, allowing an accurate reconstruction of Late Holocene rainfall trends.

Implications for Climate Preparedness in the Middle East

Speaking to Phys.org, Sam Purkis, Professor and Chair of the Department of Marine Geosciences at the University of Miami Rosenstiel School, stated that the study underscores the importance of climate resilience as development projects like NEOM in Saudi Arabia reshape the region. The assumption of long-term climate stability is not reliable, according to Amy Clement, a Professor in the Department of Atmospheric Sciences at the same institution.

Urgency for Enhanced Flood and Drought Management

The Middle East, already vulnerable to extreme weather, faces rising instances of flash floods and droughts. The catastrophic flooding seen across the Arabian Peninsula in early 2024 reinforces the need to study historical rainfall patterns to improve disaster preparedness. Mattie Rodrigue, Science Program Director at OceanX, highlighted the importance of technological advancements in climate research to better predict future hydroclimate trends.

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