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Recent archaeological research has uncovered evidence that humans were living near West Papua more than 55,000 years ago, offering new insights into early human migration into the Pacific. The discovery was made in Mololo Cave, located on Waigeo Island in the Raja Ampat archipelago. This significant find includes stone tools, animal bones, and a tree resin artefact, which points to the complex skills developed by these early settlers. These findings provide valuable clues about how humans adapted to the challenging environments of tropical rainforests and coastal regions during this critical period in human history.

Archaeological Findings at Mololo Cave

The Mololo Cave excavation is the result of an extensive international collaboration involving experts from New Zealand, West Papua, and Indonesia. The cave, surrounded by dense tropical rainforest, revealed several layers of ancient human occupation.

Radiocarbon dating confirmed that humans were present at the site at least 55,000 years ago. Among the most intriguing discoveries was a tree resin artifact, representing the earliest known use of resin outside Africa. This artifact, likely used as a fuel source, showcases the innovative approaches early humans employed to thrive in their environment.

Seafaring Routes to the Pacific

The study also sheds light on the routes early humans took as they migrated into the Pacific region. The evidence supports the theory that the earliest seafarers traveled along a northern route through West Papua, before eventually reaching Australia. This challenges the previously held belief that a southern route via Timor was the primary path. Understanding these migration routes is essential, as it provides a clearer picture of how quickly humans dispersed across Asia and Oceania, and how they interacted with other species, such as the “hobbit” (Homo floresiensis) in Indonesia.

The Role of West Papua in Human Migration

Despite these recent findings, much of West Papua’s ancient history remains a mystery due to political and social challenges in the region. The new research highlights the importance of continuing archaeological work in this area to gain a deeper understanding of the origins and adaptations of early Pacific settlers. Ongoing excavations and studies in West Papua will help fill in the gaps in our knowledge about the early migration patterns and the development of human societies in this vast and complex region.

Implications for Future Research

The discoveries at Mololo Cave are just the beginning of a more comprehensive exploration of West Papua’s role in human history. As researchers continue to investigate this region, they hope to uncover more evidence that will provide insights into how early humans adapted to different environments, from dense rainforests to coastal areas. These findings will not only contribute to our understanding of human migration but also offer a more detailed view of the diverse strategies employed by our ancestors to survive and thrive in new and challenging landscapes.

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Earth’s Oldest Impact Crater Turns Out to Be Much Younger Claims New Study

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Earth’s Oldest Impact Crater Turns Out to Be Much Younger Claims New Study

A location in Western Australia that used to be named as the oldest meteorite impact crater on Earth is now actually a lot younger than that, scientists announced today in Science Advances. The structure — previously dated to 3.5 billion years ago and located within Western Australia’s North Pole Dome region of the Pilbara — was believed to be older than any of Earth’s known impact craters. Today, new research published in the journal Geochemistry found that what we now call the Miralga impact structure is, in fact, much younger, at 2.7 billion years old, and considerably smaller in diameter. This recasts earlier ideas on the early Earth’s geological activity and questions previous theories regarding impact-driven crust formation or perhaps even early life.

Miralga Crater Loses Oldest Impact Title but Gains New Scientific Relevance

As per The Conversation article republished by Space.com, the teams that explored the crater could only point to one thing that was likely — it had been formed by an impact. However, they ultimately disagreed as to whether this event had been and how large it was. Younger rocks contain shatter cones, indicating Earth’s early continental geology shielded the impact to a specific 2.7 billion-400 million-year period despite earlier assertions.

They made the determination to honour the cultural revision of one site from 100 km across to a more manageable 16 km wide crater named Miralga. It’s the site – still affected by seawater – of events too recent to influence the Earth’s crust.

The Miralga basalt feature (unique to basalt) is a rare site for an instrument to practice on before heading to Mars, while advancing our understanding of impacts and early life prospects.

Isotopic dating to clarify the crucial part played by this, the oldest crater on Earth and unique in a geological sense, in planetary science and early Earth history is presently ongoing at Miralga.

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NASA’s TRACERS Satellites Begin Solar Wind Study Despite SV1 Glitch

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NASA's TRACERS Satellites Begin Solar Wind Study Despite SV1 Glitch

NASA’s TRACERS mission twin satellites were launched on July 23, 2025, to study how solar activity causes magnetic reconnection in Earth’s atmosphere. After launch, a power subsystem anomaly had affected one of the satellites (Space Vehicle 1, SV1) on July 25, causing periodic communication loss. NASA said satellite 2 (Space Vehicle 2, SV2) is “healthy,” and transition is beginning to the instrument commissioning phase. The idea behind TRACERS was to develop a complete toolkit that would allow us, for the first time, to observe all of these complex solar wind connection processes at once. NASA engineers are actively working to recover SV1. Single vector views (SV2) spacecraft are completing a healthy checkout and readying themselves for their science mission.

Recovery Efforts for SV1 Satellite

According to NASA, controllers detected a problem with SV1’s power subsystem in late July that led to intermittent contacts and a loss of communication. Data suggest SV1 can only remain active when its solar panels receive sufficient sunlight. Because of the spacecraft’s current orientation, engineers plan to wait until later in August — when SV1’s panels will receive more sun — to reestablish contact and continue recovery steps.

Meanwhile, mission teams are reviewing onboard data to diagnose the issue and plan next steps. Any time contact is regained, the team will assess SV1’s status and check for impacts on the mission’s science goals. For now, no significant updates on SV1 are expected for several weeks.

SV2 Operational Status

The mission’s other satellite, SV2, is in good health and fully operational. Mission teams have been testing SV2’s onboard instruments and systems through a standard commissioning process. This checkout is proceeding as expected, with NASA anticipating that commissioning will finish by the end of August.

Once SV2 is fully checked out, it will begin coordinated science operations with its twin to study magnetic reconnection – the process that shapes how solar activity affects Earth’s magnetic environment. For now, SV2 continues its planned tests and will soon be ready to collect valuable science data as part of the TRACERS mission.

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Scientists Explore Role of Space Radiation in Powering Alien Microbial Life

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Scientists Explore Role of Space Radiation in Powering Alien Microbial Life

The search for alien life traditionally focuses on planets in the “Goldilocks zone” — the orbital band where surface water can exist. But new research suggests life might thrive far from starlight in a so-called “radiolytic habitable zone,” where penetrating cosmic rays break buried water molecules (a process called radiolysis) into hydrogen, oxygen and energy-rich electrons. Simulations of icy worlds like Mars, Europa and Saturn’s moon Enceladus show cosmic rays can reach subsurface water. Researchers suggest these electrons could fuel microbes in hidden reservoirs, effectively creating underground oases of life.

Radiation as a Power Source

According to the new study, cosmic rays are fast-moving particles (electrons, protons or nuclei) blasted out by supernovas and distant stars. On Earth, most are stopped by our magnetic field and thick atmosphere. But Mars and the icy moons (which lack such shields) get hit directly; their thin air or vacuum allows rays to penetrate deep into ice and rock. When these particles strike water or ice, they trigger radiolysis – shattering molecules and freeing hydrogen, oxygen and electrons. Some Earth microbes already exploit this: for example, a bacterium 2.8 km underground in a gold mine lives entirely on hydrogen produced by radioactive decay.

Expanding the Search for Life

Dubbed the “Radiolytic Habitable Zone,” this hidden-energy band lies beneath ice or rock where cosmic rays can sustain life. Simulations show Saturn’s icy moon Enceladus has the highest radiolytic potential, followed by Mars and then Jupiter’s moon Europa. NASA’s upcoming Europa Clipper mission and telescopes like ALMA will probe these frozen worlds for chemical signs of life. Even more intriguingly, cosmic-ray impacts can directly create complex organic molecules (for example, amino-acid precursors) in ice. Because cosmic rays pervade the galaxy, even a rogue planet adrift in space would be bathed in intense radiation.

As Dimitra Atri, an astrophysicist and co-author of the new study puts it, “life might be able to survive in more places than we ever imagined”, suggesting hidden biospheres could exist in many cold, dark niches.

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