Category Astronomy/Space

Radio signal from the very early universe offers clues about the first stars

The image shows a deep galaxy field, featuring thousands of galaxies of various shapes and sizes

Understanding how the universe transitioned from darkness to light with the formation of the first stars and galaxies is a key turning point in the universe’s development, known as the Cosmic Dawn. However, even with the most powerful telescopes, we can’t directly observe these earliest stars, so determining their properties is one of the biggest challenges in astronomy.

Now, an international group of astronomers led by the University of Cambridge has shown that we will be able to learn about the masses of the earliest stars by studying a specific radio signal—created by hydrogen atoms filling the gaps between star-forming regions—originating just a hundred million years after the Big Bang.

By studying how the first stars and their remnants affected this signal, called the 2...

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The solar system’s greatest mystery may finally be solved

Artist's impression of Planet Nine as an ice giant eclipsing the central Milky Way, with a star-like Sun in the distance. Neptune's orbit is shown as a small ellipse around the Sun. (Credit : Nagual Design)
Artist’s impression of Planet Nine as an ice giant eclipsing the central Milky Way, with a star-like Sun in the distance. Neptune’s orbit is shown as a small ellipse around the Sun. (Credit : Nagual Design)

For years, astronomers have been searching for a mysterious ninth planet lurking in the dark outer reaches of our solar system. Now, a team of researchers have taken a completely different approach to this cosmic detective story—instead of looking for reflected sunlight, they’re hunting for the planet’s own heat signature.

The story begins with a puzzle in the outer solar system. Scientists noticed that small icy bodies called Kuiper Belt Objects, which orbit far beyond Neptune, seem to be clustered together in unusual ways...

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Surprising discovery shows a strong link between Earth’s magnetic field and atmospheric oxygen levels

Every breath we take in contains 21% oxygen, the gas that makes life on Earth possible. Oxygen, in its combined oxide state, has always been abundant in Earth’s crust, but elemental diatomic oxygen became part of our atmosphere around 2.4 to 2.5 billion years ago as a gift from cyanobacteria, which triggered the Great Oxidation Event and breathed life into Earth.

A joint venture between NASA Goddard Space Flight Center and the University of Leeds discovered that the Earth’s magnetic field strength and atmospheric oxygen levels over the past 540 years have seemed to spike and dip at the same time, showing a strong, statistically significant correlation between the two.

This correlation could arise from unexpected connections between geophysical processes in Earth’s deep interior,...

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Exploring late accretion’s role in terrestrial planet evolution


Media Title
High-energy Venus Impacts

Southwest Research Institute has collaborated with Yale University to summarize the scientific community’s notable progress in advancing the understanding of the formation and evolution of the inner rocky planets, the so-called terrestrial planets. Their paper focuses on late accretion’s role in the long-term evolution of terrestrial planets, including their distinct geophysical and chemical properties as well as their potential habitability.

The Review paper is published in the journal Nature.

Solar systems form when clouds of gas and dust begin to coalesce. Gravity pulls these elements together, forming a central star, like our sun, surrounded by a flattened disk of consolidating materials...

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