Category Astronomy/Space

Scientists Recover Nova 1st Spotted 600 years ago by Korean Astrologers

This image shows the recovered nova of March 11, 1437 and its ejected shell. It was taken with the Carnegie SWOPE 1-meter telescope in Chile using a filter that highlights the hot hydrogen gas of the shell. The now-quiescent star that produced the nova shell is indicated with red tick marks; it is far from the shell's center today. However, its measured motion across the sky places it at the red '+' in 1437. The position of the center of the shell in 1437 is at the green plus sign. The agreement of the 1437 positions of the shell center and of the old nova are the 'clock' that demonstrates that the old nova of 1437 A.D. really is the source of the shell. Credit: © K. Ilkiewicz and J. Mikolajewska

This image shows the recovered nova of March 11, 1437 and its ejected shell. It was taken with the Carnegie SWOPE 1-meter telescope in Chile using a filter that highlights the hot hydrogen gas of the shell. The now-quiescent star that produced the nova shell is indicated with red tick marks; it is far from the shell’s center today. However, its measured motion across the sky places it at the red ‘+’ in 1437. The position of the center of the shell in 1437 is at the green plus sign. The agreement of the 1437 positions of the shell center and of the old nova are the ‘clock’ that demonstrates that the old nova of 1437 A.D. really is the source of the shell. Credit: © K. Ilkiewicz and J. Mikolajewska

New study proves that novae have long-term life cycle with multiple stages...

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Star-formation ‘fuel tanks’ found around Distant Galaxies

This cartoon shows how gas falling into distant starburst galaxies ends up in vast turbulent reservoirs of cool gas extending 30 000 light-years from the central regions. ALMA has been used to detect these turbulent reservoirs of cold gas surrounding similar distant starburst galaxies. By detecting CH+ for the first time in the distant Universe, this research opens up a new window of exploration into a critical epoch of star formation. Credit: ESO/L. Benassi

This cartoon shows how gas falling into distant starburst galaxies ends up in vast turbulent reservoirs of cool gas extending 30 000 light-years from the central regions. ALMA has been used to detect these turbulent reservoirs of cold gas surrounding similar distant starburst galaxies. By detecting CH+ for the first time in the distant Universe, this research opens up a new window of exploration into a critical epoch of star formation. Credit: ESO/L. Benassi

5 of 6 distant starburst galaxies were found by ALMA to be surrounded by turbulent reservoirs of hydrogen gas, the fuel for future star formation. In the early universe, brilliant starburst galaxies converted vast stores of hydrogen gas into new stars at a furious pace...

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What Lit up the Universe? Black Holes may have Punctured Darkened Galaxies, allowing light to escape

The earliest known galaxies in the universe. Some of these galaxies formed just 600 million years after the Big Bang. Credit: ESA/NASA

The earliest known galaxies in the universe. Some of these galaxies formed just 600 million years after the Big Bang. Credit: ESA/NASA

Soon after the Big Bang, the universe went completely dark. The intense, seminal event that created the cosmos churned up so much hot, thick gas that light was completely trapped. Much later – perhaps as many as one billion years after the Big Bang -the universe expanded, became more transparent, and eventually filled up with galaxies, planets, stars, and other objects that give off visible light. That’s the universe we know today. How it emerged from the cosmic dark ages to a clearer, light-filled state remains a mystery.

In a new study, researchers at the University of Iowa offer a theory of how that happened...

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Artificial Intelligence Analyzes Gravitational Lenses 10 million Times Faster

Neural Nets and Gravitational Lenses

KIPAC scientists have for the first time used artificial neural networks to analyze complex distortions in spacetime, called gravitational lenses, demonstrating that the method is 10 million times faster than traditional analyses. (Greg Stewart/SLAC National Accelerator Laboratory)

Brain-mimicking ‘neural networks’ can revolutionize the way astrophysicists analyze their most complex data. Researchers from the Department of Energy’s SLAC National Accelerator Laboratory and Stanford University have for the first time shown that neural networks – a form of artificial intelligence — can accurately analyze the complex distortions in spacetime known as gravitational lenses 10 million times faster than traditional methods...

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