heavy elements tagged posts

Astronomers Discover Heavy Elements after Bright Gamma-Ray Burst from Neutron Star Merger

An artist illustration of a merger of two neutron stars that create heavy elements.
Illustration courtesy of Luciano Rezzolla, University of Frankfurt, Germany

Breakthrough discovery puts astronomers one step closer to solving the mystery of the origin of elements that are heavier than iron. An international team of astronomers — including Clemson University astrophysicist Dieter Hartmann — obtained observational evidence for the creation of rare heavy elements in the aftermath of a cataclysmic explosion triggered by the merger of two neutron stars.

The massive explosion unleashed a gamma-ray burst, GRB230307A, the second brightest in 50 years of observations and about 1,000 times brighter than a typical gamma-ray burst. GRB230307A was first detected by NASA’s Fermi Gamma-Ray Space Telescope on March 7, 2023.

Using multiple space- and ground-based telescopes, in...

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Metal-poor Stars are more Life-friendly

A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighborhood.

Stars that contain comparatively large amounts of heavy elements provide less favourable conditions for the emergence of complex life than metal-poor stars, as scientists from the Max Planck Institutes for Solar System Research and for Chemistry as well as from the University of Göttingen have now found. The team showed how the metallicity of a star is connected to the ability of its planets to surround themselves with a protective ozone layer. Crucial to this is the intensity of the ultraviolet light that the star emits into space, in different wavelength ranges...

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Neutron Star Collisions are ‘Goldmine’ of Heavy Elements, study finds

Illustration shows two white cloud-like structures spiraling together to form a sphere circled by a ring of smaller gold particles

Mergers between two neutron stars have produced more heavy elements in last 2.5 billion years than mergers between neutron stars and black holes. Most elements lighter than iron are forged in the cores of stars. A star’s white-hot center fuels the fusion of protons, squeezing them together to build progressively heavier elements. But beyond iron, scientists have puzzled over what could give rise to gold, platinum, and the rest of the universe’s heavy elements, whose formation requires more energy than a star can muster.

A new study by researchers at MIT and the University of New Hampshire finds that of two long-suspected sources of heavy metals, one is more of a goldmine than the other.

The study, published today in Astrophysical Journal Letters, reports that in the last 2...

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Special Star is a Rosetta Stone for Understanding the Sun’s Variability and Climate Effect

Image of our sun showing dark sunspots and bright diffuse faculae (best seen around the edges). A new study shows how the larger mix of heavy elements leave such spots unchanged, while increasing the contrast of the bright diffuse faculae. Credit: NASA/SDO

Image of our sun showing dark sunspots and bright diffuse faculae (best seen around the edges). A new study shows how the larger mix of heavy elements leave such spots unchanged, while increasing the contrast of the bright diffuse faculae. Credit: NASA/SDO

The spots on the surface on the Sun come and go with an 11-year periodicity known as the solar cycle. The solar cycle is driven by the solar dynamo, which is an interplay between magnetic fields, convection and rotation. However, our understanding of the physics underlying the solar dynamo is far from complete. One example is the Maunder Minimum, a period in the 17th century, where spots almost disappeared from the surface of the Sun for a period of over 50 years.

Now, a large international team has found a star that can help shed light ...

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