Category Astronomy/Space

Galactic Archaeology

‘Galactic archaeology’ refers to the study of second generation stars to learn about the physical characteristics of the first stars, which disappeared only tens of millions of years after the Big Bang. A computational physics study modeled for the first time faint supernovae of metal-free first stars, yielding carbon-enhanced abundance patterns for star formation. Slice of density, temperature, and carbon abundance for a 13 solar mass progenitor model at times (left-right) 0.41, 15.22, and 29.16 million years after the supernovae explosion in a box with a side 2 kpc. Credit: Chiaki, et al.

Supercomputers dig into first star fossils...

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ALMA shows Volcanic Impact on Io’s Atmosphere

Credit: ALMA (ESO/NAOJ/NRAO), I. de Pater et al.; NRAO/AUI NSF, S. Dagnello; NASA/JPL/Space Science Institute

New radio images from the Atacama Large Millimeter/submillimeter Array (ALMA) show for the first time the direct effect of volcanic activity on the atmosphere of Jupiter’s moon Io.

Io is the most volcanically active moon in our solar system. It hosts more than 400 active volcanoes, spewing out sulfur gases that give Io its yellow-white-orange-red colors when they freeze out on its surface.

Although it is extremely thin — about a billion times thinner than Earth’s atmosphere — Io has an atmosphere that can teach us about Io’s volcanic activity and provide us a window into the exotic moon’s interior and what is happening below its colorful crust.

Previous research has sh...

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Ultraviolet shines light on Origins of the Solar System

Artist rendition of the protosun and the solar nebula. Oxygen isotopes can be altered by ultraviolet light (gold arrows). Short-lived radiogenic isotopes of aluminum (maroon wavy arrows) may also have been injected into the solar nebula. Insets: electron backscatter images from calcium-aluminum inclusions and the approximate location at which these high-temperature condensates formed.

Credit: NASA JPL-Caltech/Lyons/ASU

In the search to discover the origins of our solar system, an international team including planetary scientists has compared the composition of the sun to the composition of the most ancient materials that formed in our solar system: refractory inclusions in unmetamorphosed meteorites.

By analyzing the oxygen isotopes (varieties of an element that have some extra neutr...

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Evidence of Broadside Collision with Dwarf Galaxy discovered in Milky Way

The Milky Way’s Shell Structure Reveals the Time of a Radial Collision
Thomas Donlon II, Heidi Jo Newberg, Robyn Sanderson, Lawrence M. Widrow

‘Shell structures’ are first of their kind found in the galaxy. Nearly 3 billion years ago, a dwarf galaxy plunged into the center of the Milky Way and was ripped apart by the gravitational forces of the collision. Astrophysicists announced today that the merger produced a series of telltale shell-like formations of stars in the vicinity of the Virgo constellation, the first such “shell structures” to be found in the Milky Way. The finding offers further evidence of the ancient event, and new possible explanations for other phenomena in the galaxy.

Astronomers identified an unusually high density of stars called the Virgo Overdensity about ...

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