Category Astronomy/Space

Numerical Simulations of Planetesimal Formation Reproduce Key Properties of Asteroids, Comets

Numerical simulations of planetesimal formation reproduce key properties of asteroids, comets
Comparison between the predictions by Polak and Klahr for the mass distribution of asteroids (red circles), compared with observations (white circles). The horizontal axis shows the size of the asteroids in question, and the vertical axis shows the fraction of the total mass of the pebble cloud that ends up in asteroids larger or equal to the chosen size value. If the total mass were to end up in a single asteroid, that asteroid would have been 152 km in diameter. Both in the prediction and according to the observations, 84% of the total asteroid mass ends up in objects between 90 km and 152 km in diameter. Overall, the primordial asteroids follow a normal (Gaussian) distribution (blue line) in mass with a most likely size of 125 km...
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The Bubbling Universe: A previously unknown Phase Transition in the Early Universe

The bubbling universe: A previously unknown phase transition in the early universe
AI generated illustration of colliding bubbles in early universe. Credit: Birgitte Svennevig, University of Southern Denmark

What happened shortly after the universe was born in the Big Bang and began to expand? Bubbles occurred and a previously unknown phase transition happened, according to particle physicists.

Think of bringing a pot of water to the boil: As the temperature reaches the boiling point, bubbles form in the water, burst and evaporate as the water boils. This continues until there is no more water changing phase from liquid to steam.

This is roughly the idea of what happened in the very early universe, right after the Big Bang, 13.7 billion years ago.

The idea comes from particle physicists Martin S...

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Evidence that Saturn’s moon Mimas is a Stealth Ocean World

Saturn moon Mimas and a graph of two options of its geology
Courtesy of NASA/JPL/SSI/SwRI

Simulations suggest that Saturn’s smallest, innermost moon could have an expanding, geologically young ocean. When a Southwest Research Institute scientist discovered surprising evidence that Saturn’s smallest, innermost moon could generate the right amount of heat to support a liquid internal ocean, colleagues began studying Mimas’ surface to understand how its interior may have evolved. Numerical simulations of the moon’s Herschel impact basin, the most striking feature on its heavily cratered surface, determined that the basin’s structure and the lack of tectonics on Mimas are compatible with a thinning ice shell and geologically young ocean.

“In the waning days of NASA’s Cassini mission to Saturn, the spacecraft identified a curious libration, or os...

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Scientists release newly Accurate Map of all the Matter in the Universe

Two views of the sky side-by-side with dark and lighter spots
By comparing maps of the sky from the Dark Energy Survey telescope (at left) with data from the South Pole Telescope and the Planck satellite (at right), the team could infer how the matter is distributed.
Image courtesy Yuuki Omori

Analysis combines Dark Energy Survey, South Pole Telescope data to understand evolution of universe. A group of scientists have released one of the most precise measurements ever made of how matter is distributed across the universe.

When the universe began, matter was flung outward and gradually formed the planets, stars and galaxies that we know and love today. By carefully assembling a map of that matter today, scientists can try to understand the forces that shaped the evolution of the universe.

A group of scientists, including several with the Uni...

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