Category Astronomy/Space

Black Hole team discovers path to Razor-sharp Black Hole Images

George Wong (UIUC) and Michael Johnson (CfA)The image of a black hole has a bright ring of emission surrounding a “shadow” cast by the black hole. This ring is composed of a stack of increasingly sharp subrings that correspond to the number of orbits that photons took around the black hole before reaching the observer.

A team of researchers have published new calculations that predict a striking and intricate substructure within black hole images from extreme gravitational light bending. Last April, the Event Horizon Telescope (EHT) sparked international excitement when it unveiled the first image of a black hole...

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Turbulent Convection at the Heart of Stellar Activity

A look into the interior of the Sun and a more evolved giant star.
© MPS / Aalto University / hormesdesign.de

Different stars can exhibit different levels of activity. The Sun’s signs of solar activity are rather feeble on an astronomical scale. Other stars are up to ten times more active. While researchers have identified the magnetic fields generated in the interior of stars in a dynamo process as drivers of activity, the exact workings of this dynamo are unclear. Scientists now find that a common, turbulence-dependent dynamo mechanism plays a crucial role for stellar activity in all stages of stellar evolution.

In their interiors, stars are structured in a layered, onion-like fashion. In those with solar-like temperatures, the core is followed by the radiation zone...

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‘Strange’ Glimpse into Neutron Stars and Symmetry Violation

Inner vertex components of the STAR detector at the Relativistic Heavy Ion Collider (righthand view) allow scientists to trace tracks from triplets of decay particles picked up in the detector’s outer regions (left) to their origin in a rare “antihypertriton” particle that decays just outside the collision zone. Measurements of the momentum and known mass of the decay products (a pi+ meson, antiproton, and antideuteron) can then be used to calculate the mass and binding energy of the parent particle. Doing the same for the hypertriton (which decays into different “daughter” particles) allows precision comparisons of these matter and antimatter varieties.

New results from precision particle detectors at the Relativistic Heavy Ion Collider (RHIC) offer a fresh glimpse of the particle...

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Exoplanet where it Rains Iron discovered

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Artist’s impression of the night side of WASP-76b

Researchers using ESO’s Very Large Telescope (VLT) have observed an extreme planet where they suspect it rains iron. The ultra-hot giant exoplanet has a day side where temperatures climb above 2400 degrees Celsius, high enough to vaporise metals. Strong winds carry iron vapour to the cooler night side where it condenses into iron droplets.

“One could say that this planet gets rainy in the evening, except it rains iron,” says David Ehrenreich, a professor at the University of Geneva in Switzerland. He led a study, published today in the journal Nature, of this exotic exoplanet. Known as WASP-76b, it is located some 640 light-years away in the constellation of Pisces.

This strange phenomenon happens because the ‘iron rain’ plane...

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