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First Direct Image of Protoplanet Swirling Surrounding Gas
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First Direct Image of Protoplanet Swirling Surrounding Gas

The formation and evolution of planets is the driving force behind both where and how we might find life beyond Earth. This complex and lengthy process first begins with a massive ball of gas and dust that swirls until it flattens into a disk, followed by rocks ranging in size from pebbles to kilometer-scale objects clumping together in a process known as accretion, as they too swirl around within the larger disk and form rocky planets closer to the star and the farther out planets collect the gas, ice, and dust that the star couldn’t evaporate. Until now, researchers have been limited to visualizing the swirling gas and dust forming planets through computer models.

Coldest Lava Exoplanet Found to Hold an Atmosphere
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Coldest Lava Exoplanet Found to Hold an Atmosphere

Exoplanets continue to challenge our understanding of planetary formation, evolution, and whether they might be able to support life as we know it. Scientists often use planets in our solar system as analogs for exoplanets, studying exoplanets with extremely short orbital periods forces scientists to constantly rethink our understanding of what planets can withstand during their lifetimes. One such type of exoplanet that has entered the foray in recent years are “lava world” exoplanets, and especially lava exoplanets that orbit dangerously close to their stars. But while it has been long known that lava worlds on with higher temperatures have atmospheres, “colder” lava worlds have been found to lack atmospheres.

Watch Plasma Erupt in Full Color Inside a Fusion Reactor at 16,000 FPS
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Watch Plasma Erupt in Full Color Inside a Fusion Reactor at 16,000 FPS

The glow of deuterium and lithium inside Tokamak Energy's ST40 fusion reactor. (Tokamak Energy/YouTube) Look at this spectacular nonsense.ScienceAlert stories are written, fact-checked, and edited by humans, never generated by AI. Don't miss a story, subscribe here.

Science Says Who You Eat Dinner With Matters as Much as What's on Your Plate
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Science Says Who You Eat Dinner With Matters as Much as What's on Your Plate

(urbazon/E+/Getty Images) We are social creatures.ScienceAlert stories are written, fact-checked, and edited by humans, never generated by AI. Don't miss a story, subscribe here.

CHIME telescope unlocks new way to study the universe's bafflign expansion
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CHIME telescope unlocks new way to study the universe's bafflign expansion

Scientists have a new tool for mapping the universe's perplexing acceleration.A Canadian telescope designed to chart the distribution of hydrogen gas across the ancient universe has proved it can do so using only its own data for the first time, without the help of other telescopes. The results took seven years to prove, but the payoff could be huge. According to the authors of a new study published Monday (Sept. 28) in The Astrophysical Journal, the telescope could give scientists a new, cost-effective way to study dark energy, the poorly understood force that is causing the universe to expand at an accelerating rate over time."Hydrogen is the most common element in the universe and the raw material from which stars form," study co-author Arnab Chakraborty, a postdoctoral fellow at the University of Toronto, said in a statement. "Its faint radio emission acts like a cosmic tracer, revealing how matter is distributed across space." The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a set of radio telescopes, principally located near Penticton, British Columbia, that map the entire northern sky every day. Before the results from the new study, CHIME had to confirm its own observations with other telescopes — an expensive and time-consuming process. It was important for CHIME to look at the universe's ancient hydrogen gas with its own data, to serve as an independent point of measurement that did not rely on other telescopes, the team explained. The new paper, which was nearly a decade in the making, is based on 94 nights of observations in 2019 that were carefully double-checked before publication. The telescope can detect radio signals as far back as 3 billion years after the Big Bang, when the universe was a fraction of its current age.Related storiesJames Webb telescope traces origin of brightest fast radio burst ever detectedScientists discover fast-spinning 'unicorn' object that defies physicsScientists Have Discovered a Mysterious Repeating Radio Signal from Deep Space"We worked very hard to convince ourselves that this wasn't a false alarm," Chakraborty said. "After all the tests, the signal remained. That gave us confidence we were seeing real hydrogen from the distant universe." An accompanying paper published in The Astrophysical Journal includes more information about where hydrogen is found in the cosmos. This study suggests that about 2% of hydrogen is "neutrally atomic" — meaning the atoms contain a balance of just one proton and one electron, resulting in no overall electric charge — which is "broadly consistent" with measurements by other telescopes, Shabbir Shaikh, a postdoctoral fellow in the School of Earth and Space Exploration at Arizona State University and a co-author of both papers, said in the statement.Mapping the distribution of this common gas could reveal new clues about the expansion of the universe at different times in cosmic history. In future research, the team plans to go through CHIME's other seven years of observations to gather more information about its hydrogen gas studies.