Life on Venus? Intriguing molecule phosphine spotted in planet’s clouds again

The Venus phosphine saga continues.

In September 2020, a team of scientists led by Jane Greaves of Cardiff University in Wales reported the detection of phosphine, a possible indicator of life, in the clouds of Venus. The announcement sparked a heated debate and a surge of follow-up studies, which have generally failed to spot the intriguing molecule in the Venusian atmosphere. 

Now there’s a new twist. Speaking at the Royal Astronomical Society’s National Astronomy Meeting 2023 in Cardiff this week, Greaves revealed the discovery of phosphine deeper in the atmosphere of Venus than it had been spotted before. Using the James Clark Maxwell Telescope (JCMT) at the Mauna Kea Observatory in Hawaii, Greaves and her colleagues delved into the atmosphere of Venus, down to the top and even the middle of the planet’s clouds. 

The unions of Hollywood are trying to save it from itself

Fran Drescher, SAG-AFTRA president and the creator of the iconic Fran Fine, stepped up to the microphone, vibrating with fury. She was there with a small group of SAG-AFTRA members to announce their first strike since 1980. “The eyes of the world and particularly the eyes of labor are upon us,” Drescher said. “The gravity of this move is not lost on me, or our negotiating committee, or our board members who have voted unanimously to proceed with a strike.”

This strike is different. It’s far more complicated than just wanting a bigger cut of the hit films and TV shows that actors and writers helped create. A rapid shift toward streaming — coupled with the existential threat posed by AI — has created a canyon between what Hollywood writers and actors want and what the country’s largest media companies are willing to give. As Drescher so bluntly puts it: “You cannot change the business model as much as it has changed and not expect the contract to change too.”

Cheops shows scorching exoplanet acts like a mirror

Data from ESA’s exoplanet mission Cheops has led to the surprising revelation that an ultra-hot exoplanet that orbits its host star in less than a day is covered by reflective clouds of metal, making it the shiniest exoplanet ever found.

STEREO-A Comes Home

STEREO-A is coming home in the summer of 2023 for the first time since it was launched 17 years ago and is providing amateur astronomers with a unique opportunity to do some citizen science. The spacecraft has inferior conjunction with Earth on August 17, 2023 and will be approximately 8.2 million kilometres distant then. While still far from Earth, STEREO-A will be unusually close to Earth and produce a unique opportunity to decode its deep space beacon and view stunning images of the Sun as it approaches solar maximum. In solving this riddle in the sky we present how we figured out how to decode STEREO-A’s images and present a suggestion of how to celebrate STEREO-A’s return to the vicinity of home.

Monster gravitational waves spotted for first time

Gravitational waves are back, and they’re bigger than ever.

After the historic first detection of the space-time rattles in 2015 using ground-based detectors, researchers could have now rediscovered Albert Einstein’s waves with an entirely different technique. The approach tracks changes in the distances between Earth and beacon stars in its Galactic neighbourhood called pulsars, which reveal how the space in between is stretched and squeezed by the passage of gravitational waves.

Whereas the original discovery spotted waves originating from the collision and merger of two star-sized black holes, the most likely source of the latest finding is the combined signal from many pairs of much larger black holes — millions or even billions of times the mass of the Sun — slowly orbiting each other in the hearts of distant galaxies. These waves are thousands of times stronger and longer than those found in 2015, with wavelengths of up to tens of light years. By contrast, the ripples detected since 2015 using a technique called interferometry are just tens or hundreds of kilometres long.

Detecting disparities in police deployments using dashcam data

Large-scale policing data is vital for detecting inequity in police behavior and policing algorithms. However, one important type of policing data remains largely unavailable within the United States: aggregated police deployment data capturing which neighborhoods have the heaviest police presences. Here we show that disparities in police deployment levels can be quantified by detecting police vehicles in dashcam images of public street scenes. Using a dataset of 24,803,854 dashcam images from rideshare drivers in New York City, we find that police vehicles can be detected with high accuracy (average precision 0.82, AUC 0.99) and identify 233,596 images which contain police vehicles. There is substantial inequality across neighborhoods in police vehicle deployment levels. The neighborhood with the highest deployment levels has almost 20 times higher levels than the neighborhood with the lowest. Two strikingly different types of areas experience high police vehicle deployments — 1) dense, higher-income, commercial areas and 2) lower-income neighborhoods with higher proportions of Black and Hispanic residents. We discuss the implications of these disparities for policing equity and for algorithms trained on policing data.

M20, the Trifid Nebula, using data processed from a remotely accessible telescope in Chile.