Lifeboat Foundation

Synopsis: How can we think rigorously about the far future, and use this to guide near-term projects? In this talk I will outline my “grand futures” project of mapping the limits of what advanced civilizations can achieve – in terms of survival, expanding in space, computation, mastery over matter and energy, and so on – and how this may interact with different theories about what truly has value.

For some fun background reading, see ‘What is the upper limit of value?‘which Anders Sandberg co-authored with David Manheim.

Continue reading “Anders Sandberg — Grand Futures — Thinking Truly Long Term” »

The launch of the American space agency’s big new Moon rocket is facing a potentially lengthy delay.

The universe is a beautiful yet mysterious place. Here are 50 stunning images that will make you reconsider your existence.

A new study has estimated the chance of causalities from falling rocket parts over the next ten years.

A ‘dead’ sunspot on the surface of the Sun has erupted, and as a result, a massive plasma ball has been blasted straight towards Earth.

While Hubble can spot Jupiter’s auroras when capturing ultraviolet light, Webb’s infrared image shows the auroras in greater detail.

“I’ve never seen anything like that before,” O’Donoghue said, adding, “I can’t quite believe we’ve got that shot from such a vast distance. It really speaks to how effective JWST is at picking up faint light.”

Webb’s new images of Jupiter show two of the planet’s moons, Amalthea and Adrastea, the smaller of the two, measures just 12 miles across, according to NASA. In comparison, Hubble’s image of Jupiter shows the planet’s ocean-filled moon, Europa, which measures 1,940 miles across.

What goes on inside planets like Neptune and Uranus? To find out, an international team headed by the Helmholtz-Zentrum Dresden-Rossendorf (HZDR), the University of Rostock and France’s École Polytechnique conducted a novel experiment. They fired a laser at a thin film of simple PET plastic and investigated what happened using intensive laser flashes. One result was that the researchers were able to confirm their earlier thesis that it really does rain diamonds inside the ice giants at the periphery of our solar system. And another was that this method could establish a new way of producing nanodiamonds, which are needed, for example, for highly-sensitive quantum sensors. The group has presented its findings in the journal Science Advances.

The conditions in the interior of icy giant planets like Neptune and Uranus are extreme: temperatures reach several thousand degrees Celsius, and the pressure is millions of times greater than in the Earth’s atmosphere. Nonetheless, states like this can be simulated briefly in the lab: powerful laser flashes hit a film-like material sample, heat it up to 6,000 degrees Celsius for the blink of an eye and generate a shock wave that compresses the material for a few nanoseconds to a million times the atmospheric pressure.

“Up to now, we used hydrocarbon films for these kinds of experiment,” explains Dominik Kraus, physicist at HZDR and professor at the University of Rostock. “And we discovered that this extreme pressure produced tiny diamonds, known as nanodiamonds.”

The most massive star known by astronomers is truly of gargantuan proportions. Dubbed R136a1, this is the most massive and luminous star ever discovered in the cosmos. Additionally, it belongs to the Large Magellanic Cloud and is one of the hottest stars out there, and it is very, very different than our Sun.

Astronomers have obtained the sharpest image ever of star R136a1, the most massive known star in the Universe, with the 8.1-meter Gemini South telescope in Chile, part of the International Gemini Observatory operated by NSF’s NOIRLab. Researchers at NOIRLab, led by Venu Kalari, challenge our understanding of the most massive stars and suggest their mass may be lower than previously believed.

The formation of the biggest stars – those with 100 times the mass of the Sun – is still a mystery to astronomers. Observing these giants, which normally reside within dust-shrouded star clusters, is challenging. A giant star’s fuel reserves are depleted in less than a million years. Compared with our Sun, which has a lifespan of about 10 billion years, ours is less than halfway through. Individual massive stars in clusters are difficult to distinguish due to their densely packed nature, short lifetimes, and vast astronomical distances.

Scientists had previously theorised that extremely high pressure and temperatures turn hydrogen and carbon into solid diamonds thousands of kilometres below the surface of the ice giants.

Now new research, published in Science Advances, inserted oxygen into the mix, finding that “diamond rain” could be more common than thought.

Ice giants like Neptune and Uranus are thought to be the most common form of planet outside our Solar System, which means diamond rain could be occurring across the universe.