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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.

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Albert Einstein taught us that space and time belong together to a common entity: space-time. This means that time becomes a dimension, similar to space, and has profound consequences for the nature of time. Most importantly it leads to what has been called the block universe, a universe in which all moments of time exist the same way together. The future, the present, and the past are the same, it is just our perception that suggests otherwise.

Continue reading “Does the Past Still Exist?” »

NASA’s new moon rocket sprang another dangerous fuel leak Saturday, forcing launch controllers to call off their second attempt to send a crew capsule into lunar orbit with test dummies.

The first attempt earlier in the week was also marred by escaping hydrogen, but those leaks were elsewhere on the 322-foot (98-meter) rocket, the most powerful ever built by NASA.

Continue reading “Fuel leak ruins NASA’s 2nd shot at launching moon rocket” »

This “Waterworld” could reveal more about what makes a planet habitable.

NASA’s TESS satellite found a rare exoplanet covered in deep oceans, making it an excellent candidate for Webb to take a closer look at and learn more about habitability.

The new research provides a more complete picture of how diamond rain forms on other planets.

Researchers have discovered that “diamond rain,” unique precipitation that has long been speculated to occur on icy giant planets, may occur more frequently than previously believed.

To learn more about the circumstances on the icy giant planets Neptune and Uranus, a group of researchers from Germany and France has created an intriguing experiment, according to an article published by Physic.org on Friday.

Continue reading “Scientists create nanodiamonds from plastic bottles” »

A new image using data collected by NASA’s James Webb Space Telescope shows off one of the most perfect “Einstein rings” ever captured.

2nd launch attempt scrubbed.

A fuel leak forced NASA to call off its second attempt to launch the Artemis 1 moon mission on Saturday (Sept. 3).

A team of Japanese and US physicists has pushed thousands of Ytterbium atoms to just within a billionth of a degree above absolute zero to understand how matter behaves at these extreme temperatures. The approach treats the atoms as fermions, the type of particles like electrons and protons, that cannot end up in the so-called fifth state of matter at those extreme temperatures: a Bose-Einstein Condensate.

When fermions are actually cooled down, they do exhibit quantum properties in a way that we can’t simulate even with the most powerful supercomputer. These extremely cold atoms are placed in a lattice and they simulate a “Hubbard model” which is used to study the magnetic and superconductive behavior of materials, in particular the collective motion of electrons through them.

The symmetry of these models is known as the special unitary group, or, SU, and depends on the possible spin state. In the case of Ytterbium, that number is 6. Calculating the behavior of just 12 particles in a SU Hubbard model can’t be done with computers. However, as reported in Nature Physics, the team used laser cooling to reduce the temperature of 300,000 atoms to a value almost three billion times colder than the temperature of outer space.