On 19 June 2018, a peculiar number emerged from the blockchain space. The series of numbers and letters sent the cryptosphere into overdrive, sparking rampant talk of quantum computing breakthroughs, time travel, Satoshi’s return, and the esoteric meaning of Bitcoin.
No need to be an atomic scientist, when you’re considering the state of the World today, to understand the picture is an alarming one. Allegorically-speaking, the Earth is now only two minutes away from impending catastrophe.
Observing Negative Mass at Washington State University
Negative mass has always been theoretically possible, and the concept has finally made it from a mathematical idea on paper to a reality achieved in the lab. Scientists at Washington State University have created a fluid with negative mass.
Just over a century ago, Einstein proposed the existence of waves in the spacetime continuum – the logical deduction from his Theory of General Relativity. In February 2016, scientists finally announced the detection of those “ripples” in gravity, using the technique of laser interferometry.
Erm…No. Not Mona Lisa! (Rolls eyes.) Think again!! This is LISA – the Lisa Pathfinder satellite, the key element for a grand new project: a space-based gravitational observatory.
You know how when you throw a rock into a pool, that makes ripples in the water? And how Einstein once upon a time predicted that the very mass of stars and planets should warp spacetime? Although we have had a justified inkling that Einstein was right for quite some time, we had never before detected such a phenomenon. Until THIS happened…
Already this article is beginning to sound like one of those sempiternal quizzes you so often get on social media… but it actually shows how science reality connects. Are you having a scientific identity crisis?
With his wind-swept mane, the inimitable Richard Feynman looked devilishly handsome. And he darn-diddly knew it too! As for Fritz Haber, Rosalind Franklin and Neil deGrasse Tyson, they were the original hipsters. That’s according to BuzzFeed anyway…
Marie Curie (1867-1934) – the ‘foreign student‘ who conducted pioneering research on radioactivity. She didn’t shy away from a bold pattern.
Fritz Haber (1868-1934) figured out the method used in industry to synthesise ammonia from nitrogen and hydrogen gases. Known as the Haber-Bosch process, the food production for half the World’s current population depends on this method for producing nitrogen fertilisers. So, you wouldn’t dream of taking a dig at his glasses…
Robert Oppenheimer (1904-1967) may be considered to be the “father of the atomic bomb”, but you wouldn’t think of criticising his tie.
Stylish Rosalind Franklin (1920-1958) was unravelling the mysteries of DNA structure, long before anyone even heard of DNA.
And Neil deGrasse Tyson? The only thing hotter than his facial hair are the supernovae he studied in his field of Astrophysics…
If you thought physicists weren’t known for their good dress sense, think again!
Let’s talk about size… 😉 How big are the objects floating in our Universe and how big can they get? Starting with a “big” object, our very own Moon… Embark on a tour of space… A tour of our Universe…
1/60 minute. 1/3,600 hour. 1/86,400 day. 1/1 hertz. The duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of a 133 55Cs caesium isotope corresponds to one second. But what does it look like? And where might you find a second?