GlaxoSmithKline Plc is exploring the trillions of microbes that inhabit the gut in pursuit of novel ways to prevent some of the world’s most common ailments.
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There’s battle lines being drawn.
Nobody’s right if everybody’s wrong.
Young people speaking their minds
Getting so much resistance from behind
It’s time we stop, hey, what’s that sound.
Everybody look what’s going down ”
Deep Knowledge Group is delighted to have supported and participated in the landmark International Longevity Policy and Governance and AI for Longevity Summits that took place on November 12th at King’s College London, which gathered an unprecedented density and diversity of speakers and panelists at the intersection of Longevity, AI, Policy and Finance. The summits were organized by Longevity International UK and the AI Longevity Consortium at King’s College London, with the strategic support of Deep Knowledge Group, Aging Analytics Agency, Ageing Research at King’s (ARK) and the Biogerontology Research Foundation. Together they managed to attract the interest of major financial corporations, insurance companies, investment banks, Pharma and Tech corporations, and representatives of international governmental bodies, organisations and embassies, as well as leading media, and featured presentations and panel discussions from top executives and directors of Prudential, Barclays Business UK, HSBC, AXA, L&G, Longevity. Capital, Longevity Vision Fund, Juvenescence, the UK Office of AI, Microsoft, NVIDIA, Babylon Health, Huawei Europe, Insilico Medicine, Longevity International UK, the Longevity AI Consortium and others.
November 14, 2019, London, UK: Deep Knowledge Group executives Dmitry Kaminksiy and Eric Kihlstrom spoke at a landmark one-day event held yesterday at King’s College London with the strategic support Deep Knowledge Group. The event united two Longevity-themed summits under the shared strategic agenda of enabling a paradigm shift from treatment to prevention and from prevention to Precision Health via the synergistic efforts of science, industry, AI, policy and governance, to enable the UK to become an international leader in Healthy Longevity.
Earlier today, Genevieve O’Hagan updated Lifeboat readers on this week’s momentous event in Astronomy. At least, I find it fascinating—and so, I wish to add perspective…
30 years ago, astronomer Jack Hills demonstrated the math behind what has become known as the “Hills Mechanism”. Until this week, the event that he described had never been observed.* But his peer astronomers agreed that the physics and math should make it possible…
Hills explained that under these conditions, a star might be accelerated to incredible speeds — and might be even flung out of its galaxy:
If conditions are right, one star ends up orbiting the back hole while the other is jettisoned at incredible speed, yet holding onto its mass and shape. All that energy comes from the gravity of the black hole and the former momentum of the captured star. [20 sec animation] [continue below]
This week, astronomers found clear evidence of this amazing event and traced it back to our galactic center: Five million years ago — as our ancestors learned to walk upright — a star that passed close to the massive black hole at The Milky Way center was flung away at a staggering 6 million Kmh. It is traveling so fast, that it is no longer bound to our galaxy or galactic cluster. It is headed out of the galaxy.
Footage has since emerged capturing the US Space Force craft “following” the astronauts in the sky, conspiracists have claimed.
Neutron stars cannot exist.
“The sky was clear—remarkably clear—and the twinkling of all the stars seemed to be but throbs of one body, timed by a common pulse.” —Thomas Hardy.
On June 13, 2012 NASA launched the Nuclear Spectroscopic Telescope Array (NuSTAR) on a mission to study X-rays in what are thought to be the remnants of supernova explosions, called pulsars. NuStar joins other X-ray space telescopes like Chandra and XMM-Newton, except that it is capable of focusing X-rays to a sharp point, enabling it to “see” energies up to 79,000 electron-volts. That capability makes it more than 100 times more powerful than the other observatories.
