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It’s a fantastic comic that holds up well as a story for a number of reasons. It’s cyberpunk without the genre’s trademark dinge: Robertson, Ramos, and colorist Nathan Eyring deserve a lot of credit for making a future packed with information overload, but not obscured by smog or gloom or perpetual rain. It’s also genuinely funny. Angry Warren Ellis is gifted at turning the combination of rage, foul language, and body parts into something beautiful. It’s also appropriately cynical, and I think this is where a lot of the comparisons to the present day come from.


Holy mother of God, Transmet is over 20 years old. But is it still sharp commentary, or a relic of its time?

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How large is a neutron star? Previous estimates varied from eight to 16 kilometres. Astrophysicists at the Goethe University Frankfurt and the FIAS have now succeeded in determining the size of neutron stars to within 1.5 kilometres by using an elaborate statistical approach supported by data from the measurement of gravitational waves. The researchers’ report appears in the current issue of Physical Review Letters.

Neutron are the densest objects in the universe, with a mass larger than that of our sun compacted into a relatively small sphere whose diameter is comparable to that of the city of Frankfurt. This is actually just a rough estimate, however. For more than 40 years, the determination of the size of has been a holy grail in nuclear physics whose solution would provide important information on the fundamental behaviour of at nuclear densities.

The data from the detection of from merging stars (GW170817) make an important contribution toward solving this puzzle. At the end of 2017, Professor Luciano Rezzolla, Institute for Theoretical Physics at the Goethe University Frankfurt and FIAS, together with his students Elias Most and Lukas Weih already exploited this data to answer a long-standing question about the maximum mass that neutron stars can support before collapsing to a black hole—a result that was also confirmed by various other groups around the world. Following this first important result, the same team, with the help of Professor Juergen Schaffner-Bielich, has worked to set tighter constraints on the size of neutron stars.

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Sending stuff up to space is no easy task — even 45 years after Apollo 11. Size, weight, and cost are all massively important, so some researchers are turning to advanced origami to fold up solar arrays. The result of their two years’ worth of work is a solar array with a diameter of just 8.9 feet (2.7 meters) when folded and a massive 82 feet (25 meters) when unfurled. A 1/20th scale model of the array is what you see here.

To build the solar array, Shannon Zirbel and professor Larry Howell of Brigham Young University, and mechanical engineer Brian Trease of NASA’s Jet Propulsion Laboratory, enlisted the help of renowned origami expert Robert Lang. One of the major difficulties faced by the team is that solar arrays are not as thin as paper. “You have to rethink a lot of that design in order to accommodate the thickness that starts to accumulate with each bend,” Trease said in a press release.

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Today we have a report from Open Longevity School: Summer Camp 2018, an initiative in Russia focused on developing a personal health and longevity strategy, Elena Milova went to investigate.


When we ask researchers when, in their opinion, the cures for aging will be ready, we often hear an optimistic answer: 20–25 years. As a well-informed optimist, I add another 10 years to this number, because wherever the therapies appear, it will take time for them to be distributed to other countries and become affordable. I will be happy if it takes less time, but what if it doesn’t? I am nearly 40, and when I add 35 years to my current age, I vividly imagine how my reflection in the mirror will show a 75-year-old lady. Honestly, I don’t want to see my body change, and it can explain why I aspire to get first-hand information about any means to slow down aging as soon as possible. Evidence-based information, of course.

Before I tell you my story of discovering how to control my aging, I must provide a disclaimer. This article does not contain any medical recommendations. The websites of the projects I will tell you about, once again, do not contain medical recommendations and cannot be independently used to make health decisions. The experience I will share, and the activities of the projects I will tell you about, are aimed at teaching you about the existing scientific knowledge about aging and interventions that have the potential to change the way we age. Whatever you decide to implement in your everyday life, please talk to your medical advisor first.

I am always looking for the means to keep myself as young as possible. Luckily for me, in Russia, there is a project focused on collecting this kind of information and making it publicly available. It is Nestarenie.ru (translation: “not aging”), an online encyclopedia created by professional sports trainer, valeologist and citizen scientist Dmitry Veremeenko. The amount of information that Dmitry has managed to process is hard to imagine; it consists of more than 70,000 scientific papers. The development of this database took him several years of work. Each article of his encyclopedia summarizes a specific drug, food or lifestyle element that can slow down or even reverse age-related changes, with a deep explanation of the underlying mechanisms. Each of his information-dense articles has lots of internal links to actual scientific papers (including the freshest meta-analyses) and finishes with a list of additional references.

In a breakthrough discovery, University of Wollongong (UOW) researchers have created a “heartbeat” effect in liquid metal, causing the metal to pulse rhythmically in a manner similar to a beating heart.

Their findings are published in the 11 July issue of Physical Review Letters, the world’s premier journal for fundamental physics research.

The researchers produced the heartbeat by electrochemically stimulating a drop of liquid gallium, causing it to oscillate in a regular and predictable manner. Gallium (Ga) is a soft silvery metal with a low melting point, becoming liquid at temperatures greater than 29.7C.

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