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David Goggins
Former Navy Seal
Career Development
Bryan Cranston
Actor
Critical Thinking
Liv Boeree
International Poker Champion
Emotional Intelligence
Amaryllis Fox
Former CIA Clandestine Operative
Management
Chris Hadfield
Retired Canadian Astronaut & Author
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A new perfume can help you smell like an astronaut

Ever want to smell like a spacesuit? Now you can!

A bottle of Eau De Space

Eau De Space
  • After years of trying, a group has produced the smell of outer space in a perfume.
  • Astronauts have described the smell of space as similar to "ozone," "gunpowder," and "fried steak."
  • Exactly what causes the scent is still debated.
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The “new normal” paradox: What COVID-19 has revealed about higher education

Higher education faces challenges that are unlike any other industry. What path will ASU, and universities like ASU, take in a post-COVID world?

Photo: Luis Robayo/AFP via Getty Images
Sponsored by Charles Koch Foundation
  • Everywhere you turn, the idea that coronavirus has brought on a "new normal" is present and true. But for higher education, COVID-19 exposes a long list of pernicious old problems more than it presents new problems.
  • It was widely known, yet ignored, that digital instruction must be embraced. When combined with traditional, in-person teaching, it can enhance student learning outcomes at scale.
  • COVID-19 has forced institutions to understand that far too many higher education outcomes are determined by a student's family income, and in the context of COVID-19 this means that lower-income students, first-generation students and students of color will be disproportionately afflicted.
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Humanity’s impact is monkeying with animals’ evolution

Animals are adapting all the time these days to stay out of our way.

Image source: Sergei Mironenko/Shutterstock
  • If you don't want to get poached, try losing that trunk.
  • Pollution determines which moths dominate the tree trunks of the U.K.
  • More animals are becoming night owls.

We often think of evolution as taking place over extended periods of time as mutations prove themselves advantageous, or not. Mutations, though, are not rare things: They happen all the time. Scientists estimate that there were 37 trillion of them in your own body just over the last 24 hours. (It's amazing more things don't go wrong, right?) The characteristics we see in ourselves and other organisms are merely the latest winners in a wild and woolly mutation free-for-all competition, in which nature, or random chance, tries out many, many wonderful, bizarre, and ridiculous traits as things settle out over the long term.

Adaptations in response to changing environmental factors occur all the time, too: An attribute that may have been meaningless before may suddenly become very helpful. Here in the Anthropocene, animals are adapting to all sort of habitat changes we've imposed on them. While not yet long-term changes, necessarily, these characteristics suggest we may be having a considerable impact on the ongoing process of evolution in the world's organisms.

Industrialized moths

Image source: Marek R. Swadzba/Shutterstock

Before the Industrial Revolution got up and running in the U.K., light-colored pepper moths, Biston betularia morpha typica, were a common sight. However, by about 1864, they'd been essentially replaced by a darker pepper-moth cousin, Biston betularia morpha carbonaria. Why?

Pollutants — mostly coal soot —covered the British countryside, darkening its trees. Worse, sulfur dioxide emissions wiped out many of the trees' lichen and moss coverings. Against these darkened backdrops, light-colored pepper moths became far too easy to spot by predators. Better suited were the darker pepper moths, which soon came to dominate the habitat — by 1895, some 98% of pepper moths spotted were the darker variety.

Fortunately, the Industrial Revolution days passed, with dirty factories over time being replaced by cleaner alternatives, and today, the ligh-colored pepper moths are back on top.

The story is a pretty fast-paced and dramatic example of how extreme our impact can be, and also — and there's a hopeful feeling to this — how short- lived it can be if we fix what we've broken.

Foxy

Urban vs. rural red fox skull measurements

Image source: K.J. Parsons, et al

NAs investigations continue apace into what, exactly, the fox says, researchers published in June a really interesting study regarding a surprising way in which foxes are adapt to life in human-dominated urban environments.

An examination of 111 red fox skulls from London, UK, revealed "urban individuals tending to have shorter and wider muzzles relative to rural individuals."Essentially, the more urban a fox's environment is, the shorter was its snout likely to be. The change may be considered an example of Darwin's "domestication syndrome," as Big Think has reported.

The study suggests it's all about the biomechanics benefits imparted by such a change:

"Firstly, a shorter snout, as found in urban foxes, should confer a higher mechanical advantage but with reduced closing speed of the jaw. This may be advantageous in an urban habitat where resources are more likely to be accessed as stationary patches of discarded human foods. Furthermore, in some cases, these foods may require a greater force to access them, explaining the expanded sagittal crest in skulls of urban foxes."

If these traits make an individual fox better suited to its city life, it's that much more likely to survive and reproduce than a longer-snouted competitor.

Nighttime on human Earth

Image source: Viktor Grishchenko/Shutterstock

Obviously, habitat loss is the single most destructive thing we're doing to animals. It can lead to utter displacement and death, and it can also change the way animals go about doing the things they need to do to survive.

In many cases, animals dealing with fresh human encroachment bend before they break, and some are trying to carry on around us, so to speak. A 2018 study in the journal Science, finds, for example, that animals are becoming more nocturnal to get out of the bipeds' way.

The authors of the study analyzed data from 76 other reports to learn how 62 species on six continents were trying to adapt to our intrusive presence. The data was sourced from all sorts of devices such as cameras to GPS trackers, and ran the gamut from 'possums to pachyderms.

What the researchers found was that animals known to split their activities between day and night were overwhelmingly becoming busier after dark. There was a 68% increase in nighttime activity among such animals.

If this habitat pressure continues, will we start to see individuals with, for example, better night vision, come to dominate as competitors for scarce resources? It'll be interesting to see.

Evolution

When people say, "Such and such animal has this trait because it allows them to…" what they're really saying is that "Of all the crazy mutations that nature tried out, individuals with this mutation fared better than others did." Whether it's effective camouflage, the ditching of a trunk, or becoming a night owl — except for owls who already… never mind — temporary adaptations become fixed evolutionary traits when the conditions in which they're beneficial remain in place long enough. In the case of the pressure we're continually imposing on other life forms, it bears saying that only the ones lucky enough to survive humankind's challenging influence in the first place will get that chance to change.

Creativity: The science behind the madness

Human brains evolved for creativity. We just have to learn how to access it.

Creativity: The science behind the madness | Rainn Wilson, David Eagleman, Scott ...
  • An all-star cast of Big Thinkers—actors Rainn Wilson and Ethan Hawke; composer Anthony Brandt; neuroscientists David Eagleman, Wendy Suzuki, and Beau Lotto; and psychologist Scott Barry Kaufman—share how they define creativity and explain how our brains uniquely evolved for the phenomenon.
  • According to Eagleman, during evolution there was an increase in space between our brain's input and output that allows information more time to percolate. We also grew a larger prefrontal cortex which "allows us to simulate what ifs, to separate ourselves from our location in space and time and think about possibilities."
  • Scott Barry Kaufman details 3 brain networks involved in creative thinking, and Wendy Suzuki busts the famous left-brain, right-brain myth.

Dinosaur bone? Meteorite? These men's wedding bands are a real break from boredom.

Manly Bands wanted to improve on mens' wedding bands. Mission accomplished.

Sex & Relationships
  • Manly Bands was founded in 2016 to provide better options and customer service in men's wedding bands.
  • Unique materials include antler, dinosaur bones, meteorite, tungsten, and whiskey barrels.
  • The company donates a portion of profits to charity every month.
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Giant whale sharks have teeth on their eyeballs

The ocean's largest shark relies on vision more than previously believed.

An eight-metre-long Whale shark swims with other fish at the Okinawa Churaumi Aquarium on February 26, 2010 in Motobu, Okinawa, Japan.

Photo by Koichi Kamoshida/Getty Images
Surprising Science
  • Japanese researchers discovered that the whale shark has "tiny teeth"—dermal denticles—protecting its eyes from abrasion.
  • They also found the shark is able to retract its eyeball into the eye socket.
  • Their research confirms that this giant fish relies on vision more than previously believed.
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A massive star has mysteriously vanished, confusing astronomers

A gigantic star makes off during an eight-year gap in observations.

Image source: ESO/L. Calçada
Surprising Science
  • The massive star in the Kinsman Dwarf Galaxy seems to have disappeared between 2011 and 2019.
  • It's likely that it erupted, but could it have collapsed into a black hole without a supernova?
  • Maybe it's still there, but much less luminous and/or covered by dust.

A "very massive star" in the Kinman Dwarf galaxy caught the attention of astronomers in the early years of the 2000s: It seemed to be reaching a late-ish chapter in its life story and offered a rare chance to observe the death of a large star in a region low in metallicity. However, by the time scientists had the chance to turn the European Southern Observatory's (ESO) Very Large Telescope (VLT) in Paranal, Chile back around to it in 2019 — it's not a slow-turner, just an in-demand device — it was utterly gone without a trace. But how?

The two leading theories about what happened are that either it's still there, still erupting its way through its death throes, with less luminosity and perhaps obscured by dust, or it just up and collapsed into a black hole without going through a supernova stage. "If true, this would be the first direct detection of such a monster star ending its life in this manner," says Andrew Allan of Trinity College Dublin, Ireland, leader of the observation team whose study is published in Monthly Notices of the Royal Astronomical Society.

So, em...

Between astronomers' last look in 2011 and 2019 is a large enough interval of time for something to happen. Not that 2001 (when it was first observed) or 2019 have much meaning, since we're always watching the past out there and the Kinman Dwarf Galaxy is 75 million light years away. We often think of cosmic events as slow-moving phenomena because so often their follow-on effects are massive and unfold to us over time. But things happen just as fast big as small. The number of things that happened in the first 10 millionth of a trillionth of a trillionth of a trillionth of a second after the Big Bang, for example, is insane.

In any event, the Kinsman Dwarf Galaxy, or PHL 293B, is far way, too far for astronomers to directly observe its stars. Their presence can be inferred from spectroscopic signatures — specifically, PHL 293B between 2001 and 2011 consistently featured strong signatures of hydrogen that indicated the presence of a massive "luminous blue variable" (LBV) star about 2.5 times more brilliant than our Sun. Astronomers suspect that some very large stars may spend their final years as LBVs.

Though LBVs are known to experience radical shifts in spectra and brightness, they reliably leave specific traces that help confirm their ongoing presence. In 2019 the hydrogen signatures, and such traces, were gone. Allan says, "It would be highly unusual for such a massive star to disappear without producing a bright supernova explosion."

The Kinsman Dwarf Galaxy, or PHL 293B, is one of the most metal-poor galaxies known. Explosive, massive, Wolf-Rayet stars are seldom seen in such environments — NASA refers to such stars as those that "live fast, die hard." Red supergiants are also rare to low Z environments. The now-missing star was looked to as a rare opportunity to observe a massive star's late stages in such an environment.

Celestial sleuthing

In August 2019, the team pointed the four eight-meter telescopes of ESO's ESPRESSO array simultaneously toward the LBV's former location: nothing. They also gave the VLT's X-shooter instrument a shot a few months later: also nothing.

Still pursuing the missing star, the scientists acquired access to older data for comparison to what they already felt they knew. "The ESO Science Archive Facility enabled us to find and use data of the same object obtained in 2002 and 2009," says Andrea Mehner, an ESO staff member who worked on the study. "The comparison of the 2002 high-resolution UVES spectra with our observations obtained in 2019 with ESO's newest high-resolution spectrograph ESPRESSO was especially revealing, from both an astronomical and an instrumentation point of view."

Examination of this data suggested that the LBV may have indeed been winding up to a grand final sometime after 2011.

Team member Jose Groh, also of Trinity College, says "We may have detected one of the most massive stars of the local Universe going gently into the night. Our discovery would not have been made without using the powerful ESO 8-meter telescopes, their unique instrumentation, and the prompt access to those capabilities following the recent agreement of Ireland to join ESO."

Combining the 2019 data with contemporaneous Hubble Space Telescope (HST) imagery leaves the authors of the reports with the sense that "the LBV was in an eruptive state at least between 2001 and 2011, which then ended, and may have been followed by a collapse into a massive BH without the production of an SN. This scenario is consistent with the available HST and ground-based photometry."

Or...

A star collapsing into a black hole without a supernova would be a rare event, and that argues against the idea. The paper also notes that we may simply have missed the star's supernova during the eight-year observation gap.

LBVs are known to be highly unstable, so the star dropping to a state of less luminosity or producing a dust cover would be much more in the realm of expected behavior.

Says the paper: "A combination of a slightly reduced luminosity and a thick dusty shell could result in the star being obscured. While the lack of variability between the 2009 and 2019 near-infrared continuum from our X-shooter spectra eliminates the possibility of formation of hot dust (⪆1500 K), mid-infrared observations are necessary to rule out a slowly expanding cooler dust shell."

The authors of the report are pretty confident the star experienced a dramatic eruption after 2011. Beyond that, though:

"Based on our observations and models, we suggest that PHL 293B hosted an LBV with an eruption that ended sometime after 2011. This could have been followed by
(1) a surviving star or
(2) a collapse of the LBV to a BH [black hole] without the production of a bright SN, but possibly with a weak transient."

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