Subscribe to the 1440 Daily Digest

The most impactful stories of the day, expertly curated and explained. 100% free, unsubscribe anytime. Terms & Privacy.

White Dwarfs and Last Week's News and Research

Plus, the latest findings from across the web

Good morning. It's Tuesday, Oct. 20, and welcome to this week's Science & Technology newsletter. First time reading? Sign up here or forward to share with friends.

 

Having explored neutron stars and black holes in the past, this week we're wrapping up the major trio of objects that stars can become at the end of their lives by taking a look at white dwarfs. Our own sun will become one of these stellar remnants billions of years from now, and it's never too early to see what's in store for the solar system!

 

We're also breaking down the abolition of leap seconds, deep-sea rocks catching on fire, how to measure the speed of light with a microwave oven, and much more.

 

Want to share your thoughts on this newsletter? Whether it's something you enjoyed learning about, potential improvements, or a suggested topic for a future issue, simply reply to this newsletter or email [email protected].

 

—Marco Daniel Machado, 1440 Science & Technology Section Editor

 

PS—Missed a past newsletter, recently subscribed, or are curious to see what we've written about before? Check out our archive of topics and resource feed here.

Life After Fusion

 

White dwarfs are the most common stellar remnants and the fate of about 97% of stars. They form after a star with less than about eight times the sun's mass runs out of viable nuclear fuel in its core. Lacking the gravity to hold on to its outer layers, they are ejected by stellar winds and radiation pressure from the core. The leftover, Earth-sized core is the white dwarf, composed mostly of carbon and oxygen.

 

> What makes a star become a white dwarf, a neutron star, or a black hole?
> View a gallery of planetary nebulae—a misnomer for the layers around white dwarfs.

 

Unable to carry out nuclear fusion, white dwarfs resist collapsing under their own gravity due to quantum pressure exerted by electrons. However, electron degeneracy pressure can only support white dwarfs up to about 1.44 times the sun's mass—the Chandrasekhar limit. If a white dwarf gains mass and approaches this limit, carbon fusion ignites in a runaway thermonuclear explosion that obliterates the entire star and briefly outshines all others in its galaxy.

 

> Watch an explainer and visualization of electron degeneracy pressure.

> See a simulated detonation of a white dwarf via a Type Ia supernova.

> White dwarfs can repeatedly explode without self-destructing through novae.

 

Because of their predictable peak luminosity, these supernovae are considered standard candles—tools for measuring cosmic distances. In 1998, scientists used these exploding stars to measure the universe's expansion and uncovered that it was accelerating. White dwarfs that don't accumulate matter or explode will gradually crystallize and cool into black dwarfs over quadrillions of years.

 

> Stellar models and observations suggest white dwarfs crystallize from the inside out, forming diamond-like cores.

> Black dwarfs have never been seen because the universe is too young.

 

Discover more:

> "White dwarfs" may be a misnomer, as the remnants exist in many different colors.

> In 2017, astronomers discovered a white dwarf pulsar—a white dwarf behaving like a neutron star.

> What would happen if you stood on a white dwarf?

 

Keep learning by exploring all our findings on White Dwarfs here.

News in Context

 

1440 brings you the knowledge and context behind the week's stories:

 

Timekeepers abandoned leap seconds in favor of adopting the leap hour starting next year, though it won't be needed for millennia. (More)

 

> Why have we added 27 leap seconds to clocks since 1972?

> Rather than leap seconds, technology companies had been implementing leap smears to avoid critical errors.

 

Astronomers identified the most distant fast radio burst ever recorded, which originated in a tiny galaxy more than 10 billion years ago. (More)

 

> The one-time nature of many FRBs has made determining what causes them difficult, but it may be related to neutron stars.

> ... or the cores of galaxies that consume up to 100 Earths a minute.

 

Nikon disqualified the winner of its Small World in Motion competition after determining that the entry violated its AI-use rules. (More)

 

> The new top-five winning videos feature jellyfish larvae and a colorful sea slug.

> Check out this 90-second guide to spotting AI-generated videos.

 

Hackers remotely raised the temperatures of refrigerators and freezers at more than 500 French shops and supermarkets, causing fires and food spoilage. (More)

 

> Hackers have exploited backdoors that manufacturers have intentionally installed on devices.

> Learn about the hidden device that's allowed hackers to control millions of cars.

Research Spotlight

 

Like all great researchers, we love spending time learning about the latest breakthroughs across science and technology. Here's what we found this week.

 

EV batteries can last over 20% longer by avoiding less powerful cells.

Chalmers University of Technology | Henrik Dahlberg. The batteries in electric vehicles consist of multiple interconnected cells, with overall battery performance held back by cells that wear out and degrade sooner. Models suggest that a battery architecture that allows weak cells to be bypassed individually can improve EV battery lifespan in high-voltage vehicles, thereby reducing replacement costs. (More)

 

> Why do batteries lose their capacity to store power over time?

> Power cells can wear out more quickly through fast charging.

 

Tardigrades inspire a new method of cryopreserving red blood cells in mice.

American Chemical Society | Staff. Storing red blood cells typically involves adding glycerol to prevent the formation of damaging ice crystals, but removing glycerol before transfusion damages the cells. A new method instead uses a protein fragment that tardigrades use to survive extreme environments and has been used to reduce freezer burn, with up to 89% of mouse red blood cells fully recovering. (More)

 

> What are tardigrades, and what allows them to survive decades without water?

> Tardigrades can survive over 1,000 times more radiation than humans thanks to a bubble wrap-like protein.

 

Microplastics become chemically active in water-rich environments.

Columbia University | Staff. Although plastic is not supposed to react with other chemicals—explaining its use in food and water packaging—researchers found that microplastics interact with water to facilitate the transfer of electrons needed for chemical reactions. Their increased surface-to-volume ratio creates more chemically active locations, which may produce biologically harmful reactive radicals. (More)

 

> The use of sewage sludge to fertilize farmland has introduced microplastics into human food chains.

> Microplastic deposits in major arteries have been linked to increased risk of cardiovascular diseases.

 

Deep-sea rocks can spontaneously catch fire during laboratory processing.

USGS | Staff. Seafloor massive sulfides contain elements critical to various modern technologies, but extracting them requires extensive refinement. Scientists found that some of these rocks can heat up and combust when brought to the surface and exposed to air, introducing a potential hazard to deep-sea mining operations. (More)

 

> Watch a 3D visualization of how deep-sea mining machines collect resources.

> Deep-sea mining may provide enormous economic benefits at the cost of losing ecosystems and potential lifesaving medicines.

Etcetera

 

> Learn how to open a shaken can of soda without making it explode.

 

> You can measure the speed of light at home using a microwave oven.


> By keeping half their brains awake at all times, dolphins never fully fall asleep.


> A network crash messed up the first message sent over the internet's predecessor.

 

> See why Euler's identity is considered mathematics' most beautiful equation.

 

> The US features a location with more geysers than the rest of the world combined.

 

> The Concorde supersonic airliner would get longer whenever it flew.
 

> The Drake equation allows scientists to estimate the number of extraterrestrial civilizations that we can detect. 

 

> Particles moving faster than light give nuclear reactors their eerie blue glow.
 

> Google's expansive global network of servers began with some Lego bricks.

 

> Despite having only animal cells, this sea slug can perform photosynthesis.


> Explore an interactive 3D visualization of the nearest 100,000 stars to Earth.

🔭 Want more? Explore over 100 of our write-ups and thousands of fascinating insights and resources at 1440's hub for Science & Technology.

"Many billions of years will elapse before the smallest, youngest stars complete their nuclear burning and shrink into white dwarfs. But with slow, agonizing finality, perpetual night will surely fall."

—Paul Davies

Join millions of insatiably curious news readers:

1440 Daily Digest

 

The "1440 Explores" podcast: 

Apple, Spotify, YouTube

 

Weekly 1440 Topics newsletters: 

Science & Technology (Tuesday)

Health & Medicine (Wednesday)

Business & Finance (Thursday)

Society & Culture (Saturday)

Behind the Name. Why 1440? The printing press was invented around the year 1440, spreading knowledge to the masses and changing the course of history. More facts: In every day, there are 1,440 minutes. We’re here to make each one count.

 

Want to connect with millions of insatiably curious minds? Become a 1440 partner here.

1440 Media 111 N Canal St, Suite 1210 Chicago, IL 60606

Copyright © 2026, 1440 Media, All rights reserved.