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Ceasefire With Iran Is Likely, But Nuclear Deal Needs More Time

On: Saturday, June 20, 2026

Nuclear Plant
There is a possible agreement to end the war between the United States and Iran and it was announced last 14 June by U.S. President Donald Trump and Pakistani Prime Minister Shehbaz Sharif.

The deal includes stopping military actions, reopening the Strait of Hormuz, and eventually lifting U.S. restrictions on Iranian ports. Still, Iran’s nuclear program, a key issue, has not been settled and will be discussed in future talks.

Even with this diplomatic progress, negotiators have delayed decisions about Iran’s nuclear activities.

According to Iranian officials, discussions during the ceasefire period will focus on sanctions relief and the future of Tehran’s nuclear program. Sources indicate that the issue remains among the most difficult issues facing both sides.

The dispute goes back years. During Trump’s first term, the U.S. withdrew from the 2015 nuclear deal negotiated under President Obama. After that, Iran increased its uranium enrichment and built up more than 400 kilograms (about 900 pounds) of uranium close to weapons-grade.

Former Biden administration State Department spokesperson Matthew Miller criticized the framework, saying: "We have no assurances the nuclear program will ever be addressed, but Iran has shown the world it can take the global economy hostage and get something from the U.S. in return."

Republican Senator Lindsey Graham welcomed the ceasefire but stressed that future nuclear talks will be watched closely. "Under our law, any nuclear deal with Iran will be sent to Congress for review and a vote,” he said. “Congratulations to all on getting us to this point."

As negotiators prepare for formal talks in Switzerland, the focus is now on whether the ceasefire will last and if both sides can agree on Iran’s nuclear future.

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NASA Debunks Space Mysteries

On: Friday, June 19, 2026

Space
Mankind is still a long way off from colonizing other planets, but that hasn't stopped our quest to learn more about what mysteries lay beyond the boundaries of planet Earth.

Despite our progress since the Space Age began, including the successful landing of astronauts on the moon in 1969, there's still so much we don't know about the universe. Little by little, though, we're starting to learn more about outer space as our technology advances, and scientists at the National Aeronautics and Space Administration (NASA) have done much to highlight new discoveries and dispel age-old fallacies.

Since humans first started looking to the sky, there have been no shortage of misconceptions about space, and here are three examples of absurd space myths that NASA has helped debunk. As for our solar system's biggest debate, though, it seems there's growing momentum to make Pluto a planet again.

The Sun Is Burning The sun is hot — that is a fact. But why is it hot? If you're a connoisseur of 1960s rock 'n' roll, you're surely familiar with the Tommy James and the Shondells song, "Ball of Fire," which suggests that the sun is, in fact, a ball of fire in the sky. Alas, Tommy James might be one of the greatest recording artists of all time, but a scientist he is not.

The solar photosphere has ribbons of fire that shoot out from the sun's gaseous surface, but the sun itself isn't a ball of fire – it's a ball of gas fueled by nuclear fusion. Its heat comes not from flames, but from radiation, which is why you should never touch a meteorite with your bare hands. The "flaming tongues of fire" are a side-effect of the sun's heat interacting with the photosphere, and NASA's Interface Region Imaging Spectrograph (IRIS) showed as much during its measurements of the temperature levels of the various parts of the sun's atmosphere.

The Great Wall of China Can Be Seen From Space The legend goes that you can see the Great Wall of China from space. Naturally, China loves this story, since it posits the notion that this structure, which dates back about 2,700 years, could change the visage of the planet. This claim goes back hundreds of years — long before humans were able to visit outer space to make such a claim. Now that various nations of Earth have the technology, we finally have the data to verify or disprove the idea that the Great Wall can be seen from outer space.

During the Apollo 12 mission, NASA pilot Alan Bean looked, but could not find the Great Wall, or any other artificial structure. He said, "No man-made object is visible at this scale." Leroy Chiao, NASA commander on the International Space Station, took a photo, purportedly of the Wall, but it's far from definitive proof.

In truth, it takes extremely high-powered cameras to capture a photo where the Great Wall is clearly visible from space. Even from the ISS, which is far closer to the Earth than the moon is, the naked eye simply isn't capable of spotting the Great Wall of China unaided.

Death Is Imminent When Exposed To Space Much like the need to dodge asteroids, Hollywood would also have us believe that we would suffer an instant death if exposed to outer space without protection. The film "Mission to Mars" is one such example where (spoiler alert!) Tim Robbins' character removes his helmet in space, instantly freezing due to the harsh cold of the vacuum of space and preventing his wife from putting herself in danger in a futile attempt to rescue him. While not as sudden, Peter Quill nearly dies in "Guardians of the Galaxy" after just seconds of exposure to space.

In reality, neither scenario shows what would actually happen, and NASA proved it. In the vacuum of space, there aren't enough atoms to transfer one's body heat to that vast emptiness. Simply put, you'd retain your heat much longer than you would on, say, an iceberg in the Arctic Ocean.

That's not to say there's no danger in space. The lack of oxygen and the extremely low pressure would be detrimental to one's health for extended periods. In 1966, NASA technician named Jim LeBlanc was testing a prototype spacesuit in a vacuum chamber when he suffered accidental decompression. It took 87 seconds for the room to repressurize, and LeBlanc suffered no greater injury than an earache. While rapid changes in pressure can be dangerous and even fatal, it's not the instant death like many believe.

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Expect A Much Stronger El Niño This Year

On: Saturday, June 13, 2026

El Nino
The FIFA World Cup matches began this week, but that is not the only thing with global implications in recent days. The National Oceanic and Atmospheric Administration announced that El Niño has formed.

"El Niño has developed in the tropical Pacific," wrote a NOAA press release earlier this week announcing an El Nino Advisory. "El Niño, the warm phase of the El Niño Southern Oscillation (ENSO), is predicted to intensify to a moderate or strong level this fall," the notice continued.

NOAA forecasters and experts around the world say there is a 63 percent chance that the sea surface temperatures in the eastern Central Pacific will exceed 2 degrees Celsius above the neutral threshold." For those of you who do not speak Celsius, that is 3.6 degrees Fahrenheit. "If this threshold is surpassed, NOAA considers the event a "very strong" El Niño," the press release stated.

That could be conservative. While some climate experts weeks ago cautioned that it was too early to be conclusive about the strength of this event, all signs indicate that the "hype" may be warranted. El Niño is a part of a natural climate oscillation called ENSO. If temperatures are nearly 1.0 degree Fahrenheit above average or greater for consecutive months, then El Niño or the warm phase is declared.

La Niña is the cool phase. The ENSO cycle is related to a coupled relationship between winds, temperature, and pressure in the Pacific Ocean. The global models and indices used to diagnose and predict ENSO phases rely on an array of satellite, ocean, and atmospheric observations. Scientists have noted that global ocean observing systems play an important role in monitoring El Niño, which has significant impacts on agriculture, national security, energy, and other societal activities.

Both phases have an impact on global weather patterns. That's the "so what?" According to NOAA typical impacts for the U.S. include:

  • Less active hurricane season in the Atlantic basin due to stronger upper-level winds, but enhanced storm development in the central and eastern Pacific basins.
  • Stormy conditions in the southern tier of the country.
  • Increase likelihood of high tide flooding and harmful algal blooms, particularly the West Coast.
"Dry regions of Peru, Chile, Mexico, and the southwestern United States are often deluged with rain and snow, and barren deserts have been known to explode in flowers," according to NASA's website. "Wetter regions of the Brazilian Amazon and the northeastern United States often plunge into months-long droughts," it continued. Agricultural, fishing, and other ecosystem services can be disrupted by strong events.

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Scientists Traced The Mysterious Radio Signals From A Vampire Star

On: Monday, June 8, 2026

Vampire Star
The clashing magnetic fields of a white dwarf star and its neighboring red dwarf star are the source of signals from space that have remained a puzzle for over 20 years, radio astronomers in Australia have found.

The signals, or long-period radio transients, are a class of celestial radio emissions discovered in 2005. Most radio-producing objects release bursts that last for mere seconds or less, but long-period radio transients, about a dozen of which are known, produce radio waves in bursts lasting from minutes to over an hour.

Speculation had focused on highly magnetic pulsars called magnetars as the origin of these radio bursts, but now new research led by Kovi Rose of the University of Sydney, using the Australian SKA Pathfinder (ASKAP) radio telescope, has shown that symbiotic binaries are to blame for at least some long-period radio transients.

Symbiotic binaries feature a compact object — usually a white dwarf, which is the core remains of a sun-like star — stealing matter from a close companion star. This scenario often leads to a nova explosion when too much material accretes onto the surface of the white dwarf.

"Long-period radio transients have puzzled astronomers for years," said Rose, who is a postgrad student, in a statement. "Now we've been able to show that the source for one of these transients comes from a white dwarf actively pulling material from a companion star."

The system in question has been catalogued as ASKAP J1745-5051, and features a white dwarf that is about the diameter of Earth but a mass similar to that of our sun, accreting matter from a red dwarf star with a mass just a tenth of our sun's mass.

What makes ASKAP J1745-5051 stand out is that not only does it produce these long-period radio bursts, but it also produces blasts of X-rays.

"These emissions are all tied to the orbital motion of the system," said Rose. "But interestingly, the radio and X-ray signals don't peak at the same time, which tells us they're being produced in different regions of the system."

The X-rays are produced as matter spirals in from the red dwarf onto the white dwarf. As it gets closer to the white dwarf, gravity causes it to bunch up, friction increasing the temperature to hundreds of thousands, or even millions, of degrees, which is hot enough to emit X-rays. Exactly where it bunches depends on the relative positions of the white dwarf and red dwarf.

The origin of the radio waves is more complex. Both the white dwarf and the red dwarf have their own intrinsic magnetic fields. Their orbit around each other, which takes just 1.4 hours to complete, is not circular but strongly elliptical, meaning that at times the two objects are closer together than at other times. When they are close their magnetic fields clash, stripping charged particles from each other's surface. These charged particles then spiral around the magnetic-field lines and release a form of radio waves known as synchrotron radiation. The radio bursts last for the duration that the magnetic fields are in contact, every 1.4 hours.

While this explains ASKAP J1745-5051, it does not necessarily explain all long-period radio transients. For instance, only one other has been shown to produce X-rays. It is therefore possible that some other long-period radio transients have a different origin. However, Rose hopes that this new research will help distinguish between the different types.

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US NAS Head Pushed For Innovation

On: Wednesday, June 3, 2026

McNutt
The past year has been "filled with turmoil" in science policy, National Academy of Sciences (NAS) president Marcia McNutt said last 2 June during the annual State of the Science address in Washington, D.C.

McNutt cited problems such as "uncertainty" over federal support for science, "abrupt downsizing" of science agencies, a mass exodus of federal employees and the fact that the world’s top scientific minds are leaving the U.S.

"We always were the country where STEM talent came to us," McNutt said, referring to science, technology, engineering and math fields. "Now we are exporting our science talent elsewhere." After about 10 years as president of NAS, McNutt plans to step down on 30 June.

Since President Donald Trump took office last year, U.S. science has been a target for funding cuts, firings and intense regulatory scrutiny. By one estimate, around 100,000 federal employees at scientific agencies have either been fired or left public office in his second term. The administration has also cut nearly 8,000 scientific grants, mostly from the National Institutes of Health and the National Science Foundation, according to a Nature analysis published in January (some grants have since been reinstated by the courts).

And just last week, as Scientific American reported, the administration published a proposal to give political appointees final say on grant funding instead of researchers, overturning a decades-long precedent. "Now, what could possibly go wrong with that?" McNutt quipped.

"Frustrated and demoralized as many of us are right now, we must consider what is in our power, as a research community, to improve while, at the same time, pushing back against inappropriate political interference in research," she said.

To make science more "resilient" and "competitive," McNutt said that scientists should partner with industry—and that universities should support researchers who do so. And she urged scientists to train students to take science-adjacent jobs outside of academia.

Without bridging the gap between industry and science, she warned, the "best and brightest" students may "shun" careers in science, "domestic talent" will continue to seek opportunities abroad, and the economy will suffer.

The speech was met with some skepticism from scientists and science advocates who called attention to the threats facing U.S. research. "This focus on the private sector as we are facing down complete and total destruction of actual SCIENCE is unreal to me," wrote Colette Delawalla, founder and CEO of Stand Up for Science, in a post on Bluesky. "We are doing publicly-funded free training for companies ... this is the selling out of science to the Tech Bros," she added.

McNutt also recommended cutting red tape and lowering regulatory hurdles for researchers, as well as furthering reliance on artificial intelligence to "increase the rate of discovery."

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