Category: 7. Science

  • New Book Explores Past to Inform on Climate Change

    New Book Explores Past to Inform on Climate Change

    In today’s state of overwhelm, it’s easy to spend more time consumed with the present and the future than contemplating the events of the past. This constant forward motion can, at times, become exhausting and disorienting. We lose our grounding. We miss out on the context and insights that history can provide, and the lessons that may guide us through the tumult of the present. This holds true not just for national history and global history, but also geological history. That is, even events that unfolded millions or billions of years ago can offer insights that remain relevant to our lives and national policies today. 

    I wrote Strata: Stories from Deep Time to share this geologic lens with readers, and to spotlight the researchers working to untangle some of our planet’s oldest stories. This excerpt explores how scientists first began recognizing that oxygen didn’t billow up into the atmosphere until roughly halfway through Earth‘s existence — and how the arrival of this highly reactive gas fundamentally changed the planet from the seafloor to the stratosphere. By learning how and why oxygen showed up when it did, and how the planet responded to this period of intense global environmental change, we can gain context for the environmental crises unfolding across our planet today — and become better equipped to set ourselves on a more stable path forward.

    ***

    As you read this line, the oxygen you are pulling inside your body makes your body possible. It is allowing you to digest your most recent meal, move your eyes across these words, and think your thoughts. It is the single most important gas to your survival. You share this in common with every other animal on Earth, save for one lone parasite of Chinook salmon that somehow doesn’t need it. Well done, Henneguya salminicola.

    Throughout a given day, you fill your lungs with oxygen some 20,000 times. Most of us probably don’t give it much thought. Maybe we assume that this gas has always been here, a given on this highly habitable pale blue dot.

    But it turns out that this dot has not always been highly habitable, nor, for that matter, has it always been blue. The early Earth’s young magma surface sat gooey and cloaked in steam, too hot to hold liquid seas. It took a long time for continents to rise up and for ocean basins to fill in, and far longer still for oxygen to pool up in the atmosphere.

    “And so,” writes Rachel Carson in The Sea Around Us, “the rough outlines of the continents and the empty ocean basins were sculptured out of the surface of the earth in darkness, in a Stygian world of heated rock and swirling clouds and gloom.”

    Even in those earliest of gloomy days, oxygen — the element O — was all over the place, bound up in molecules like water vapor and quartz and carbon dioxide. It’s the third most abundant element in the universe, and it has been present on Earth since the beginning. But free oxygen — two atoms of O bound together by a pair of shared electrons, liberated from any other material but itself — didn’t emerge as a gas until more than halfway through Earth’s existence.

    If you reach out your arms and imagine Earth’s 4.54-billion-year history as a timeline that extends from the tip of your right hand to the tip of your left, the arrival of oxygen gas falls around your heart, at about 2.4 billion years ago, give or take a couple hundred million years.

    The fashionably late arrival of oxygen may sound like a planetary sigh of relief. Finally, the possibility for life larger than one cell, with lungs and lips and all the rest of it. But scientists familiar with oxygen’s highly reactive habits suggest its arrival was more like a nightmare.

    As is true of all elements, an atom of oxygen contains a cloud of negatively charged electrons that spin in an arrangement of “shells” around a positively charged nucleus. The outermost electron shell constantly seeks stability by filling to its capacity. In oxygen’s case, its outermost shell is two electrons short — comparatively fewer than other elements — and the configuration of those electrons contribute to oxygen’s high reactivity. Oxygen’s electron cloud is also relatively thin compared to other elements. Without much of a barrier between it and the outside world, the positive pull of the nucleus easily seeps out and lures in the negative charges of the two electrons it needs to stabilize. Two atoms of oxygen bound together as oxygen gas have a pull similarly as strong as a single atom on its own.

    When oxygen first appeared on Earth, it desperately rooted out and bonded with anything willing to share its electrons, fundamentally changing the materials it bonded with. It weaseled into microbial cells and mutilated their machinery. It sulked into currents and eddies and made arsenic more soluble, it spread hydrogen peroxide poisons into DNA. With all the havoc it wreaked, this gas might have initiated one of the worst mass extinctions in all of Earth history — though it’s hard to know this for sure, since the single-celled beings that would have gone extinct were too squishy to leave behind reliable fossils. Even so, some call this geologic moment the Oxygen Catastrophe.

    Over time, molecules from the bottom of the ocean to the top of the atmosphere grew to accept oxygen’s reactivity, and living things evolved ways to cope with this new gas. Their cells grew to tolerate it, and then to depend on it. They used it to break down food and generate energy that allowed them to grow larger and more complex, with multiple cells that communicated across newly sophisticated membranes. These oxygen-fueled innovations expanded and cascaded and eventually led to the evolution of eyeballs and brains and lungs and lips and, over billions of years, the possibility of us.

    So what, exactly, happened around 2.4 billion years ago? Why did oxygen arrive when it did? And how can we read this in the rock record?

    Courtesty of W. W. Norton & Company

    THE SEARCH FOR OXYGEN’S origin began with a problem. When Charles Darwin published On the Origin of Species in 1859, he agonized over the seeming absence of fossils in the planet’s oldest rocks. The ages of rocks at this time were known only in a relative sense — as in, what formed first and what followed. The scientific law of superposition, proposed by Danish geologist Nicolas Steno in the seventeenth century, helped clarify that younger strata always sit atop older strata, since that’s how sediments accumulate in lake beds and seafloors and so on.

    As hard as paleontologists of that time looked, they couldn’t find any remnants of ancient life in the oldest, bottom-most strata that they examined. Then bits and bobs appeared in what looked like an explosion of living things in strata above a certain age. This troubled Darwin deeply. Any such explosion of life undermined his theory of natural selection, a process of elimination that he argued should inherently take a very long time to unfold. By his estimations, it could never have taken place as instantaneously as those earliest fossils suggested.

    Halfway through On the Origin of Species, he gravely acknowledged the implications of this predicament. “The case at present must remain inexplicable[,]” he wrote, “and may be truly urged as a valid argument against the views here entertained.”

    But here we are, still entertaining Darwin’s views more than 150 years later. And that is thanks largely to rocks discovered not long after World War II.

    At the end of the war, a wave of mineral exploration arose across the world to meet the needs of rapidly expanding economies. Federal agencies hired geologists to scour continents for oil, gas, and coal to fuel those economies, along with metals like iron and uranium to build up arsenals of defense. This was of national interest, not just private economic interest.

    As geologists marched around the globe and sketched up their maps of these resources, they noticed other curious details about the planet’s history. That is, in their search for the materials that humans desired, they found inklings of how we got to be here desiring anything in the first place.

    In the summer of 1953, Wisconsin geologist Stanley Tyler was studying iron-rich rocks on the north shore of Lake Superior in Canada when he took a Sunday off to rent a boat and go fishing. While his lure bobbed in the water, he absently noted the shapes and colors along the shore, as any geologist might. One outcrop caught his eye, so he motored over to take a closer look.

    Tyler recognized the deposit as an extension of the Gunflint Chert, a rock formation with the texture of tightly packed brown sugar and the contents of ancient seafloor sediments. Cherts can take on a whole range of colors depending on the conditions they form within, from beige to red to green to other hues in between. Most of the chert that Tyler had found on that trip had been maroon, but this outcrop caught his eye for its striking shade of jet black. He knew that the color black in rocks was sometimes indicative of organic material, remnants of ancient life.

    He lopped off a chunk, stashed it in his boat, and motored on.

    Back at his lab in Madison he placed a sliver of that black chert under a microscope, and found shapes that did not speak the language of minerals. The rods, spheres, and squiggles he found did, as he suspected, look more lifelike than lithic.

    Based on geologic maps of the region, he knew these rocks had formed during the allegedly fossil-free epoch that had so troubled Darwin. Tyler’s gut told him he may have just found some of the earliest evidence of life ever discovered, but he was a mineralogist more than a paleontologist and so he needed a second opinion.

    That fall, he took photographs of his findings to a geology conference in Boston and shared them with a couple of colleagues. One among them, a Harvard paleobotanist named Elso Barghoorn, agreed that the samples looked rather lifelike, and the two published a short paper describing what they had found.

    This publication quadrupled the length of the fossil record. It was groundbreaking, but was brief and preliminary. They needed more time to study the fossils to do justice to the scope of their findings.

    For years, they didn’t make progress on a follow-up paper. A decade went by and, in 1963, Tyler passed away at the age of 57 from heart complications, without the satisfaction of sharing his discoveries more completely with the world. By 1965, an impatient colleague named Preston Cloud — a bantamweight boxing champion turned acclaimed Earth historian — threatened to beat Barghoorn to the punch with his own paper on the fossils. That was enough to push Barghoorn into gear. He rushed to complete a manuscript and published it in the journal Science a couple months before Cloud published his.

    “For all of time it will probably stand as the most important article ever written in the field . . . ,” writes William Schopf, a graduate student who helped Barghoorn pen that manuscript, but who humbly declined authorship himself because he didn’t feel he had contributed enough.

    Spurred by this new paper on the Gunflint Chert, geologists went searching for evidence of ancient life in black cherts around the world. Papers flooded out, claiming to have solved Darwin’s dilemma and showing how fossils had been in those seemingly lifeless rocks all along — they had simply been microscopic. The theory of natural selection persevered, and the lengthy record of our ancient roots began to fill out.

    But while those microscopic rods and squiggles resolved one nagging dilemma, they opened up a slew of other questions. What, exactly, were those fossils? What kind of world did they evolve into? And what kind of world did they create with their growth?

    Around the same time that these questions began bubbling up, another set of observations from the rock record thickened the plot of the squiggles. Geologists were compiling evidence that, before those lifeforms lived, the planet’s atmosphere had no oxygen gas in it at all. Minerals that disintegrate in the presence of oxygen were found locked up in ancient riverbeds older than a certain age. Then, around the time they believed those squiggles showed up on the scene, those riverbed minerals disappeared and the very first, rusty red fingerprints of oxygen began appearing in strata around the world.

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    Perhaps, some reasoned, those squiggles were responsible for painting the world’s soil and seafloor sediments red, by ushering in the very first poofs of oxygen. And perhaps, in their delivery of this gas, they catapulted Earth out of its original barrenness and into the tangle of complex life we know today.

    Excerpted from Strata: Stories from Deep Time. Copyright © 2025 by Laura Poppick. Used with permission of the publisher, W. W. Norton & Company, Inc. All rights reserved.

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  • Quantum Science Information | AZoQuantum.com

    Quantum Science Information | AZoQuantum.com

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  • Meteorological satellites observe temperatures on Venus

    Meteorological satellites observe temperatures on Venus

    image: 

    A photo with magnified sections to show just how small Venus is in the field of view of the observation satellites. Despite this limitation, researchers can still gather useful data. ©2025 Nishiyama et al. CC-BY-ND


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    Credit: ©2025 Nishiyama et al. CC-BY-ND

    Imaging data from Japan’s Himawari-8 and -9 meteorological satellites have been successfully used to monitor temporal changes in Venus’ cloud-top temperature, revealing unseen patterns in the temperature structure of various waves. A team led by the University of Tokyo collated infrared images from 2015–25 to estimate brightness temperatures on day to year scales. The results demonstrate that meteorological satellites can serve as additional eyes to access the Venusian atmosphere from space and complement future observations from planetary missions and ground-based telescopes.

    The Himawari-8 and -9 satellites, launched in 2014 and 2016, respectively, were developed to monitor global atmospheric phenomena through use of their multispectral Advanced Himawari Imagers (AHIs). The University of Tokyo team led by visiting researcher Gaku Nishiyama saw the opportunity to use the cutting-edge sensor data for spaceborne observations of Venus, which is coincidentally captured by the AHIs near the Earth’s rim.

    Observing temporal temperature variations in the cloud tops of Venus is essential to understand its atmospheric dynamics and related phenomena, such as thermal tides and planetary-scale waves. Obtaining data for these phenomena presents multiple challenges, as Nishiyama explained. “The atmosphere of Venus has been known to exhibit year-scale variations in reflectance and wind speed; however, no planetary mission has succeeded in continuous observation for longer than 10 years due to their mission lifetimes,” he said. “Ground-based observations can also contribute to long-term monitoring, but their observations generally have limitations due to the Earth’s atmosphere and sunlight during the daytime.” 

    Meteorological satellites on the other hand appear suited to fill this gap with their longer mission lifetimes (the Himawari-8 and -9 satellites are scheduled for operation until 2029). The AHIs allow multiband infrared coverage, which has been limited in planetary missions to date, essential for retrieving temperature information from different altitudes, along with low-noise and frequent observation. Aiming to demonstrate this potential to contribute to Venus science, the team investigated the observed temporal dynamics of the Venusian atmosphere and provided a comparative analysis with previous datasets. “We believe this method will provide precious data for Venus science because there might not be any other spacecraft orbiting around Venus until the next planetary missions around 2030,” said Nishiyama.

    The team first established a data archive by extracting all Venus images from the collected AHI datasets, identifying 437 occurrences in total. Taking into account background noise and apparent size of Venus in the captured images, they were able to track the temporal variation in cloud-top temperature during the periods where the geostationary satellite, Venus and the Earth lined up in a row.

    The retrieved temporal variations in brightness temperatures were then analyzed on both year and day scales and compared for all infrared bands to investigate variability of thermal tides and planetary-scale waves. Variation in thermal tide amplitude was confirmed from the obtained dataset. The results also confirmed change in amplitude of planetary waves in the atmosphere with time, appearing to decrease with altitude. While definitive conclusions on the physics behind the detected variations were challenging due to the limited temporal resolution of the AHI data, variations in the thermal tide amplitude appeared possibly linked to decadal variation in the Venus atmosphere structure.

    In addition to successfully applying the Himawari data to planetary observations, the team was further able to use the data to identify calibration discrepancies in data from previous planetary missions.

    Nishiyama is already looking at implications of the study beyond Venus’ horizon. “I think that our novel approach in this study successfully opened a new avenue for long-term and multiband monitoring of solar system bodies. This includes the moon and Mercury, which I also study at present. Their infrared spectra contain various information on physical and compositional properties of their surface, which are hints at how these rocky bodies have evolved until the present.” The prospect of accessing a range of geometric conditions untethered from the limitations of ground-based observations is clearly an exciting one. “We hope this study will enable us to assess physical and compositional properties, as well as atmospheric dynamics, and contribute to our further understanding of planetary evolution in general.”

    ###

    Journal article: Gaku Nishiyama, Yudai Suzuki, Shinsuke Uno, Shohei Aoki, Tatsuro Iwanaka, Takeshi Imamura, Yuka Fujii, Thomas G. Müller, Makoto Taguchi, Toru Kouyama, Océane Barraud, Mario D’Amore, Jörn Helbert, Solmaz Adeli, Harald Hiesinger, “Temporal variation in the cloud-top temperature of Venus revealed by meteorological satellites”, Earth, Planets and Space, DOI: 10.1186/s40623-025-02223-8

    Funding: This work was supported by JSPS KAKENHI Grant Number JP22K21344, 23H00150, and 23H01249, and JSPS Overseas Research Fellowship.

        
    Useful links:

    Department of Earth and Planetary Science – https://www.eps.s.u-tokyo.ac.jp/en/
    Graduate School of Science – https://www.s.u-tokyo.ac.jp/en/index.html

    Research contact:
    Dr. Gaku Nishiyama
    Department of Earth and Planetary Science, The University of Tokyo,
    7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
    gaku.nishiyama@dlr.de

    Press contact:
    Mr. Rohan Mehra
    Public Relations Group, The University of Tokyo,
    7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-8656, Japan
    press-releases.adm@gs.mail.u-tokyo.ac.jp
     

    About The University of Tokyo:

    The University of Tokyo is Japan’s leading university and one of the world’s top research universities. The vast research output of some 6,000 researchers is published in the world’s top journals across the arts and sciences. Our vibrant student body of around 15,000 undergraduate and 15,000 graduate students includes over 5,000 international students. Find out more at www.u-tokyo.ac.jp/en/ or follow us on X (formerly Twitter) at @UTokyo_News_en.


    Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.

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  • NASA Webb ‘Pierces’ Bullet Cluster, Refines Its Mass

    NASA Webb ‘Pierces’ Bullet Cluster, Refines Its Mass

    NASA’s James Webb Space Telescope recently zeroed in on the Bullet Cluster — delivering highly detailed images that show a greater abundance of extremely faint and distant galaxies than ever before. Using Webb’s crisp near-infrared observations of this region, researchers have more completely mapped the colliding galaxy clusters’ contents.

    “With Webb’s observations, we carefully measured the mass of the Bullet Cluster with the largest lensing dataset to date, from the galaxy clusters’ cores all the way out to their outskirts,” said Sangjun Cha, the lead author of the paper published in The Astrophysical Journal Letters and a PhD student at Yonsei University in Seoul, South Korea. (Previous studies of the Bullet Cluster with other telescopes relied on significantly less lensing data, which netted out with less precise estimates of the system’s mass.)

    “Webb’s images dramatically improve what we can measure in this scene — including pinpointing the position of invisible particles known as dark matter,” said Kyle Finner, a co-author and an assistant scientist at IPAC at Caltech in Pasadena, California.

    Mapping the Dark Matter

    All galaxies are made up of stars, gas, dust, and dark matter, which are bound together by gravity. The Bullet Cluster is made up of two very massive collections of galaxies, known as galaxy clusters, that are themselves bound by gravity.

    These galaxy clusters act as gravitational lenses, magnifying the light of background galaxies. “Gravitational lensing allows us to infer the distribution of dark matter,” said James Jee, a co-author, professor at Yonsei University, and research associate at UC Davis in California.

    To visualize gravitational lensing and dark matter, think of a pond filled with clear water and pebbles. “You cannot see the water unless there is wind, which causes ripples,” Jee explained. “Those ripples distort the shapes of the pebbles below, causing the water to act like a lens.” The same thing happens in space, but the water is dark matter and the pebbles are background galaxies.

    In all, the team measured thousands of galaxies in Webb’s images to accurately “weigh” both the visible and invisible mass in these galaxy clusters. They also carefully mapped and measured the collective light emitted by stars that are no longer bound to individual galaxies — known as intracluster stars.

    The revised map of the Bullet Cluster is shown in a new image: Layered on top of an image from Webb’s NIRCam (Near-Infrared Camera) is data from NASA’s Chandra X-ray Observatory that shows hot gas in pink, including the bullet shape at right. Refined measurements of the dark matter, calculated by the team using Webb’s observations, are represented in blue. (See the defined galaxy clusters within the dashed circles.)

    Their findings are persuasive: “We confirmed that the intracluster light can be a reliable tracer of dark matter, even in a highly dynamic environment like the Bullet Cluster,” Cha said. If these stars are not bound to galaxies, but to the cluster’s dark matter, it might become easier to pin down more specifics about the invisible matter.

    Viewed as a whole, the researchers’ new measurements significantly refine what we know about how mass is spread throughout the Bullet Cluster. The galaxy cluster on the left has an asymmetric, elongated area of mass along the left edge of the blue region, which is a clue pointing to previous mergers in that cluster.

    Dark matter does not emit, reflect, or absorb light, and the team’s findings indicate that dark matter shows no signs of significant self-interaction. If dark matter did self-interact in Webb’s observations, the team would see an offset between the galaxies and their respective dark matter.

    “As the galaxy clusters collided, their gas was dragged out and left behind, which the X-rays confirm,” Finner said. Webb’s observations show that dark matter still lines up with the galaxies — and was not dragged away.

    Although earlier measurements with other telescopes also identified invisible mass in addition to the mass in the galaxies, it was still possible that the dark matter could interact with itself to some degree. These new observations place stronger limits on the behavior of dark matter particles.

    ‘Replaying’ the Collision

    The strange new clumps and elongated line of mass the team identified may mean that the Bullet Cluster was produced by more than one collision of galaxy clusters billions of years ago.

    The larger cluster, which now sits on the left, might have suffered a minor collision before it rammed through the galaxy cluster now at right. The same larger cluster may also have experienced a violent interaction afterward, causing an additional shake up of its contents. “A more complicated scenario would lead to a huge asymmetric elongation like we see on the left,” Jee said.

    The Head of a ‘Giant’

    The Bullet Cluster is huge, even in the vast expanse of space. Webb’s NIRCam covered a significant portion of the hulking debris with its images, but not all of it. “It’s like looking at the head of a giant,” said Jee. “Webb’s initial images allow us to extrapolate how heavy the whole ‘giant’ is, but we’ll need future observations of the giant’s whole ‘body’ for precise measurements.”

    In the near future, researchers will also have expansive near-infrared images from NASA’s Nancy Grace Roman Space Telescope, which is set to launch by May 2027. “With Roman, we will have complete mass estimates of the entire Bullet Cluster, which would allow us to recreate the actual collision on computers,” Finner said.

    The Bullet Cluster is found in the Carina constellation 3.8 billion light-years from Earth.

    The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

    To learn more about Webb, visit:

    https://science.nasa.gov/webb

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  • Remembering When NASA Mounted The Space Shuttle Atop A Boeing 747

    Remembering When NASA Mounted The Space Shuttle Atop A Boeing 747

    The Boeing 747 continues to be recognized as one of the most iconic commercial jets of all time. Originally introduced in the 1960s, the game-changing aircraft brought unprecedented capacity, range, and comfort to the commercial aviation industry. After its launch, airlines across the world flocked to the type, with some even continuing to operate it today. The 747 and most of its variants are undoubtedly a major success.

    Launch Customer(s)

    Pan American World Airways

    First Delivery

    January 22, 1970

    Last Delivery

    January 31, 2023

    Number Delivered

    1,573


    While the 747 was a commercial success, it has served important roles in aviation beyond passenger operations. The aircraft was famously operated by the United States’ National Aeronautics and Space Administration (NASA), where two modified 747 variants carried the Space Shuttle, the aircraft used for recurring space travel. NASA’s impressive feat of using the jet comes with several interesting facts and a colorful history, further solidifying that the Boeing 747 was the true Queen of the Skies.

    The Shuttle Carrier Brought The Space Shuttle Back To Florida

    NASA Boeing 747 space shuttle carrier

    Photo: Carla Thomas NASA | Wikimedia Commons

    The Boeing 747s used to carry NASA’s Space Shuttle were known as “Shuttle Carrier” aircraft. The aircraft were used between 1977 and 2012, according to the National Air and Space Museum. The aircraft’s primary purpose was to transport the Space Shuttle from its landing location back to the Kennedy Space Center near Cape Canaveral, Florida. This purpose made the Shuttle Carrier a critical link in NASA’s space flight ambitions.

    Both aircraft involved in the program were modified Boeing 747 jets. The aircraft had to undergo several changes to safely transport such a massive piece of equipment, but still, the jets hold significant resemblance to the base model of the Boeing 747. Both aircraft were Boeing 747-100 variants, according to NASA. The first aircraft in the program was acquired from American Airlines in the mid-1970s, not long after the first Boeing 747 entered commercial service.

    Since the program’s launch, the Shuttle Carrier has become an iconic symbol of the United States’ space exploration aspirations. Though the Space Shuttle, and thus its carriers, are no longer in service, many remember the striking and rather unusual appearance of a 747 lifting off with another aircraft attached to the top of its fuselage. But for that to be possible, the aircraft underwent some major enhancements and modifications to be capable of transporting the Space Shuttle.

    Major Modifications Were Made To The Shuttle Carriers

    NASA Boeing 747 and Space Shuttle Enterprise

    Photo: Udo Haafke | Wikimedia Commons

    Because they were carrying such a large aircraft on top of their fuselages, both Shuttle Carrier jets were given some major enhancements. Three struts and their respective structural strengthening in the aircraft’s interior were placed on top of the Shuttle Carriers. In addition to improving the strength of the fuselage, it provided a place for the orbiter to be attached to the aircraft.

    The engineers also added enhanced horizontal stabilizers for improved directional stability. These were attached to the aircraft’s existing horizontal stabilizers, giving a unique and recognizable look to the aircraft’s tail section. Less visible to the public was the removal of the aircraft’s entire interior and cabin, which was necessary given that the aircraft was coming from a commercial airline.

    More advanced instruments to be used by flight crews were also installed. The primary purpose of these added systems were to monitor electrical loads of the orbiter during ferry flights. All of these changes, while certainly costly, made the 747 capable of carrying the Space Shuttle. Beyond these modifications, the aircraft’s appearance remained remarkably close to a standard Boeing 747.

    Related

    How The Boeing 747 Made A Comeback At Delta Air Lines

    30 years after the carrier initially retired the jumbojet, it made a comeback to its fleet.

    The First Shuttle Carrier Did More Than Ferry Aircraft

    747 SCA

    Photo: NASA | Wikimedia

    While the Shuttle Carrier was immortalized for its role in US space exploration, before it was converted into a ferry aircraft, the first jet in the program was actually used for a different purpose upon its arrival at NASA. According to NASA, the government agency used it to perform a series of flight tests at the Armstrong Research Center in Edweards, California. These tests shaped Federal Aviation Administration regulations that were designed to ensure safety for aircraft operating in wake turbulence.

    The tests focused on the phenomenon of wake turbulence, which is often found in the path of large aircraft. Though typically causing minor bumps, in the right conditions, it could pose a threat to the safety of flights that are following larger aircraft. These tests provided the foundation for new flight procedures for arriving and departing commercial aircraft. While used for NASA, it seems the Shuttle Carrier has also contributed to ensuring daily commercial aircraft operations remain safe.

    Following the aircraft’s time with flight tests focused on wake turbulence, it was sent to Boeing to be modified to carry the Space Shuttle. Though the aircraft had important contributions to the world of aviation, its most popular role would not start until changes were made by its manufacturer. The first Shuttle Carrier was utilized until November 1990, before its replacement aircraft was deployed.

    NASA’s Second Shuttle Carrier Also Logged An Impressive History

    Space-shuttle-Boeing-747

    Photo: NASA

    The second Boeing 747-100 to enter the Shuttle Carrier program was first built in 1973. The jet initially entered service with Japan Airlines, but was ultimately obtained by NASA in 1989. Like with the original 747 Shuttle Carrier, the second aircraft was modified by Boeing. Upon the completion of the necessary modifications, the aircraft was delivered to NASA on November 20, 1990. It would remain with the agency for over two decades.

    The aircraft was officially retired in February 2012, marking the end of an iconic and impressive chapter for NASA and the United States’ space exploration efforts. By the time the aircraft was removed from service, it had completed an impressive amount of work for NASA. Among its achievements were:

    Flight Hours

    33,004

    Flights With Shuttle

    66

    The Shuttle Carrier program proved to be a successful one for NASA, and has demonstrated the impressive capabilities of the Boeing 747 and other modern, commercial jets. Despite the Boeing 747’s success, the aircraft is becoming an increasingly rare sight in the skies across the world. It won’t be much longer before airlines follow NASA’s move and retire the aircraft type entirely.

    Related

    Which Boeing 747 Variant Was Used As The Shuttle Carrier Aircraft?

    Both aircraft were ex-commercial passenger jets.

    The 747 Is An Increasingly Rare Jet

    Lufthansa Boeing 747-8 aircraft

    Photo: Vincenzo Pace | Simple Flying

    Unfortunately for 747 fans, the aircraft is reaching the end of its service life. Though it might take longer for freighter airlines (which have embraced the jet) to completely retire the 747, in the commercial segment of the aviation industry, the aircraft has quickly lost favor. The 747’s four engines make it far less efficient than modern twin-engine jets, leading airlines to retire their fleets of the Queen of the Skies in favor of smaller, more cost-efficient aircraft.

    Though the 747’s reign is coming to an end, it boasts a long and successful career in connecting the world. Some of the 747’s largest passenger operators over its lifespan include Japan Airlines, British Airways, Singapore Airlines, and United Airlines. Additionally, major cargo carriers like Atlas Air and Kalitta Air invested heavily in the type.

    The 747 has become an iconic aircraft that revolutionized flying. Though it may soon disappear from the skies, it will likely be remembered for years to come. Countless 747s are displayed in museums across the world, keeping the memory of the famous jet alive. Additionally, for fans of the 747, Lego recently released a new set featuring the 747’s role as a Shuttle Carrier.

    747 Fans Can Now Purchase A Lego Shuttle Carrier Model

    Screenshot 2025-06-24 211837

    Photo: Lego

    Fans of NASA, Lego, or the 747 might enjoy one of Lego’s newest products: a replica of the Shuttle Carrier. The set comes with the pieces to assemble both the 747-100 and Space Shuttle, unlocking a new way to preserve and appreciate the aircraft’s legacy. This set costs about $230 and comes with a whopping 2,417 pieces.

    This isn’t the first tribute to modern aviation Lego has made. The company already sells a Concorde model, immortalizing the only supersonic passenger jet. Lego fans have embraced the kit, potentially paving the way for more aviation-themed Lego sets. The price of the Shuttle Carrier set also indicates Lego’s confidence in demand and excitement for the product.

    This Lego set, among countless other memorials to the Shuttle Carrier and the Boeing 747, demonstrates the widebody aircraft’s role in shaping modern travel and even space exploration. As the jet continues to be retired by commercial carriers, many are still celebrating the aircraft’s contributions to modern travel. Whether it’s displays in museums, Lego kits, or other experiences, the legacy of the Boeing 747 and the Shuttle Carrier is being kept alive by fans and stakeholders across the world.

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  • Hubble Spots Reflection Nebula in Taurus Molecular Cloud

    Hubble Spots Reflection Nebula in Taurus Molecular Cloud

    Astronomers using the NASA/ESA Hubble Space Telescope have produced an outstanding image of the reflection nebula GN 04.32.8.

    This Hubble image shows GN 04.32.8, a reflection nebula some 480 light-years away in the constellation of Taurus. The color composite was assembled from images taken in visible and near-infrared light. It is based on data obtained through two filters. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / G. Duchêne.

    GN 04.32.8 is located approximately 480 light-years away in the constellation of Taurus.

    Also known as DG 41, it is a small part of the stellar nursery known as the Taurus Molecular Cloud.

    “Reflection nebulae are clouds of dust in space that don’t emit their own light, as other nebulae do,” the Hubble astronomers said in a statement.

    “Instead, the light from nearby stars hits and scatters off their dust, lighting them up.”

    “Because of the way the light scatters, many reflection nebulae tend to appear blue, GN 04.32.8 included.”

    GN 04.32.8 is illuminated by a system of three bright stars in the center of the Hubble image, mainly the variable star V1025 Tauri in the very center.

    “One of those stars overlaps with part of the nebula: this is another variable star that is named HP Tauri, but is classified as a T Tauri star, for its similarity to yet another variable star elsewhere in the Taurus Molecular Complex,” the astronomers said.

    “T Tauri stars are very active, chaotic stars at an early stage of their evolution, so it’s no surprise that they appear in a prolific stellar nursery like this one.”

    “The three stars are also named HP Tau, HP Tau G2 and HP Tau G3; they’re believed to be gravitationally bound to each other, forming a triple system.”

    “Eagle-eyed viewers might notice the small, squashed, orange spot, just left of center below the clouds of the nebula, that’s crossed by a dark line,” the researchers said.

    “This is a newly-formed protostar, hidden in a protoplanetary disk that obstructs some of its light.”

    “Because the disk is edge-on to us, it’s an ideal candidate for study.”

    “We are using Hubble here to examine it closely, seeking to learn about the kinds of exoplanets that might be formed in disks like it.”

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  • World Asteroid Day 2025 — Watch live views of near-Earth asteroids for free online on June 30

    World Asteroid Day 2025 — Watch live views of near-Earth asteroids for free online on June 30

    World Asteroid Day 2025 is upon us! Here’s how you can celebrate the event by livestreaming real-time views of near-Earth asteroids from the comfort of your home.

    June 30 is the 10th anniversary of World Asteroid Day, an annual United Nations-backed event wherein partners raise awareness of asteroids, their scientific value and how humanity is working to mitigate the risks posed by these wandering solar system bodies. The date coincides with the anniversary of the 1908 Tunguska event, which saw a large meteor detonate over Siberia, flattening millions of trees and triggering widespread forest fires.

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  • Space, Tech, And AI: What Astronaut Tim Peake Can Teach Us About The Future Of Humanity

    Space, Tech, And AI: What Astronaut Tim Peake Can Teach Us About The Future Of Humanity

    When you’ve spent 6 months orbiting Earth in the International Space Station, your perspective on the planet and its problems is likely to change forever. Few people understand this more intimately than Tim Peake, the British astronaut, test pilot, and ambassador for STEM (Science, Technology, Engineering and Mathematics) education, who joined me for a fascinating conversation about space, AI, and the future of life on Earth.

    What struck me most in our conversation was how clearly Tim connects the dots between space exploration and the challenges we face on Earth, drawing on his remarkable experience and expertise. Whether it’s the climate crisis, the energy transition, or the role of AI in decision-making, space is not some distant frontier. It is deeply entangled with our present and our future.

    Looking Down On Earth From Orbit

    Peake vividly describes the emotional and intellectual impact of seeing our planet from above.

    “It gives you a fresh appreciation of how isolated and remote the planet is,” he told me. “A lot of people say fragile. I caution against using that word because I think the Earth’s pretty robust. But in terms of being remote and isolated, it makes you realize that this small rock is perfectly designed to support the life that has evolved on it.”

    And while the view from orbit can feel peaceful and serene, it’s also a powerful reminder of just how interconnected and dynamic our ecosystems really are. From wildfires in one region to dust storms in another, the visible signs of global interdependence are unmistakable from space.

    Peake explained, “You see wildfires and the smoke spreading across continents. You see sandstorms in the Sahara drifting across Northern Europe. That’s because the atmosphere is so thin, so tiny, and you see that very clearly from space.”

    The Promise Of Space-Based Technology

    Beyond the view, Peake is just as excited about what space can do for us back on Earth. Advances in manufacturing, communications, and energy are all being accelerated by what’s happening in orbit.

    One of the most compelling developments he pointed to is space-based manufacturing. In the absence of gravity, new kinds of structures can be created with unprecedented purity and precision.

    “For example, we can grow very large protein crystals in space that you can’t grow on Earth,” he said. “That can help pharmaceutical companies create better drugs with fewer side effects and lower dosages. Or if you’re trying to print out a human heart, doing that on Earth needs some sort of scaffolding. In space, gravity is not distorting the cellular structure.”

    He also believes that space-based solar power is not just science fiction. It could soon become a meaningful contributor to our global energy mix.

    “If we can make two-kilometer square solar arrays that beam energy back to Earth using microwaves, we can reduce the pressure on our grid and use space to help solve the energy crisis,” Peake explained.

    The falling cost of getting into orbit is a key enabler. As heavy-lift launch costs continue to drop, opportunities that once sounded fantastical, like factories in space or orbital data centers, suddenly look commercially viable.

    AI, Space Missions, And Human Judgment

    Naturally, we also discussed artificial intelligence. Peake believes that AI has a crucial role to play in helping humanity manage the deluge of data coming from satellites, sensors, and scientific instruments.

    “AI can analyze vast amounts of data and make good assumptions from it,” he said. “If a government is introducing a carbon emission policy in a city, AI can help measure the impact, evaluate the policy, and improve it based on outcomes.”

    But Peake also emphasized the continued need for human oversight. When it comes to critical decisions, especially in high-stakes environments like space missions or healthcare, humans must remain in the loop.

    “If you’re screening for breast cancer, for example, AI can assist doctors. But you still want the diagnosis coming from a person,” he said. “As humans, we like that reassurance. We want someone to put their intelligence on top of the AI’s assessment.”

    In other words, AI is not a replacement for human decision-making but a powerful augmentor, especially in environments where timely action matters.

    Why The Future Needs STEM… And STEAM

    Throughout our conversation, one theme kept coming up: the importance of inspiring the next generation, especially around STEM. For Peake, this is not a side mission; it’s central to why he does what he does.

    “I try to encourage kids to get involved in STEM, even if they don’t see themselves taking it to higher education,” he said. “The more you know about science and tech today, the more doors it opens for your future.” One initiative doing an outstanding job of sparking that curiosity is the Future Lab at the Goodwood Festival of Speed, where Peake serves as an ambassador. Curated by Lucy Johnston, the Future Lab showcases cutting-edge innovations from across the globe, from robotic rescue dogs and deep-sea exploration tools to mind-blowing space tech like the James Webb Space Telescope. “It’s hands-on, inspiring, and brilliantly curated,” Peake said. “You see people of all ages walking around in awe, and that’s exactly the kind of experience that can ignite a lifelong passion for science and technology.”

    Having taken my own son to Future Lab, I can say with certainty that it works. There’s something magical about seeing kids light up as they touch, feel, and interact with the technology that’s shaping tomorrow.

    The Space Economy Is Already Here

    Another eye-opener in our chat was just how much space already affects daily life. “On average, everyone touches about 42 satellites a day,” Peake said. Whether it’s making an online purchase, using navigation, or checking the weather, you’re using space infrastructure.

    And that footprint is only growing. Companies are already working on putting data centers in orbit to reduce energy consumption and cooling requirements on Earth. Communications, navigation, Earth observation, and climate monitoring are all becoming more dependent on space-based assets.

    But with growth comes risk. Peake is also an ambassador for The Astra Carta, an initiative supported by King Charles aimed at ensuring space is used sustainably. Space debris, orbital traffic, and light pollution are becoming serious issues.

    “We need rules of the road for space,” he said. “If we want to keep using it safely, we need to manage how we operate up there.”

    Reaching Beyond Earth And Into The Unknown

    As we wrapped up our conversation, I asked Tim the big one: Does he believe there’s intelligent life out there?

    “I absolutely do,” he said without hesitation. “Statistically, the odds are too strong. When you’re in space, and you see 200 billion stars in our galaxy alone, and then remember there are hundreds of billions of galaxies, it’s hard to believe we’re alone.”

    He also believes that space exploration will help answer some of the biggest questions humanity has ever asked about life, existence, and our place in the universe. But even if we don’t find extraterrestrials any time soon, the journey itself has value.

    Space inspires. It informs. And, increasingly, it enables.

    That, I think, is what makes Peake’s perspective so valuable. He’s lived at the intersection of science, technology, and wonder. And he reminds us that the frontier of space is not just about what lies out there but about what it can help us achieve here on Earth.


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  • Just a moment…

    Just a moment…

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  • Paddling 30,000 years into the past: Scientists replicate prehistoric seafaring with a primitive canoe

    Paddling 30,000 years into the past: Scientists replicate prehistoric seafaring with a primitive canoe

    • Canoe is paddled 140 miles (225km) across the open sea
    • The journey is from Taiwan to Japan’s Yonaguni Island
    • Research is reminiscent of famed 1947 Kon-Tiki expedition

    TOKYO, June 30 — Our species arose in Africa roughly 300,000 years ago and later trekked worldwide, eventually reaching some of Earth’s most remote places. In doing so, our ancestors surmounted geographic barriers including treacherous ocean expanses. But how did they do that with only rudimentary technology available to them?

    Scientists now have undertaken an experimental voyage across a stretch of the East China Sea, paddling from Ushibi in eastern Taiwan to Japan’s Yonaguni Island in a dugout canoe to demonstrate how such a trip may have been accomplished some 30,000 years ago as people spread to various Pacific Islands.

    The researchers simulated methods Palaeolithic people would have used and employed replicas of tools from that prehistoric time period such as an axe and a cutting implement called an adze in fashioning the 25-foot-long (7.5-metre) canoe, named Sugime, from a Japanese cedar tree chopped down at Japan’s Noto Peninsula.

    Researcher Kunihiro Amemiya uses a period-accurate axe to chop down a Japanese cedar tree in Noto Peninsula, Japan, to make a dugout canoe for a crossing across a region of the East China Sea from Taiwan to Yonaguni Island, in this handout image released on June 25, 2025. — Yousuke Kaifu handout pic via Reuters

    A crew of four men and one woman paddled the canoe on a voyage lasting more than 45 hours, traveling roughly 140 miles (225km) across the open sea and battling one of the world’s strongest ocean currents, the Kuroshio. The crew endured extreme fatigue and took a break for several hours while the canoe drifted at sea, but managed to complete a safe crossing to Yonaguni.

    Just as prehistoric people would have, the voyagers navigated by the sun and stars, as well as the direction of the ocean swells, though for safety’s sake they were accompanied by two escort craft. Yonaguni is part of the Ryukyu chain of islands stretching from Kyushu, the southernmost of Japan’s four main islands, down to Taiwan.

    The researchers previously failed with attempted crossings using reed rafts and then bamboo rafts, finding that they were too slow, insufficiently durable and unable to overcome the strong ocean current.

    A dugout canoe is pictured before departure on a crossing across a region of the East China Sea to Yonaguni Island, with leaf wave guards at the bow and stern, near Ushibi, Taiwan, in this handout image released on June 25, 2025. — Yousuke Kaifu handout pic via Reuters

    A dugout canoe is pictured before departure on a crossing across a region of the East China Sea to Yonaguni Island, with leaf wave guards at the bow and stern, near Ushibi, Taiwan, in this handout image released on June 25, 2025. — Yousuke Kaifu handout pic via Reuters

    “Through the project with many failures, we have learned the difficulties of crossing the ocean, and this experience gave us a deep respect for our Palaeolithic ancestors,” said University of Tokyo anthropologist Yousuke Kaifu, lead author of the study published on Wednesday in the journal Science Advances.

    “We found that the Palaeolithic people could cross the sea with the strong ocean current if they had dugout canoes and were skilful, experienced paddlers and navigators. They had to face the risk of being drifted by the strong ocean current and the possibility that they would never be able to come back to their homeland,” added Kaifu, who was aboard one of the escort boats.

    Archaeological evidence indicates that people approximately 30,000 years ago first crossed from Taiwan to some of the Ryukyu islands, which include Okinawa. But scientists had puzzled over how they could do this with the rudimentary technology of the time — no maps, no metal tools and only primitive vessels. And the Kuroshio current, comparable in strength to the Gulf Stream off Mexico, presented a particular challenge.

    The research was in the vein of the famous 1947 Kon-Tiki expedition in which Norwegian explorer Thor Heyerdahl carried out a much longer journey by raft from South America across the Pacific to the Polynesian islands. Heyerdahl aimed to show how prehistoric people from the Americas could have colonised Polynesia.

    An axe accurate to a period of 30,000 years ago, that scientists used to make a dugout canoe for a crossing across a region of the East China Sea from Taiwan near Ushibi to Yonaguni Island, traversing the Kuroshio current, is seen at Noto Peninsula, Japan, in this handout image released on June 25, 2025. — Yousuke Kaifu handout pic via Reuters

    An axe accurate to a period of 30,000 years ago, that scientists used to make a dugout canoe for a crossing across a region of the East China Sea from Taiwan near Ushibi to Yonaguni Island, traversing the Kuroshio current, is seen at Noto Peninsula, Japan, in this handout image released on June 25, 2025. — Yousuke Kaifu handout pic via Reuters

    “His theory is now countered by a series of pieces of evidence, but it was a great trial at the time. Compared to the time of the Kon-Tiki, we have more archaeological and other evidence to build realistic models” of prehistoric voyages, Kaifu said.

    The researchers in a companion study published in the same journal used simulations of sea conditions between Taiwan and Yonaguni 30,000 years ago to examine whether such a crossing was attainable at a time when the Kuroshio was even more powerful than today.

    “As our paleo-ocean model simulation showed, crossing the Kuroshio was possible in ancient times, so I believe they achieved it,” said physical oceanographer and study lead author Yu-Lin Chang of the Japan Agency for Marine-Earth Science and Technology.

    “However, ocean conditions were highly variable. Thus, ancient people may have encountered unpredictable weather conditions during their journey, which could have led to failure,” Chang added. — Reuters

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