Connect with us


The Recurrence of Unexploded Bombs from World Wars





The Earth possesses a substantial quantity of explosive bomb material, amounting to millions of tons, primarily originating from the two global conflicts that occurred throughout the 20th century. Although a significant portion of these entities has been neglected and overlooked in recent decades, recent studies have revealed that a considerable number of them contain a chemical compound that renders them progressively more susceptible to detonation over time.

Amatol, a potent explosive compound derived from a blend of TNT and ammonium nitrate, was extensively employed in various explosive devices utilized throughout World War One and World War Two. These devices encompassed airplane bombs, shells, depth charges, and naval mines.

Additional frequently employed explosives, such as pure trinitrotoluene (TNT) or pentaerythritol tetranitrate (PETN), exhibit generally consistent stability throughout time and do not exhibit an increase in their level of hazard compared to their first stages. Nevertheless, Amatol exhibits an increasing susceptibility to effect over time when subjected to specific settings.

Two scientists from the University of Oslo and the University of Stavanger in Norway conducted a series of experiments where they applied weights to five samples of amatol explosives obtained from battlefields. This finding demonstrated that the bombs exhibited a higher degree of sensitivity to impact than previously acknowledged, and their volatility progressively escalated as they underwent aging.

The observed change in temperament can be attributed to the chemical reactivity of amatol with other substances present in the natural environment.

The study authors note that the presence of moisture, coupled with other conditions, can enhance the impact sensitivity of amatols.

It is widely acknowledged that explosive compositions, including ammonium nitrate, have the potential to undergo sensitization upon exposure to trace amounts of metals or interactions with metals. “The presence of these metal contaminants can undergo a chemical reaction with ammonium nitrate, resulting in the formation of complex salts and the sensitization of the mixture,” they state.

The presence of unexploded bombs from World War II is a frequent occurrence, often resulting in significant disruptions.

In February 2024, a German bomb weighing 500 kilograms (1,102 pounds) was found in a backyard in Plymouth, UK. More than 100 military personnel and specialists in bomb disposal were sent, while a significant number of surrounding inhabitants were compelled to flee, paradoxically signifying one of the most extensive evacuation endeavors since the conclusion of the Second World War.

Fortunately, the detonation of the device was executed without any casualties; nonetheless, such occurrences can occasionally culminate in terrible outcomes. In 2008, a total of 17 individuals sustained injuries at a building site located in the German town of Hattingen. The incident occurred when an excavator collided with a 250-kilogram (550-pound) bomb from the World War II era, resulting in its detonation.

Recent research suggests that occurrences involving unexploded bombs, such as the one described, have the potential to escalate into a significant issue. In conclusion, the researchers emphasize the importance of informing individuals responsible for dismantling unexploded explosives of the heightened sensitivity of amatol to impact.

The recent research findings have been published in the esteemed publication, Royal Society Open Science.

As Editor here at GeekReply, I'm a big fan of all things Geeky. Most of my contributions to the site are technology related, but I'm also a big fan of video games. My genres of choice include RPGs, MMOs, Grand Strategy, and Simulation. If I'm not chasing after the latest gear on my MMO of choice, I'm here at GeekReply reporting on the latest in Geek culture.

Continue Reading
Click to comment
Notify of
Inline Feedbacks
View all comments


Threads, a competitor of Meta’s X, is inviting developers to register for API access and has released documentation





Following the limited release of its developer API to a few chosen firms in March, Threads, Meta’s alternative to Twitter and other similar platforms, is now providing developer documentation and a registration form for individuals or organizations who are interested in using the API before its official public debut in June.

The updated documentation provides comprehensive information about the existing constraints and endpoints of the API. This information is beneficial for developers who wish to commence their development of Threads-connected applications and other projects that interface with the new social network.

For example, those who wish to monitor metrics related to Threads’ articles can utilize an Insights API to obtain data such as views, likes, replies, reposts, and quotes. Additionally, the API provides instructions on publishing posts and media, retrieving answers, and a set of troubleshooting suggestions.

According to the documentation, Threads accounts have a restriction of 250 API-published posts and 1,000 replies within a 24-hour period. This limitation is in place to prevent spam or other forms of excessive usage. Additionally, Threads provides the specific requirements for images and videos uploaded by users. It mentions that text posts in threads are limited to a maximum of 500 characters, which is longer than the previous character limit of 280 characters on Twitter. However, it is significantly less than the 25,000 characters available to paid subscribers on X or the current limit of 100,000 characters for articles posted directly on X’s platform.

It is still to be determined whether Meta will show preference for specific types of apps.

The current beta testers for the Threads API include prominent social media tool developers such as Sprinklr, Sprout Social, Social News Desk, Hootsuite, and the technology news platform Techmeme.

While Threads has started integrating with the broader fediverse, which consists of interconnected social networking sites like Mastodon, it seems that enabling or disabling fediverse sharing cannot be done directly using the API. However, users still need to access their settings within the Threads app in order to submit content to the fediverse.

According to Meta, the new documentation will be periodically updated based on input received from developers. Furthermore, those who are interested in constructing using the latest API and offering input can now apply for access through a registration page. This process can also assist Meta in monitoring the applications that are getting ready to be launched simultaneously with the public release of the API.

Continue Reading


Scientists conducted research on our planet’s responses during the phenomenon of totality





The snapping turtles all simultaneously entered the waters of Lake Tawakoni as soon as the moon covered the sun. The earth was adorned with twilight. The clouds swiftly traversed the sky. Jupiter was present next to the sun and was brightly radiating during the day. The majority of birds and insects had become quiet or completely silent.

Describing the experience of a total solar eclipse is challenging due to its profound effects on the surrounding light and abrupt drop in temperature, causing surprise shivering. However, on April 8th, I, along with many individuals throughout North America, had the opportunity to observe a remarkable astronomical phenomenon.

I traveled to Wills Point, located around one hour east of Dallas, to rendezvous with Darci Snowden, a space physicist from Central Washington University in Ellensburg, along with her undergraduate students. Local families gathered to watch as weather balloons were launched from a wooden pier to collect data, bringing joy to the onlookers.

Prior to the eclipse, the weather forecast in Texas indicated unfavorable conditions, including the possibility of thunderstorms and cloud cover obstructing the view of the heavens. After the situation settled, we experienced an extended period of clear skies while the moon passed in front of the sun, causing it to appear like a thin crescent. At the precise moment of totality, a substantial cloud passed past, resulting in audible expressions of disappointment from all present. Fortunately, the sun’s typically imperceptible atmosphere, known as the corona, became visible through gaps in the clouds. Fiery flares bursting from the sun’s surface were seen as tiny red spots at its edges.

Regardless of whether the weather was cloudy or clear, there were still scientific tasks to be completed. Occasions of total solar eclipses offer exceptional chances to examine the sun and its influence on Earth in unparalleled manners.

In Wills Point, the day before the April 8 eclipse, Snowden’s team initiated the launch of a sequence of 30 weather balloons, commencing at 2 p.m. CDT. The intention was to launch one object into the air every hour, consistently during the whole night, and to continue this pattern for six hours following the occurrence of the eclipse. These balloons, filled with helium, may ascend to a height of 33 kilometers (20 miles) in the stratosphere, which is the second-lowest layer of the atmosphere. They transported battery-operated instrument bundles known as radiosondes to gather data on temperature, humidity, pressure, and wind direction and speed.

Snowden and her students aim to obtain comprehensive data regarding the impact of an extraordinary occurrence, like a total solar eclipse, on Earth’s atmosphere. The researchers are investigating the phenomena occurring in the lowest part of the atmosphere, called the planetary boundary layer, which extends up to around two kilometers and covers the Earth’s surface. The topography of the terrain, which includes features like mountains, buildings, and woods, and solar radiation descending from the atmosphere, both have an impact on the dynamics of this layer.

Specifically, the team is seeking evidence of gravitational waves. It is important to distinguish gravitational waves from gravitational waves, which are disruptions in the spacetime continuum brought about by the collision of sizable celestial objects like black holes. Gravity waves, on the other hand, are a phenomenon that occurs closer to the Earth’s surface. These phenomena can occur when a mountain range or other external force lifts pockets of air, which then fall as a result of gravity. This process generates a regular oscillation that can transfer energy across the atmosphere. Additionally, sudden fluctuations in temperature might trigger their activation. When cool air gets more compact and descends, it occasionally descends to such a low point that it surpasses its balance and then rises again, creating a wave.

“It is akin to exerting pressure on an ice cube submerged in a glass of water,” Snowden remarks.

In the 2017 U.S. total solar eclipse, scientists conducted an experiment by flying balloons in Wyoming and New York, outside the path of totality. They discovered indications that the shadow of the moon, as it swiftly moved across the atmosphere, produced gravity waves near the surface that propagated outward, resembling the bow waves created by a moving ship. This phenomenon had been forecasted over half a century before but had never been conclusively observed. During the same event in 2017, scientists definitively saw eclipse-induced gravity waves at higher altitudes in the atmosphere for the first time (SN: 4/30/18).

In this instance, Snowden aims to verify the prior indications of their presence in the lower layers of the atmosphere. The objective of launching the balloons 24 hours before totality, which occurs when the moon totally obscures the sun, was to gather the first measurements prior to the eclipse. Subsequently, these measures might be juxtaposed with the ones obtained during and subsequent to the occurrence.

This data has the potential to contribute to more accurate forecasts for both short-term weather patterns and long-term climate trends. Although gravity waves are one of the smallest types of atmospheric waves that scientists investigate, they can have a substantial impact. They exert a significant impact on the dynamics of turbulence, facilitate the passage of heat, and facilitate the dispersion of airborne chemicals across the entire world. Numerous individuals traverse extensive distances, occasionally shattering akin to ocean waves at altitudes of 500 kilometers or more above the Earth’s surface.

Eli Pugsley, a senior physics major involved in leading the launches, describes the process of getting the team’s weather balloons up shortly before and during totality as “undoubtedly stressful.” “However, once we establish a consistent pattern, each individual fulfills their responsibilities, and the process proceeds effortlessly.”

The data collected from the students will be combined with data from approximately 40 other teams participating in NASA’s Nationwide Eclipse Ballooning Project. These teams will also be deploying weather balloons along the line of totality. Collectively, the data may ascertain whether the eclipse generated gravity waves in the lower atmosphere. However, it will take around one year to collect and analyze the information, according to Snowden.

Researchers and citizen scientists across the country were conducting various studies connected to the eclipse. Meanwhile, large numbers of eclipse watchers flocked to towns along the path of totality, hoping for an unobstructed glimpse of the celestial event.


Physicist Fabiano Rodrigues and his team at the University of Texas, Dallas campus, focused their attention on the ionosphere, which begins at an altitude of around 80 to 90 kilometers above the Earth’s surface.

Solar radiation bombards the thin atmospheric gases in this layer, causing ionization, where the atoms split into electrons and nuclei. During the night, while not exposed to the intense sun radiation, these charged particles have an opportunity to come together again. Analogous transformations occur when there is an abrupt transition into darkness during a complete solar eclipse.

Rodrigues and his students strategically positioned inexpensive, readily available devices with the ability to receive satellite signals, such as GPS, in a large triangular formation. One device was placed at the university, another approximately 100 kilometers to the north, and the third approximately 50 kilometers east in the town of Terrell. These detectors monitor the instantaneous increase and decrease of electron concentration in the ionosphere, which serves as an indicator of its level of ionization.

The data obtained by Rodrigues and his team during the eclipse could potentially validate the forecasts on the extent to which the ionosphere will deionize due to the reduction of sunlight caused by the eclipse. It could also identify any shortcomings in these predictions. The collected data will be utilized to study the influence and deterioration of satellite transmissions caused by changes in the ionosphere. This research aims to enable engineers to mitigate these effects in future communication and navigation systems.

According to Rodrigues, the number of electrons in the ionosphere decreased, as anticipated during the event. However, it would probably take a few days for him to determine which models provided the most precise forecasts. Although there was some cloud cover in Dallas, he is very satisfied with the outcome.

Meanwhile, when the sun regained its usual intensity above Lake Tawakoni, Snowden and her colleagues paused to contemplate the extraordinary event they had just observed before resuming their balloon releases.

“It is an awe-inspiring encounter,” she states. “I consider myself very lucky to have witnessed it.”


Continue Reading


Prepare an ample supply of food, water, and fuel in anticipation of the upcoming total solar eclipse





The Lorain County Emergency Management (EMA) in Ohio has advised individuals observing the eclipse and residents within the path of totality to ensure they have an ample supply of food, water, and fuel in preparation for the total eclipse on April 8. This recommendation is due to the anticipated increase in visits to the area.

According to those who saw it, the most recent total solar eclipse across the United States was remarkably impressive. It is challenging to imagine any improvements to the scene by the time Monday arrived after looking at the photographs.

However, if we are fortunate and the weather conditions are favorable, we may see something extraordinary since the eclipse aligns with the period of maximum solar activity, and there is a possibility of observing Baily’s beads.

“During the year 2017, the Sun was approaching a period of solar minimum.” Observers of the complete solar eclipse were able to witness the awe-inspiring corona. However, due to the Sun’s lack of activity, the streamers that extended into the solar atmosphere were limited to only the equatorial regions of the star. NASA states that during solar minimum, the Sun exhibits greater magnetic symmetry, resulting in a simpler look.

“During the 2024 eclipse, the Sun will be in or close to solar maximum, a period characterized by a magnetic field that resembles a complex and chaotic structure, similar to a tangled hairball.” It is probable that streamers will be observable throughout the corona. Furthermore, spectators will have an enhanced opportunity to observe prominences, which manifest as vivid, pink spirals or arcs emanating from the Sun.

The eclipse will be visible throughout the whole stretch of land from Mexico to Canada. The path of totality, where a total solar eclipse is visible, is broader in comparison to 2017. This is because the Moon is in closer proximity to Earth as a result of its position in its orbit. Consequently, a larger number of individuals will have the opportunity to observe the Sun’s corona.

NASA stated that there is a possibility of observing a coronal mass ejection, which is a significant release of solar material, if the timing is fortunate during the eclipse.

However, safety considerations usually arise with eclipses. Following the recent eclipse, there was a notable increase in Google queries pertaining to the consequences of directly gazing at the Sun.

Additionally, there are logistical challenges arising from a significant surge in travelers seeking to witness the celestial phenomenon. As a result, the regions situated along the path of totality are presently making preparations to accommodate this rush. Last month, Lorain County officials issued a warning about the potential consequences of the upcoming eclipse. They cautioned that there may be a surge in traffic, longer wait times for facilities like hospitals and gas stations, and challenges in obtaining food and other essential supplies.

According to USA Today, Dave Freeman, the director of Lorain County EMA, “We may experience an influx of unfamiliar crowds.” “Our current infrastructure lacks the necessary road network to support that.”

“Many of the roads in this area consist of two lanes,” Freeman stated, according to Yahoo News. “Unlike cities such as Chicago and Cleveland, our city does not have a large number of wide roads with multiple lanes. As a result, if we experience larger crowds than anticipated, the traffic situation here could become quite severe.”

The EMA is cautioning that the surge of cell phone use in the vicinity may lead to signal loss when the system becomes overwhelmed. The team advises homeowners to proactively fill their vehicles with gasoline, ensure an ample supply of food, and minimize unnecessary travel throughout the next weekend preceding the eclipse.


It is crucial that you direct your attention towards the eclipse and derive pleasure from it. However, it is imperative that you take precautions to protect your eyes from harm. To do so, please refer to our informative manual on how to properly observe eclipses. If the weather remains unclouded, you may also utilize this guide on how to capture the approaching eclipse in the most optimal manner.


Continue Reading


Would love your thoughts, please comment.x