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Space Exploration

America is currently constructing two massive telescopes, but unfortunately, there is only enough funding to complete one of them

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Three enormous optical telescopes are currently being constructed, surpassing anything we currently possess in terms of size. These three discoveries have the potential to provide answers to some of the most profound mysteries of the universe, which have remained elusive to current scientific instruments. Nevertheless, the proposed budget cap from the National Science Foundation (NSF) jeopardizes one aspect of the equation.

Even though the JWST has uncovered incredible discoveries, the future of astronomy extends beyond just space exploration. Building larger telescopes on the ground offers several advantages over their space-based counterparts. Not only are they easier to repair, maintain, and upgrade, but they also provide greater flexibility for scientific exploration. Future plans include the development of a telescope on the Moon, along with a base.

Scientists have high expectations for several ambitious projects in the field of astronomy. These include the Giant Magellan Telescope (GMT), the Thirty-meter Telescope (TMT), and the Extremely Large Telescope (ELT). Additionally, there are other telescopes, like the Square Kilometer Array, that operate at wavelengths beyond the range of human vision. Interestingly, all three of these telescopes are sometimes collectively referred to as extremely large telescopes. Despite the presence of the atmosphere, both options would provide significantly higher resolution than the JWST.

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However, a new proposal suggests eliminating one of the initial two options.

Collaboration is a key aspect of astronomy, with many individuals and organizations working together towards common goals. In this context, it may not be of great concern to some who will be responsible for building and owning certain projects. It is important to note that while the third project is a collaboration between European and South American nations, the TMT and GMT projects are both run by American organizations. That provides the ELT with a certain level of protection in the event of budget reductions. None of the consortium partners want to compromise their reputation by failing to fulfill their commitments. The work on the ELT began in 2017. Building something of this magnitude, which requires both size and precision, is a time-consuming process. As a result, the first light is anticipated to happen in 2028. Despite potential delays, there is little doubt that it will eventually occur.

Both the TMT and the GMT are American projects, with the latter being located in Chile. The funding for the GMT primarily comes from the USA’s NSF, with support from several universities and scientific institutions. Additionally, six other countries are also contributing to the project. The TMT project, although involving Indian, Japanese, and Canadian participation, originated at two California universities and is intended to be located in Hawaii.

However, the National Science Board, which advises the NSF, has suggested a limit of $1.6 billion for NSF funding for giant telescopes. That’s a lower cost compared to either of the two projected expenses individually, although considering the other factors, it should be sufficient for one.

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The statement issued by the board indicates that they have no intention of merely postponing the costs and waiting for additional funding. Furthermore, it suggests that the NSF should engage in a discussion with the Board in the upcoming May 2024 meeting regarding their strategy for choosing between the two potential telescopes to support. This discussion should encompass estimated costs and a timeline for the project.

There is a chance that the NSF might reject the recommendation, or even that Congress could allocate an additional billion and a half towards astronomy due to its perceived significance. So far, that is the current focus of each team’s representatives, at least publicly, instead of engaging in arguments about who should be given priority. It is unlikely that new funds will be available, especially considering the current political climate characterized by partisan conflicts that hinder budget allocations.

In theory, it is possible for other contributors to increase their shares. However, according to John O’Meara, the chief scientist at Keck Observatory, neither telescope currently has a viable future without investment from the NSF.

Scientists have been expressing their concern and highlighting the importance of both.

Others in different scientific fields may not be very understanding; they might even quietly make fun of those who expected to receive two new toys but had to settle for just one. However, the two instruments have been carefully crafted to function in perfect harmony. Every spot on our planet has its limitations when it comes to observing the sky. To achieve comprehensive coverage, it is necessary to have at least one instrument in the Northern Hemisphere and one in the Southern Hemisphere. Every design has been optimized to enhance specific capabilities, with the expectation that other areas will be compensated by alternative designs.

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Upon initial observation, the TMT would seem to be the most reasonable choice. Given its location in the Northern Hemisphere, it has the potential to work in collaboration with the ELT. Additionally, a suggested location in the United States could provide a group of supporters to advocate for it.

Nevertheless, there has been discussion about relocating the TMT to the Canary Islands, a northern region under Spanish jurisdiction, due to the significant opposition it faces from Native Hawaiians. In addition, discarding either project would result in a significant loss of the funds invested thus far. The GMT, being more advanced than the TMT, would incur a greater financial setback.

There are numerous valuable applications for $1.5 billion, such as medical research to combat diseases, scientific endeavors addressing global crises, or even non-scientific pursuits. However, basic research has a rich history of yielding unforeseen benefits over time. Constructing both telescopes would result in an additional $5 in taxes for every American, not on an annual basis but as a one-time payment. Their total cost will be significantly lower than that of the JWST, and each one will have a much longer lifespan.

Allocating budgets can be a challenging task, especially when comparing the potential benefits, which vary greatly. In this situation, one must consider the value of knowledge for its own sake versus options that offer practical but uncertain payoffs. In contrast, the NSF may find it relatively easy to choose between two instruments with different, but overlapping, capacities.

 

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.

Astronomy

What is the most terrifying communication that humanity could receive from outer space?

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If there are extraterrestrial civilizations within a reasonable distance capable of detecting our unintentional transmissions, there exists a possibility, albeit small, that among the initial signals they intercept, they could receive the commencement of the 1936 Olympic Games. Therefore, in the unlikely event that they do receive these signals, we might come across a speech by Adolf Hitler during our first encounter with an alien species.

“Naturally, this was not the initial transmission,” clarified Seth Shostak, a senior astronomer at SETI, during an interview with RealClearScience. “However, it was emitted at a sufficiently high frequency to penetrate the ionosphere.”

In the movie Contact, this ultimately became the initial communication that mankind received from an extraterrestrial society. The entities promptly returned the signal to Earth, unaware of the profound consequences that transmitting broadcasts of Adolf Hitler from outer space would have on the targeted species they were endeavoring to establish communication with. It is similar to greeting a random person and then unintentionally reciting a chapter from Mein Kampf.

Fortunately, it is highly likely that we won’t encounter this issue because extraterrestrial civilizations shouldn’t be able to distinguish the signal strengths.

“The power consumption would have been minimal, and the antenna used would not have had a specific direction,” Shostak elaborated. “The notion that extraterrestrial beings might intercept it is highly improbable.”

However, it is possible that we may receive significantly more alarming initial communications, as individuals have been deliberating on X (Twitter) and Reddit.

It appears that people are primarily focused on receiving warnings from extraterrestrial civilizations right now, possibly as a result of a recent unnamed television series.

What would be the scariest message humanity could receive from outer space?
byu/silly_vasily inAskReddit

According to certain proposed resolutions to the Fermi Paradox, which ask why we haven’t detected any signs of advanced extraterrestrial civilizations, the explanation is that these civilizations are intentionally concealing their presence due to the apprehension of their own annihilation.

Another concern is the possibility of receiving an unclear message that extraterrestrial beings will provide us with limited information, apart from the fact that they are en route.

What would be the scariest message humanity could receive from outer space?
byu/silly_vasily inAskReddit

One theory, called the Zoo Hypothesis, is related to this topic. The theory posits that extraterrestrial beings possess knowledge of our existence but deliberately confine us within a designated “zoo” to allow for our evolutionary and societal development. This parallels humanity’s practice of preserving certain areas as nature reserves and refraining from engaging with uncontacted tribes. Based on this hypothesis, it is possible that we may receive contact once we have reached a satisfactory level of technological and societal development and potentially be accepted into a community of other galaxies.

Although there is a prevailing apprehension that initiating communication with an extraterrestrial civilization will probably elicit fear due to humanity’s historical tendency to fear the unfamiliar, there is a potentially more alarming notion.

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Space Exploration

Bacteria on the ISS have changed into something that has never been seen before on Earth

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Movies and TV shows depict space stations as sterile and immaculate environments. However, wherever humans are present, they inevitably carry along with them a multitude of bacteria. Bacteria have colonized various habitats within the International Space Station (ISS), and due to their rapid evolutionary capacity, a particular species has been observed diverging from its terrestrial counterparts.

The bacteria in question are specific strains of Enterobacter bugandensis. This pathogen is classified as an opportunistic pathogen, which indicates that it can only cause disease in individuals who are already “perturbed” or experiencing a disruption in their health, such as those who are already battling another disease or have a weakened immune system. The bacteria is renowned for its multidrug resistance, rendering multiple antibiotic treatments ineffective in combating it. Therefore, it is crucial to comprehend the characteristics of this bacteria in space.

In 2018, researchers discovered five different variations of this bacterium on the International Space Station (ISS). Recent findings now indicate that there are a total of 13 distinct variations of this bacterium present on the space station. The first analysis showed some similarities, but the more in-depth genetic study suggests that the ISS strains may have gone through multiple mutations in response to the unique environmental stress, creating genetic and functional differences from E. bugandensis found on Earth.

The authors stated in the paper that they have identified specific genes that are only found in organisms associated with the ISS and not in their counterparts on Earth.

Gaining insight into the evolutionary processes of bacteria in space is crucial for safeguarding the well-being of astronauts and developing alternative strategies to combat these harmful microorganisms. With regards to these recently developed strains, their ability to adjust to microgravity could potentially conceal their vulnerabilities.

The authors further stated that these genes have the potential to be effective targets for therapeutic interventions against harmful microorganisms in the distinct environment of the IS.

The research team acknowledges certain constraints in the genetic analysis, preventing them from definitively attributing the characteristics of these strains solely to space. There is, however, a lot of strong evidence that these strains have become part of different bacterial communities, including those made up of opportunistic pathogens that are resistant to many drugs.

The coexistence of these organisms may have contributed to their ability to adapt and thrive in the challenging conditions of the ISS, characterized by low gravity, high radiation, and elevated levels of carbon dioxide.

The research is published in the scientific journal Microbiome.

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Space Exploration

The first-ever X-ray image of a solitary atom

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Recalling X-rays may bring back memories of fractures or routine dental examinations. However, this highly intense light has the ability to reveal more than just our skeletal structure. It is also employed to investigate the intricate realm of molecules, including real-time analysis of biochemical reactions. However, a significant challenge arises as scientists have yet to examine a solitary atom using X-rays. Up until this point,.

Scientists have successfully characterized a single atom using X-rays. They were able to distinguish the type of atoms they observed, as there were two different ones. Additionally, they successfully studied the chemical behavior exhibited by these atoms.

Scanning probe microscopes are able to capture images of atoms, but it’s impossible to determine their composition without the use of X-rays. With our advanced technology, we have the ability to precisely identify the specific type of an individual atom and analyze its chemical state simultaneously,” stated Professor Saw Wai Hla, a senior author from the University of Ohio and the Argonne National Laboratory.

Once we achieve that, we can track the materials all the way down to the smallest possible unit of just one atom. This will have a significant impact on the environmental and medical sciences and potentially lead to groundbreaking discoveries that could greatly benefit humanity. This discovery has the potential to revolutionize the world.

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Through careful analysis, the study successfully monitored the movement of an iron atom and a terbium atom, which belong to the group of rare-earth metals. Both of them were placed within their respective molecular hosts. An ordinary X-ray detector was enhanced with an additional, unique one. This particular one featured a specialized, sharp metal tip that needed to be positioned in close proximity to the sample in order to gather the X-ray-excited electrons. By analyzing the measurements obtained from the tip, the team was able to determine the composition of the substance, and that’s not the end of it.

“We have also been able to detect the chemical states of individual atoms,” Hla explained. When you look at the chemical states of an iron atom and a terbium atom in their molecular hosts, it is clear that the terbium atom stays alone and its chemical state does not change because it is a rare-earth metal. On the other hand, the iron atom exhibits strong interactions with its surrounding environment.

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The signal observed by the detector has been likened to fingerprints. Researchers can gain a comprehensive understanding of a sample’s composition and explore its physical and chemical properties. This has the potential to greatly enhance the performance and application of a wide range of materials, both commonly used and more obscure ones.

“The technique employed and the concept demonstrated in this study have made significant advancements in the field of X-ray science and nanoscale studies,” stated Tolulope Michael Ajayi, the first author of the paper and conducting this research as part of his PhD thesis. Furthermore, the utilization of X-rays for the detection and analysis of individual atoms has the potential to bring about significant advancements in research and pave the way for innovative technologies in fields like quantum information and the identification of trace elements in environmental and medical studies, among others. This accomplishment also paves the way for cutting-edge instrumentation in the field of materials science.

The study has been published in the prestigious journal Nature.

A previous iteration of this article was published in May 2023.

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