Scientists Propose Installing a Super Laser on the Moon for Revolutionary Research

Illustration of dark craters near the moon’s south pole

Explore the Dark Craters near the Moon’s South Pole

Credit: Science Photo Library / Alamy

Scientists aim to establish a groundbreaking laser system in one of the moon’s coldest craters to significantly enhance the navigation capabilities of lunar landers and rovers.

Ultra-stable lasers are vital for highly precise timing and navigation systems. These lasers operate by reflecting a beam between two mirrors within a cavity, maintaining a consistent beam speed. This precision is largely due to the chamber’s size stability, which neither expands nor contracts. To achieve this, mirrors are typically maintained in a cryogenic vacuum, insulated from external vibrations.

The moon hosts numerous craters at its poles, which lack direct sunlight due to minimal axial tilt. Consequently, these permanently shadowed areas are extremely cold, with some craters projected to reach temperatures around -253°C (20 Kelvin) during the lunar winter.

Junye from JILA, along with a research team in Boulder, Colorado, has proposed that these icy conditions, combined with the moon’s absence of natural vibrations and an almost non-existent atmosphere, make these craters ideal for ultra-stable lasers. The potential stability of these lunar lasers could surpass that of any terrestrial counterparts.

“The entire environment is incredibly stable,” Ye emphasizes. “Despite variations between summer and winter on the Moon, temperature fluctuations range only from 20 to 50 Kelvin, contributing to a remarkably consistent environment.”

Ye and his research team envision a lunar laser device akin to an optical cavity already developed in JILA’s lab, featuring a silicon chamber equipped with dual mirrors.

Current optical cavity lasers on Earth can maintain coherence for just a few seconds, meaning their light waves can synchronize briefly. However, the moon-based laser is projected to sustain coherence for at least a minute, which will facilitate its role as a reference laser for a variety of lunar missions. This includes maintaining the lunar time zone and coordinating satellite formations using lasers for distance measurement. Given that light from the moon takes just over a second to reach Earth, it could also serve as a reliable reference for Earth-based activities, as highlighted by Ye.

Although implementing this idea poses challenges, the rationale is sound and could greatly benefit future lunar missions. According to Simeon Barber from the Open University, UK, “Recent lunar landers have experienced suboptimal landings due to varying lighting conditions, complicating vision-based systems. Leveraging stable lasers for positioning, navigation, and timing could enhance the reliability of landings in high-latitude areas.”

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Source: www.newscientist.com

Philosophers Propose That Time is a Psychological Construct

In his latest book, A Brief History of the Philosophy of Time, Professor Adrian Verdon from Wake Forest University suggests that our perception of time passing is an instance of psychological projection—an error in cognition that leads to misinterpreting our experiences.

Time is an example of psychological projection. Image credit: Gemini AI.

Phrases like “Time flies,” “Time waits for no one,” and “As time passes” suggest that the movement of time is a real phenomenon influencing our lives. We navigate the present, witnessing events as they transition into memory.

Yet, articulating the concept of time’s flow is challenging. What does it mean for time to ‘pass’? Rivers flow because water moves; how does time move?

While events unfold, we speak of their positions as if they shift continuously through past, present, and future. If some events approach us as future occurrences while others recede into the past, where exactly do they reside? The notions of future and past appear to lack a physical location.

Throughout history, humans have contemplated time, ingraining it into our understanding of ourselves and the surrounding world.

This is why, as a philosopher, I have always deemed advancements in our conceptualization of time—both philosophical and scientific—to be of unique significance.

The Era of Ancient Philosophers

Many ancient philosophers expressed skepticism regarding time and change. Parmenides of Elea, a Greek philosopher from the 6th to 5th centuries BC, questioned how events could transition from future to present to past when neither the future nor the past exists.

He posited that if the future is real, it must also be real at this moment. Thus, if only the present is real, the future cannot be.

This notion implies that present events inexplicably emerge from nothing.

Parmenides wasn’t alone in his doubts; similar ideas regarding the contradictions in our discussions of time can be found in the works of Aristotle, the Advaita Vedanta philosophy of ancient Hinduism, and Augustine of Hippo, known as St. Augustine, among others.

Albert Einstein and the Theory of Relativity

During the early modern period, physicist Isaac Newton operated under the assumption of an unrecognized, real flow of time—time as a dynamic entity, akin to a cosmic clock that meticulously captures all motion and acceleration.

Then came Einstein.

In 1905 and 1915, Einstein introduced his special and general theories of relativity, respectively, challenging long-held beliefs about time and change.

Einstein’s theory dismisses Newton’s view of time as a universal phenomenon.

By Einstein’s era, it had been established that the speed of light remains constant, independent of the light source’s velocity. To accept this fact necessitated an understanding of object speeds as relative.

Nothing can be categorically labeled as stationary or in motion; it all hinges on your “frame of reference.”

A frame of reference provides the spatial and temporal context an observer assigns to an object or event, assuming it is stationary in relation to everything else.

For instance, an observer drifting through space may see a spaceship pass by, yet the universe remains indifferent to whether the observer is immobile and the spaceship is moving or vice versa.

This understanding alters our perspective on the function of watches. Since light’s speed is constant, two observers in motion relative to one another will record different times for the same events.

In a classic scenario, two lightning strikes occur simultaneously. An observer at a train station sees both at the same moment, while an observer on a moving train assigns differing times to each strike based on their relative motion.

Consequently, one observer approaches light from one strike and recedes from the other, leading to the time discrepancy.

The stationary observer perceives both strikes at identical moments since light reaches him simultaneously. Neither perspective is incorrect.

The duration between occurrences and the timing of events relies on the observer’s frame of reference.

Observers in relative motion will disagree on current events; what seems immediate to one may be future to another.

Einstein’s theory posits that all moments in time are equally real. Every past event and future occurrence is currently ‘happening’ to a hypothetical observer. There is no event merely categorized as a potentiality or a distant memory. No singular, absolute present exists; therefore, time does not flow through which events are ‘becoming.’

Change signifies a difference over intervals. I remember a point, and later, I recall even more moments. That encapsulates the essence of time’s passage.

This notion has gained acceptance among both physicists and philosophers, referred to as “eternalism.”

This leads us to an important inquiry: If time’s passage is nonexistent, why do we perceive it as such?

Time as a Psychological Projection

One prevailing notion posits that the sensation of time’s passage is illusory, echoing Einstein’s famous reflections.

Characterizing it as an “illusion” implies that our conviction in time’s passage results from a deceptive perception, akin to an optical trick.

However, I propose that this belief arises from a misunderstanding.

As I illustrate in my book, A Brief History of the Philosophy of Time, our feeling of time traversing is an example of psychological projection.

A simple analogy involves colors: a red rose isn’t inherently red; it reflects specific light wavelengths that evoke the sensation of redness.

In essence, roses aren’t really red nor do they create an illusion of redness—the experience of color arises from our interpretation of objective truths about roses.

It’s valid to distinguish roses by their color; enthusiasts of roses do not claim profound truths about color itself.

In a similar vein, my findings suggest that the experience of time’s passage is neither entirely real nor an illusion; it reflects how humans interpret their environment.

Just as our visual comprehension of reality cannot be fully understood without reference to colors, our understanding of the world relies on the passage of time.

I can assert that my GPS indicates I’ve strayed off course without attributing consciousness to the GPS.

My GPS is non-sentient. Although we lack a mental map of our surroundings, we can trust that the GPS accurately represents our location and destination.

Likewise, even if physics does not accommodate the concept of a dynamic passage of time, time remains effectively dynamic in the context of my experiential reality.

The sensation of time passing is deeply interconnected with how humans articulate their experiences.

Our representations of reality are inherently colored by our perspective as perceivers and thinkers.

The error lies in conflating our perception of reality with reality itself.

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Adrian Verdon. 2025. A Brief History of the Philosophy of Time (2nd Edition). Oxford University Press, ISBN: 9780197684108

Author: Professor Adrian Burdon, a researcher at Wake Forest University.

This article was first published in The Conversation.

Source: www.sci.news

House Democrats to Propose Legislation Aimed at Saving NOAA

House Democrats are focusing on staffing issues at the National Weather Service field office, aiming to pass legislation swiftly to thwart further funding and staffing cuts from the Trump administration affecting the National Oceanic and Atmospheric Administration, especially following severe storms nationwide.

As reported by NBC News, the proposed amendment to the Republican Budget Adjustment Bill safeguards NOAA from disbandment and prevents its responsibilities from being shifted to other federal entities, as well as protecting its website and datasets.

Democratic representatives including Eric Sorensen from Illinois, Joe Negas from Colorado, and Wesley Bell from Missouri are poised to introduce these amendments early on Wednesday.

This legislation underscores Congressional worries about staffing levels at the National Weather Service, particularly after the Trump administration’s layoffs of prosecutors and the offering of early retirement packages to long-serving employees. Recently, a short-staffed weather room managed severe thunderstorms and tornado outbreaks during a weekend that resulted in at least 28 fatalities in the Midwest and South.

“With hurricane season on the horizon and extreme weather becoming more frequent, we cannot afford to jeopardize NOAA,” said Moskowitz, a former director of Florida Emergency Management, in an emailed statement.

Sorensen, the sole meteorologist in Congress, emphasized:

“As a meteorologist who has reported on severe thunderstorms and tornadoes, I understand the critical need for the National Weather Service to be fully staffed at all times.”

Rep. Eric Sorensen, D-Ill, of Rockford, Illinois, in 2023.
Chris Nieves/USA Today Network

However, the amendment faces significant opposition from Republicans who control the House. The Trump administration’s initial budget proposal proposed cutting over $1.5 billion from NOAA.

The National Weather Service is working to address staffing shortages this spring. Recently, NOAA initiated a “period of reallocation” to recruit 76 meteorologists for critical roles that were left vacant due to budget cuts.

At least eight of the nation’s 122 weather forecast offices, including in Sacramento, California; Goodland, Kansas; and Jackson, Kentucky, anticipate reducing or discontinuing overnight operations within the next six weeks, according to Tom Fahy, director of the National Weather Service employee organization. He noted that over 52 of the weather forecast offices in the U.S. are experiencing staffing shortages exceeding 20%.

The National Weather Service has not provided additional details regarding staffing levels at its various offices.

“The National Weather Service remains committed to its mission of delivering life-saving forecasts, warnings, and decision support services to the public,” stated NOAA’s communications director, Kim Dester, in an email. “In the near future, NWS will update its service level standards for weather forecast offices to adapt to changes in human resources while prioritizing mission-essential operations.”

Last weekend, the Jackson office of Kentucky was put to the test during dangerous storms statewide. Fahy mentioned in an interview that staff worked overtime to manage the situation with “every available hand,” although the challenges were anticipated ahead of time.

“We had sufficient lead times in monitoring supercells,” Fahy explained, adding that unforeseen serious events could arise at any moment. “A severe thunderstorm has the potential to generate tornadoes and multiple tornadic activity, which can be difficult to predict.”

Meteorologists outside of the agency noted that forecasters in Jackson and other offices performed admirably during the tumultuous weekend but expressed concerns that operational pressures could overwhelm the already stretched staff.

“The tornado warnings were issued very effectively,” remarked Chris Vaguski, meteorologist and research program manager at Wisconet, a network of weather stations in Wisconsin, though he emphasized the uncertain long-term impact of staff fatigue.

“How do forecasters recover physically, mentally, and emotionally? Will this affect the quality of their warnings?” he inquired.

Vaguski noted that the warning time for tornadoes issued by the Jackson office exceeded 15 minutes, which is an improvement over the average performance.

Victor Gensini, a meteorology professor at Northern Illinois University, stated that while assessing the impact of staffing shortages is challenging, meteorological services may face declines in performance as fewer meteorologists are available for critical tasks.

“It’s challenging to evaluate performance based on a single significant event,” Gensini stated. “But we should prepare for a gradual decline in performance, though quantifying that impact may be difficult.”

Source: www.nbcnews.com

Astronomers Propose that X-ray and Ultraviolet Radiation Impact the Protoplanetary Disk in Cygnus OB2

Cygnus OB2 is the giant young stellar association closest to the Sun.

In this new composite image, Chandra data (purple) shows the diffuse X-ray emission and young stars of Cygnus OB2, along with infrared data (red, green, blue, cyan) from NASA's now-retired Spitzer Space Telescope reveals young stars. And it creates cold dust and gas throughout the region. Image credits: NASA / CXC / SAO / Drake others. / JPL-California Institute of Technology / Spitzer / N. Walk.

At a distance of approximately 1,400 parsecs (4,600 light years), Cygnus OB2 It is a huge young body closest to the Sun.

It contains hundreds of double stars and thousands of low-mass stars.

Dr. Mario Giuseppe Guarcero of the National Institute of Astrophysics, Dr. Juan Facundo Albacete Colombo of the University of Rio Negro, and colleagues used NASA's Chandra X-ray Observatory to study various regions of Cygnus OB2. observed.

This deep observation mapped the diffuse X-ray glow between the stars and also provided an inventory of young stars within the cluster.

This inventory was combined with other inventories using optical and infrared data to create the best survey of young stars within the association.

“These dense stellar environments are home to large amounts of high-energy radiation produced by stars and planets,” the astronomers said.

“X-rays and intense ultraviolet radiation can have devastating effects on planetary disks and systems that are in the process of forming.”

The protoplanetary disk around the star naturally disappears over time. Part of the disk falls onto the star, and some is heated by X-rays and ultraviolet light from the star and evaporates in the wind.

The latter process, known as photoevaporation, typically takes 5 million to 10 million years for an average-sized star to destroy its disk.

This process could be accelerated if there is a nearby massive star that produces the most X-rays and ultraviolet light.

researchers Found Clear evidence that protoplanetary disks around stars actually die out much faster when they approach massive stars that produce large amounts of high-energy radiation.

Also, in regions where stars are more densely packed, the disk dies out faster.

In the region of Cygnus OB2, which has less high-energy radiation and fewer stars, the proportion of young stars with disks is about 40%.

In regions with higher-energy radiation and more stars, the proportion is about 18%.

The strongest influence, and therefore the worst location for a star to become a potential planetary system, is within about 1.6 light-years of the most massive star in the cluster.

In another study, the same team I looked into it Characteristics of the diffuse X-ray emission of Cygnus OB2.

They discovered that the high-energy, diffuse radiation originates from regions where winds of gas blown from massive stars collide with each other.

“This causes the gas to become hot and generate X-rays,” the researchers said.

“The low-energy release is likely caused by gas within the cluster colliding with gas surrounding the cluster.”

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MG Guarcero others. 2024. Photoevaporation and close encounters: How does the environment around Cygnus OB2 affect the evolution of the protoplanetary disk? APJS 269, 13; doi: 10.3847/1538-4365/acdd67

JF Albacete vs Colombo others. 2024. Diffuse X-ray emission in the Cygnus OB2 coalition. APJS 269, 14;doi: 10.3847/1538-4365/acdd65

Source: www.sci.news