Quantum Communication with Extraterrestrials. Time to Revise the Current Experiment

Extraterrestrial (ET) communication is a subject that is fascinating to me. I have done a lot of research and composed several articles on the subject. Our historic attempts to send or receive a message from the cosmos have failed. Unless, of course, there is a giant government cover-up and conspiracy going on. A plot intended to keep the public in the dark on the matter.

The agencies charged with seeking that ET signal have been unable to follow the basic principles of the scientific method. They have had no success, yet they continue to do the same thing in the same way. They do it in the same way, hoping for a different result. Those are strong words from a guy not in the game at a professional level; however, it is a valid “hypothesis.”

The scientific method is a beacon illuminating the path of inquiry, discovery, and understanding in science. It is a systematic approach. It is a structured process that empowers scientists to unravel the natural world’s mysteries. Driven by empirical evidence and logical reasoning, the scientific method is a dynamic and iterative process that has fueled centuries of scientific progress.

The journey of discovery begins with a hypothesis based on imperial observation – a keen, curious gaze cast upon the world. Scientists, driven by an insatiable curiosity, observe natural phenomena, ask questions, and identify areas of interest. This initial step sets the stage for the scientific process, prompting the formulation of hypotheses and the framing of research questions.

Hypotheses emerge as tentative explanations for observed phenomena. These are educated guesses, informed by existing knowledge and guided by a desire to test and validate assumptions. Well-crafted hypotheses serve as the foundation for the subsequent stages of experimentation and analysis. The ET communication process has been established in part.

The heart of the scientific method beats in the laboratory or field where experimentation occurs. Rigorous investigation involves the manipulation of variables to test hypotheses. Scientists gather evidence supporting or refuting their initial assumptions through meticulous data collection. The reliability and validity of data are paramount, requiring precision and attention to detail. This part of the process in our search for an ET message has been going on for decades. It is going on at great expense with no results.

Data, the currency of scientific inquiry, undergo analysis to extract meaningful patterns and trends. Statistical methods and mathematical models help scientists discern the significance of their findings. The interpretation phase involves:

      • Connecting the dots.
      • Drawing conclusions based on empirical evidence.
      • Refining the understanding of the phenomena under investigation.

Data collection is the part of the ET communication experiment that has failed. The only data is that there is no data.

The process culminates in drawing conclusions that contribute to scientific knowledge. Most importantly, the scientific community is engaged in a continuous dialogue through peer review. Fellow scientists scrutinize, critique, and validate the experiment. Peer review acts as a quality control mechanism, upholding the standards of scientific inquiry.

The way I see it, concerning the ET communication experiment, there are two possibilities to consider. The first is that the investigation has proven that we are alone in the universe. The second is we are trying to communicate the wrong way. It is highly unlikely that that humans are the only intelligent life in the cosmos. Therefore, scientists must revise the experiment. 

Scientific knowledge is a dynamic that is subject to refinement and revision. The scientific method embraces the notion that understanding evolves with each process iteration. If new evidence is exposed, scientists must adapt their theories and hypotheses, perpetuating a continuous improvement cycle.

The scientific endeavor extends beyond the laboratory bench. Effective communication of findings through research papers, conferences, and publications is essential. Equally important is the concept of replication and the ability of other researchers to reproduce experiments and validate results independently. Replication reinforces the reliability of scientific discoveries and guards against anomalies or errors.  

While the scientific method is rigorous and objective, creativity and imagination are integral components. The formulation of hypotheses often requires creative insight, and the design of experiments demands innovative thinking. The interplay between structured methodology and creative exploration fuels the engine of scientific discovery.

The scientific method is not merely a set of procedural steps. The scientific method is a philosophy, a mindset that embraces skepticism, evidence-based reasoning, and a commitment to the pursuit of truth.

From the microscopic realm of subatomic particles to the cosmic expanses of the universe, the scientific method is humanity’s most potent tool for unraveling the intricacies of the natural world and expanding the frontiers of knowledge. It is a timeless guide, leading generations of curious minds on a quest for understanding and enlightenment.

I have published a book entitled Extraterrestrial Communication Code. The book ultimately develops a hypothesis about ET Communication based on observations. The theory is that ET communication efforts, using the same tools, need to identify a time and place from where to listen and send our ones and zeros messages.

What my book should have also considered is something called Quantum Communication. Quantum communication is a genuine and actively researched field within quantum information science. It harnesses the principles of quantum mechanics to enable secure and efficient communication between parties. Quantum mechanics is a fundamental branch of physics that deals with the behavior of matter and energy on minor scales, typically at the level of atoms and subatomic particles. It provides a mathematical framework to understand and predict the behavior of particles at the quantum level, where classical physics concepts break down. 

I will tell you that Quantum anything is complicated, and I do not pretend to be an expert or even a novice on how it all works. I aim to offer my readers the basics on how this could be a significant link to successfully establishing ET communication in our lifetime. Quantum Communication may be the adjustment to our current ET communication experiment that the scientific method demands. Scientists have achieved quantum communication. Several groundbreaking experiments and demonstrations have showcased the principles of quantum communication.

Humanity continues to turn its eyes and ears toward the stars with the prospect of communicating with extraterrestrial civilizations. The conventional means of communication, grounded in classical information theory, have proven inadequate for bridging the vast cosmic distances that separate us from potential extraterrestrial beings. Enter quantum communication, a revolutionary approach grounded in quantum mechanics principles, with the promise of transcending classical limits and establishing a cosmic dialogue with intelligence beyond our celestial borders.

At the heart of quantum communication with extraterrestrials lies the extraordinary entanglement phenomenon. Despite its mysterious and non-intuitive nature, quantum entanglement has been experimentally verified in various setups, and it remains one of the most intriguing aspects of quantum mechanics.

Quantum Communication continues to be a topic of research and exploration for its potential applications in quantum technologies and its implications for our understanding of the fundamental nature of reality.

If extraterrestrial civilizations harness quantum mechanics, this entanglement could serve as a cosmic bond, allowing instantaneous communication regardless of the immense distances that separate celestial bodies. Changes in the quantum state of particles entangled across cosmic expanses could convey messages faster than the speed of light, challenging the constraints imposed by classical communication.

In secure communication, quantum key distribution (QKD) emerges as a beacon of hope for ensuring the confidentiality of messages exchanged with extraterrestrial intelligence. The principles of QKD could enable the establishment of secure cryptographic keys, immune to eavesdropping even across the cosmic void. The secrecy of quantum keys, based on the fundamental principles of quantum mechanics, offers a level of security that classical cryptographic systems cannot match.

As cosmic distances present formidable challenges to preserving quantum information, the concept of quantum repeaters takes center stage. Quantum repeaters, akin to celestial relay stations, could extend the range of quantum communication systems, enabling the faithful transmission of quantum states over interstellar distances.

Overcoming the cosmic decoherence that threatens the integrity of quantum information becomes a pivotal step in establishing a robust quantum communication infrastructure with extraterrestrial civilizations.

The compelling concept of quantum teleportation enters the realm of cosmic communication. While not involving the physical movement of matter, quantum teleportation allows the transmission of quantum information between distant locations. Imagining a scenario where extraterrestrial civilizations employ quantum teleportation to exchange information across cosmic expanses opens avenues for instantaneous cosmic communication and collaboration.

In the quest for establishing a shared language with extraterrestrial intelligences, universal quantum languages, and mathematical constants emerge as potential communication mediums. Concepts like prime numbers or fundamental physical constants, rooted in the universality of mathematics, could serve as a cosmic Rosetta Stone by transcending linguistic and cultural barriers in our attempts to decipher extraterrestrial messages.

Envisioning a cosmic community of intelligent civilizations interconnected through quantum networks adds a layer of complexity to the dialogue. Quantum networks, linking diverse celestial entities, could facilitate the exchange of quantum information, knowledge, and cultural insights. The interplay of entangled particles across cosmic scales transforms the cosmos into a vast, interconnected quantum tapestry.

The fusion of quantum mechanics and cosmic exploration sparks the imagination in the speculative realm of quantum communication with extraterrestrials. While the technical and theoretical challenges are monumental, the allure of a heavenly dialogue conducted through the language of quantum physics propels us into uncharted territories.

As humanity contemplates its place in the cosmos, the vision of communicating with extraterrestrial intelligence through the wonders of quantum communication adds a profound and awe-inspiring dimension to our cosmic aspirations.

The journey towards understanding and connecting with other intelligent beings may well be guided by the principles of quantum mechanics, offering a heavenly bridge that transcends the limitations of classical communication methods.

It is time to recognize that our historic attempts at ET communication have failed. It is time to follow the scientific method and revise the experiment.

Sources:

Wikipedia / Britannica / Science News / Nature / The Institute of Engineering & Technology

Science Education Pioneer Guillermo Gonzalez

Guillermo Gonzalez is a prominent astrophysicist known for his contributions to astronomy and his work searching for extraterrestrial intelligence (SETI). Gonzalez was born on February 19, 1963, in Havana, Cuba. Academic excellence, research achievements, and engagement in broader scientific discussions have marked his career in astrophysics.

Guillermo Gonzalez (AP Photo/Nirmalendu Majumdar, File)

His family sparked his passion for the cosmos at an early age. They immigrated to the United States from Cuba when he was young, and this transition provided him with opportunities to pursue his scientific interests. Gonzalez earned his bachelor’s degree in physics and astronomy from the University of Arizona in 1987. His academic journey continued as he pursued a Ph.D. in astronomy from the University of Washington, which he completed in 1993.

Both research and teaching characterize his dedication. He held positions at various esteemed institutions, including the University of Washington, the University of Texas, Austin, and Iowa State University, where he served as an Assistant Professor of Physics and Astronomy.

One of Gonzalez’s significant contributions to astronomy is his research on the Galactic Habitable Zone. This concept posits that the location within a galaxy significantly influences a star system’s ability to support complex life. Gonzalez’s work in this area sheds light on the factors that contribute to a star’s habitability, considering aspects such as metallicity, radiation, and stable orbits.

In collaboration with Jay W. Richards, Gonzalez co-authored the book “The Privileged Planet: How Our Place in the Cosmos is Designed for Discovery.” The book explores the idea that Earth is habitable and uniquely positioned to allow for scientific discovery. It delves into the relationship between habitability and the ability to observe and comprehend the universe, presenting a thought-provoking perspective on the intersection of science and philosophy.

Gonzalez regularly contributed to Facts for Faith magazine, produced by Reasons To Believe, an old earth creationist group. Reasons to Believe is a nonprofit organization that promotes day-age forms of old Earth creationism. It was founded in 1986 by Hugh Ross, a Canadian-born astrophysicist and creationist Christian apologist. 

Christian apologetics is a branch of Christian theology that defends Christianity. It is a topic of theology has taken many forms over the centuries. It started with Paul the Apostle in the early church and included Patristic writers such as OrigenAugustine of HippoJustin Martyr, and Tertullian. Christian Apologetics continued with writers such as Thomas AquinasDuns ScotusWilliam of Ockham, and Anselm of Canterbury during Scholasticism.

Blaise Pascal was an active Christian apologist during the 17th century. In the modern period, the efforts of many authors defended Christianity. Some of these authors included John Henry NewmanG. K. ChestertonC. S. Lewis, and G. E. M. Anscombe.

 In the first century CE, according to Edgar J. Goodspeed, Jewish apologetic elements could be seen in works such as The Wisdom of SolomonPhilo’s On the Contemplative Life, and more explicitly in Josephus’ Against Apion.

Christian apologetics first appears in the New Testament (e.g., Paul’s preaching on Mars Hill in Acts 17:22-31). During the subapostolic age, Christianity already competed with Judaism and other religions and sects in the Greco-Roman world. Christian apologetics can be first seen in the “Preaching of Peter” (Gospel of Peter). The first explicitly apologetic work however, comes from Quadratus of Athens (c. 125 CE). In it he writes a defense of the faith to emperor Hadrian. Only a fragment, quoted by Eusebius, has survived to our day:

“But the works of our Saviour were always present, for they were genuine: those that were healed, and those that were raised from the dead, who were seen not only when they were healed and when they were raised, but were also always present; and not merely while the Saviour was on earth, but also after his death, they were alive for quite a while, so that some of them lived even to our day” (Church History iv. 3. 2)

In addition to Guillermo Gonzalez’s work for the Discovery Institute and the International Society for Complexity, Information, and Design, he is a researcher for the Biologic Institute, funded by the Institute for Research into Intelligent Design.

Guillermo Gonzalez became embroiled in controversies about his support for the theory of Intelligent Design (ID).

ID proposes that certain features of the universe and living organisms are best explained by an intelligent cause rather than an undirected process such as natural selection. Gonzalez’s advocacy for ID led to tensions within the academic community, and his tenure at Iowa State University was not renewed in 2007, a decision that sparked debates about academic freedom.

His stance on that issue and unwillingness to yield is a testament to the protection of critical thinking in education. He would not yield to the University’s closed-minded policy on the matter. He refused to be indoctrinated and pass that indoctrination policy on to his students. The world today needs more courageous teachers like Gonzales.

Gonzalez’s legacy extends beyond his specific research contributions. His work on the Galactic Habitable Zone has influenced discussions about the conditions necessary for life in the universe. While controversies surround his involvement in the Intelligent Design movement, Gonzalez remains an influential figure in astronomy.

Guillermo Gonzalez’s work as an astronomer encompasses significant contributions to our understanding of habitability in the cosmos. His research, teaching, and engagement with broader scientific and philosophical discussions have left an indelible mark on astronomy. 

Despite the controversies surrounding his advocacy for Intelligent Design, Gonzalez’s work continues to be a subject of scholarly discussion and debate.

 

The Extraterrestrial Communication Group welcomes Guillermo Gonzalez to our Hall of Fame Library.

Sources:

Wikipedia / Britannica / Discovery Institute

A Trailblazing Woman of Astronomy: Maria Mitchell: A

Maria Mitchell (1818-1889): A Trailblazing Astronomer

Maria Mitchell, an American astronomer born in 1818, is a pioneering figure in the history of astronomy. Her life and career were marked by a deep passion for the stars. She had an unyielding commitment to education, and a determination to break down social and gender barriers.

Maria Mitchell was born in Nantucket, Massachusetts, and was raised in an environment that encouraged intellectual curiosity and a love for learning. Maria Mitchell’s father was William Mitchell.

He was a dedicated amateur astronomer and a teacher who played a significant role in nurturing his daughter’s interest in astronomy and education. William Mitchell’s own passion for astronomy and his encouragement of Maria’s intellectual pursuits had a profound influence on her development as a scientist. Mitchell’s education was diverse and included exposure to mathematics, science, and the humanities. Her early education set the stage for her future endeavors.

One of Maria Mitchell’s most significant scientific achievements was the discovery of a new comet on October 1, 1847. This discovery, known as “Miss Mitchell’s Comet,” brought her international recognition. It made her the first American woman and the third woman in the world to discover a comet.

The fame she gained from this discovery was not only a testament to her observational skills but also a powerful assertion of women’s capabilities in the sciences.

Her primary instrument was a 5-inch aperture refracting telescope. This telescope, known as the “Great Refractor,” was made by the prominent American telescope manufacturer Henry Fitz, who was known for producing high-quality telescopes during the 19th century. The Great Refractor was installed at the Nantucket Atheneum library on Nantucket Island, Massachusetts. The Nantucket Atheneum was founded in 1834. It is one of the oldest public libraries in the United States. It was established by a group of Nantucket residents who shared a commitment to fostering education and intellectual pursuits. The telescope was placed in a dome on the rooftop of the Atheneum.

Mitchell used this telescope to make her historic comet discovery on October 1, 1847. The telescope’s quality and precision were instrumental in her ability to observe and document celestial objects.

In addition to her comet discovery, Maria Mitchell’s work in astronomy extended to pioneering photography as a tool for astronomical observations. She was one of the first astronomers to employ photography for capturing images of the stars. Mitchell also built her own telescopes and other astronomical instruments, exhibiting her versatility as a scientist and astronomer.

Mitchell’s dedication to studying celestial objects led her to compile extensive catalogs of stars, including their positions and characteristics. Her diligent work cataloging star positions was critical for navigation and astronomy. Mitchell’s work earned her a place at the American Nautical Almanac Office, where she contributed to the computation of navigational tables.

Beyond her groundbreaking scientific contributions, Maria Mitchell advocated for education, especially for women.

She believed that education should be accessible to all and fought for equal educational opportunities regardless of gender. Her teaching career at Vassar College, where she was the first woman appointed to a professorship in astronomy, was marked by her commitment to fostering young women’s interest in science.

Maria Mitchell’s legacy extends beyond her time as her groundbreaking achievements inspire and empower future female scientists and astronomers. Her life’s work served as a potent reminder that women could excel in fields traditionally dominated by men. She defied societal norms and paved the way for women in science, leaving an enduring mark on the history of astronomy and the broader scientific community.

In 1841, Mitchell attended the anti-slavery convention in Nantucket where Frederick Douglass made his first speech, and she also became involved in the anti-slavery movement by boycotting clothes made of Southern cotton. She later became involved in a number of social issues as a professor, particularly those pertaining to women’s suffrage and education. 

She also befriended various suffragists including Elizabeth Cady Stanton. After returning from a trip to Europe in 1873, Mitchell joined the national women’s movement and helped found the Association for the Advancement of Women (AAW), a group dedicated to educational reform and the promotion of women in higher education. Mitchell addressed the Association’s First Women’s Congress in a speech titled The Higher Education of Women in which she described the work of English women working for access to higher education at Girton College, Cambridge.

“The laws of Nature are not discovered by accident; theories do not come by chance, even to the greatest minds; they are not born of the hurry and worry of daily toil; they are diligently sought, they are patiently waited for, they are received with cautious reserve, they are accepted with reverence and awe. And until able women have given their lives to investigation, it is idle to discuss the question of their capacity for original work.”

Mitchell advocated for women working part-time while acquiring their education to not only ease the wages off of men paying for their education, but also to empower more women to be in the workforce. She also called attention to the place for women in science and mathematics and encouraged others to support women’s colleges and women’s campaigns to serve on local school boards. Mitchell served as the second president of the AAW in 1875 and 1876 before stepping down to head a special Committee on Science to analyze and promote women’s progress in the field. She held this position until her death in 1889.

Maria Mitchell’s telescope is on display in the Smithsonian Institution National Museum of American History.

 

Mitchell died of brain disease on June 28, 1889, in Lynn, Massachusetts at the age of 70. She was buried in Lot 411, in Prospect Hill Cemetery, Nantucket. The Maria Mitchell Association was established to promote the sciences on Nantucket and preserve the legacy Mitchell’s work. The Association operates a Natural History Museum, an Aquarium, a Science Library and Research Center, Maria Mitchell’s Home Museum, and an Observatory named in her honor, the Maria Mitchell Observatory.

In 1989, Mitchell was named a National Women’s History Month Honoree by the National Women’s History Project and was inducted into the National Women’s Hall of Fame in 1994. She was the namesake of a World War II Liberty ship, the SS Maria Mitchell, and New York’s Metro North commuter railroad (with its Hudson Line endpoint in Poughkeepsie near Vassar College) has a train named the Maria Mitchell Comet. A crater on the Moon was also named in her honor.   

Her unique place at the intersection of American science and culture has been captured in a number of publications. During her life, Mitchell published seven items in the Royal Society Catalog and three articles detailing her observations in Silliman’s Journal. Mitchell also authored three articles for Hours at HomeCentury, and The Atlantic.

Her story serves as an inspiration for all those who strive to overcome obstacles and make meaningful contributions to the advancement of human understanding.

“The progress of the intellect is to the clearer vision of causes, which neglects surface differences. To the poet, to the philosopher, to the saint, all things are friendly and sacred, all events profitable, all days holy, all men divine.”– Maria Mitchell

Maria Michel’s story is now a well deserving member of the Extraterrestrial Communication Group Hall of Fame Library

Sources:

Wikipedia

Britannica

Womans Natural History Museum: Maria Mitchell

Science, Faith and Education in America

I am trying to understand all of the increasing violence and twisted social, political, and ethical issues burning in virtually every country of the world today. Why is it happening? How do we fix it?

Rockets are still aimed at people to this day despite the lessons of history. How is it possible that one group of people can have such hate for another that they will raid their homes and brutalize women and children? What drives a man to chop off the head of a baby and feel as though he is doing the right thing?

How is it possible that gender identity issues and sexuality are being brought into public grade schools and put before children who still believe in the tooth fairy, the Easter Bunny, and Santa Claus? It seems like either pure evil or pure insanity or possibly both.

I believe that the root cause lies within a diminished educational balance that includes science and religion. Education is the cornerstone of progress, and the curriculum shapes the minds of future generations.

The following is my opinion on the matter based on some research of the underlying facts. 

Over recent years, there has been a documented trend away from science education in many educational systems in America and worldwide. One of the most profound challenges facing contemporary education systems is this shift away from science education. This decline in science education in American institutions is proving to be trend of critical concern.  

Excited girls using chemistry set together in elementary science classroom

Restoring science education to its rightful place in the curriculum ensures that future generations possess the knowledge and critical thinking skills required. This knowledge is necessary for a society that relies on science and technology for progress and innovation. Balancing the curriculum, improving teacher training, and depoliticizing science education are critical steps. Steps in a process to address these concerns and strengthen science education worldwide.  

Several factors contribute to this shift away from an education that includes a strong science component:

Education systems, especially in the United States, often prioritize subjects directly assessed in standardized tests.

Science, particularly in early education, receives less emphasis as it is not a primary focus of standardized assessments.

Schools need more money. Lack of funding results in fewer science courses, outdated equipment, and insufficient opportunities for hands-on learning.

Educators need more training to teach science effectively. More qualified teachers can make it easier for students to engage with scientific concepts.

Parents play a critical role in shaping the educational experiences of their children.

If parents have limited understanding or appreciation for science, they tend to not prioritize it in their children’s education. It has become a generational issue. 

The shift away from science education has several implications:

A reduced emphasis on science in education results in a less scientifically literate society. This reduced emphasis limits individuals’ ability to understand and engage with significant scientific and technological developments. In an increasingly complex and technology-driven world, scientific literacy is crucial for informed decision-making and active citizenship.

Scientific knowledge and critical thinking skills are essential for innovation. A weaker emphasis on science hinders our nation’s ability to compete globally and advance technologically. Science education fosters innovation and entrepreneurship, contributing to economic growth and development.

A lack of science education leads to insufficient understanding of critical issues such as climate change, health, and other environmental concerns. This lack of knowledge can have long-term consequences. Many of the world’s most pressing challenges, such as climate change and pandemics, require a scientifically informed public and a skilled workforce to address them.

Most children are naturally curious about the world. Science education helps nurture that curiosity. A reduced emphasis on science education stifles this innate desire to explore and understand. Science education encourages critical thinking, problem-solving, and interest. All are valuable components of personal and intellectual development.

Education plays a pivotal role in shaping the perspectives and values of future generations. In recent years, there has been increased attention to the influence of a left-wing agenda in educational institutions. The left-wing political agenda is often championed for its emphasis on social justice, government intervention, and equality. It has gained prominence in many countries, particularly in America. 

The rise of the left-wing agenda in educational institutions is a complex and controversial issue. It raises crucial questions about ideological diversity, academic freedom, and the role of education in society.

The left-wing educational agenda has grown into an educational monster that has crossed over the line from inappropriate indoctrination into the land of brainwashing young minds for the sole purpose of promoting a very scary social agenda.

Often times these kids don’t seem to truly know what they are saying and doing or why they are saying and doing it. They are just repeating the words of others without question. It is a terrifying situation we live within our world today.  

The left-wing political agenda raises significant concerns about the balance between government intervention and individual freedom, economic implications, and the preservation of cultural and traditional values. The left-wing agenda seeks to address social and economic challenges. Its critics contend that its approach does not strike the right balance between promoting equality and respecting personal liberties.

Engaging in open dialogue and constructive debate between different political perspectives is crucial for finding solutions that address the complex issues facing our societies today.

Critics argue that left wing curriculum, particularly in the humanities and social sciences, tends to emphasize left-leaning ideologies, such as social justice, identity politics, and critical race theory. It does this while marginalizing or neglecting conservative viewpoints.

Concerns about the political leanings of faculty and staff are raised. There is a left-leaning dominance and the lack of conservative representation within higher education.

There is a growing atmosphere of political correctness, safe spaces, and trigger warnings, which are directly linked to the stifling of free speech and promoting a progressive ideological echo chamber.

The left-wing agenda in educational institutions has raised several concerns. A lack of political diversity among faculty and staff can lead to a one-sided presentation of ideas and hinder constructive debate.

Promoting particular values may undermine the educational mission of fostering critical thinking and independent inquiry. (AKA Indoctrination).

Conservative students often feel marginalized or hesitant to express their viewpoints, fearing backlash or negative consequences.

The educational results we are seeing and living with in today’s world demonstrate the need for ideological diversity, academic freedom, and the role of education in society. To address these concerns, educational institutions must foster open dialogue, encourage a balanced representation of ideas, and reaffirm their commitment to critical thinking, intellectual diversity, and academic freedom. 

There is a religious component to this discussion to consider as well. There is a direct correlation between the removal of religious education for younger students and the decline in social and moral behavior as these children move into adulthood.

The role of religion in grade school education has long been a subject of debate. As societies become more diverse and secular, there has been an increasing call for the removal of religion from grade school education. This exclusion is a substantial component of the root-cause analysis to identify the causes of moral decay in modern society.

One of the primary arguments for removing religion from grade school education is the promotion of secularism and inclusivity. The idea is that public education should be neutral and free from religious bias. This neutrality ensures that all students, regardless of their faith or lack thereof, feel welcome and respected.

Critics of religious education in any public school, express concerns about the potential for religious indoctrination. They argue that exposing young and impressionable minds to spiritual teachings may lead to the undue influence of one particular faith or belief system. In increasingly diverse societies, there is recognition of the wide range of religious and non-religious beliefs. Removing religious content from the curriculum helps avoid favoring one religion over another and respects the pluralistic nature of modern communities. 

Advocates for the removal of religion from grade school education emphasize parental rights. They argue that parents should be primarily responsible for teaching their children about their religious beliefs, and the state should not infringe on this right. All of that can appear logical at face value; however, there is much more to it than that. It is strange and disturbing to me that these same people hypocritically believe it is proper for public schools to teach sexual identity and gender topics to these very young children. Even worse – to do it or try to do it without parental knowledge. It’s just not right in my mind and in my opinion. It is a root cause to the bigger problem we are talking about. 

Religion has played a significant role in shaping the culture and history of many societies. Critics argue that understanding the religious foundations of art, literature, history, and community is essential for a well-rounded education. Religion often provides a framework for moral and ethical education. It teaches values such as compassion, empathy, and respect for others. These teachings can have a positive impact on character development.

Teaching about religion (rather than religious instruction) makes it possible to teach students about different religious beliefs without promoting one over the others. This educational approach fosters tolerance and understanding. Teaching about religion offers educational value by exploring its influence on art, history, literature, and culture. Learning about religious beliefs and practices is academically enriching and contributes to a well-rounded education.

The debate over the removal of religion from grade school education is a complex one. It requires a careful balance between promoting secularism, respecting religious diversity, and recognizing the educational value of spiritual knowledge. A possible compromise involves teaching about religion in an objective, inclusive, and non-indoctrinating manner.

This can be achieved while at the same time, ensuring that parents’ rights are respected and honored, and the educational environment remains inclusive and respectful of all students. It is a mistake for the educators of our young children to think they should exclude parents from the development and teaching of a curriculum for their children.  

The removal of religion from grade school education has clearly had an enormous impact on the moral decay of society on a global scale, especially in America. Religious freedom played a significant role in the founding of America.

We have forgotten (or not taught at a young age) that religious freedom is the backbone of the American experiment. The early European settlers who came to the American colonies sought religious freedom and refuge from religious persecution in their home countries.

For example, the Pilgrims, who arrived on the Mayflower in 1620, sought religious freedom and the ability to practice their form of Protestant Christianity without persecution. Similarly, the Puritans who settled in the Massachusetts Bay Colony in the early 17th century were motivated by religious reasons. Maryland was a refuge for Catholics, and Pennsylvania was settled by Quakers who sought a place to practice their faith without interference.

The importance of religious freedom is enshrined in the First Amendment to the United States Constitution, which states:

“Congress shall make no law respecting an establishment of religion or prohibiting the free exercise thereof.” 

The First Amendment reflects the Founding Fathers’ commitment to ensuring that individuals in the newly formed United States were free to practice their religion or no religion without fear of persecution. While the American colonies were settled for various reasons, including economic and political ones, pursuing religious freedom was undoubtedly a significant driving force in the founding of the United States.

Striking an educational balance that respects the rights and beliefs of all students while recognizing the educational value of religious knowledge is essential. In this ongoing debate, it is crucial to engage in open dialogue and thoughtful consideration to find the most appropriate and inclusive approach to religious education in an increasingly diverse and secular world.

A well-rounded education should expose students to various perspectives, allowing them to think critically and make informed decisions as they navigate an increasingly complex world.

The shift away from science education is a trend that has important implications for society, education, and individual growth. There is an urgent need to reemphasize the importance of science education backed by an understanding of world religions. This focus will prepare future generations to navigate a rapidly changing world. Receiving this sort of education, I suspect that the moral issues of modern society will improve organically.

As Benjamin Franklin, one of our Founding Fathers, once stated:

“Take care of the pence, and the pounds will care for themselves.”

It is a statement something that I see as applicable to education. Take care of the building blocks of science and religious education (the pence) and a society’s morality (the pounds) will take care of itself by default. 

Achieving this requires proper funding, resources, teacher training, and a shift in societal attitudes toward science and faith in our educational system. By doing so, we can ensure that science and religion remain at the forefront of education, fostering a more scientifically literate, innovative, and engaged society.

I invite you to visit the ECG’s Library to find and enjoy additional articles and news about the historic people of Science, current events and posts about the cosmos and our place within it. 

Sources:

  1. National Science Foundation (NSF) Website
  2. “Science Education in the United States: An Analysis of Policy and Practice” by the National Academies of Sciences, Engineering, and Medicine
  3. “Religion in the Public Schools” by the National Center for Science Education (NCSE)
  4. “Social Impact of Progressive Policies” by the Center for American Progress
  5. “The Ideological Origins of the American Revolution” by Bernard Bailyn

 

Anaximander of Miletus: An Ancient Philosopher and Astronomer of “Boundless” Thinking

You might be familiar with the works of Aristotle, Socrates, and Plato due to their contributions as early Greek scholars. Have you ever heard about Anaximander, the first philosopher to make massive changes to the astronomical world and natural philosophy?

He was a pre-Socratic philosopher, predating the typical study of Greek scholars. That’s probably why you never heard of him.

When studying ancient Greek thinkers, it is natural to place them in specific categories including philosopher, astronomer, biologist, or physician. Two thousand years ago these distinctions didn’t exist. The great minds of the ancient world seldom limited themselves to a specific topic of study, as we do today. For them, there was no distinction between what we now call “science” and “philosophy.”

The line between science and philosophy can often be a blurred one. The difference is that science depends on observations and experimentation, and it produces a “result,” whereas philosophy depends on logical arguments and doesn’t necessarily have to produce a “result.”

Anaximander of Miletus, a thinker of the pre-Socratic era, is a remarkable figure in the history of philosophy and astronomy. Living around 610-546 BCE in the ancient Greek city of Miletus, Anaximander made profound contributions to cosmology, biology, and metaphysics.

His philosophical ideas laid the foundation for a more rational and systematic approach to understanding the natural world, marking a significant shift from mythological explanations to early scientific thought.

In the 2017 essay collection Anaximander in Context: New Studies on the Origins of Greek Philosophy, Dirk Couprie, Robert Hahn, and Gerald Naddaf describe Anaximander’s mind as “one of the greatest minds in history.” Couprie goes on to state that he considers him on par with Newton.

Anaximander is the first scholar to write a book on Natural Philosophy, which paved the path for many contemporary philosophers. His book “On Nature” argued for the concept of the Aperion. 

The apeiron concept is his most enduring contribution to philosophy. He postulated that an underlying, boundless, and indefinite principle was the source of all things. According to Aristotle and Theophrastus, the first Greek philosophers were looking for the “origin” or “principle” (the Greek word “archê” has both meanings) of all things. Anaximander identified it with “the Boundless” or “the Unlimited” (Greek: “Apeiron,” that is, “that which has no boundaries”).

“Everything has an origin or is an origin. The Boundless has no origin. For then, it would have a limit. Moreover, it is both unborn and immortal, a kind of origin. For that which has become has also, necessarily, an end, and there is a termination to every process of destruction”.

Most of this book is unidentified as the fragments are lost in time. A primary source is his successor, Theophrastus, who referenced some parts of “On Nature” and was a follower of Anaximander’s accounts of Geography, Biology, and Astronomy.

Anaximander never fully or clearly explained explain what he meant by “the Boundless.” More recently, authors have disputed whether the Boundless should be interpreted spatially or temporarily without limits, perhaps as that which has no qualifications or as inexhaustible. Some scholars have even defended the meaning as:

“That which is not experienced” by relating the Greek word “Apeiron” not to “peras” (“boundary,” “limit”) but to “perao” (“to experience,” “to apperceive”).

The Greeks in those days were familiar with the idea of the immortal Homeric gods. Anaximander added two distinctive features to the concept of divinity:

        • Boundless is an impersonal something, and
        • Boundless is not only immortal but also unborn.

“All the heavens and the worlds within them” have sprung from “some boundless nature.”

This concept directly challenged prevailing mythological explanations for the origins of the cosmos.

Anaximander’s life and background are essential for understanding his philosophical contributions. Born in Miletus, a thriving city of Ionia, he was a contemporary of Thales, another prominent pre-Socratic philosopher. His background likely included exposure to the cosmopolitan culture of Ionia and its connection to the broader Mediterranean world. 

Anaximander is credited as the first Greek geographer to attempt the map of our world, at least according to ancient observers. It was not unusual to use regional maps in the olden times. However, the thought of mapping out the whole globe was much more novel. Only after Anaximander started this endeavor, Hecataeus of Miletus, who was a traveler, attempted making the perfect map out of his predecessor’s creation while improving on it. 

He did not restrict his thinking to astronomy and geography. Anaximander extended his philosophical inquiries into the realm of biology. He theorized about evolution, concluding that life first arose in wet rather than dry conditions.  He sought to explain the origins and development of life, suggesting that humans and animals evolved from simpler forms. His ideas were among the earliest precursors to the theory of evolution.

Anaximander developed a unique cosmological model that challenged traditional beliefs about the Earth’s centrality in the cosmos.

He proposed a universe where the Earth was not at the center but a celestial body in its own right. Three propositions, which make up the core of Anaximander’s astronomy, are a tremendous jump forward and constitute the origin of our Western concept of the universe. His astronomical speculations are as follows:

Celestial bodies make full circles and pass beneath the Earth.
The Earth floats free and unsupported in space.
The celestial bodies lie behind one another.

The idea that the celestial bodies, in their daily course, make complete circles and thus pass beneath the Earth – from Anaximander’s viewpoint – is so self-evident to us that it is hard to understand how daring its introduction was.

That the celestial bodies make full circles is not something he could have observed but a conclusion he must have drawn. 

 

 

His cosmological ideas laid the foundation for future astronomers and philosophers to explore the universe’s structure.

Among many of his other inventions, Anaximander was also responsible for introducing the gnomon and sundial into Greek culture. He traveled to Sparta to set up a gnomon, a simple pillar that is fixed straight over markings on the ground, representing a dial. Based on the shadows cast by the pillar and their interaction with the markings, one could accurately tell the time.

His philosophical ideas left a lasting imprint on the development of Greek thought and Western philosophy. He was crucial in the transition from mythological explanations to a more systematic and rational approach to understanding the natural world.

Anaximander of Miletus stands as a foundational figure in the history of philosophy. His ideas on the apeiron, cosmology, and biology challenged traditional beliefs and paved the way for future generations of thinkers to explore the mysteries of the universe.

His legacy survives as a testament to human curiosity, intellectual courage, and the timeless quest for understanding the world in which we live.

He is our latest ECG Hall of Fame Library addition.

Sources:

World History Encyclopedia – Joshua J. Mark

Internet Encyclopedia of Philosophy

Wikipedia

 

Cecelia Payne-Gaposchkin: Harvard’s First Woman PhD in Astrophysicist and Much More

Spotlight on Cecelia Payne-Gaposchkin:

 Cecilia Payne-Gaposchkin (born Cecilia Helena Payne; May 10, 1900 – December 7, 1979) was a British-born American astronomer and astrophysicist. In 1925, she became the first woman to earn a PhD in astronomy at Harvard University. In 1956, she became the first woman to be promoted to full professor from within the faculty at Harvard’s Faculty of Arts and Sciences. Payne was the first ever recipient of the Annie J. Cannon Award in Astronomy

 She was appointed the Phillips Professor of Astronomy in 1958. Later, with her appointment to the Chair of the Department of Astronomy, she also became the first woman to head a department at Harvard.

In her 1925 doctoral thesis, she proposed that stars were composed primarily of hydrogen and helium. Her thesis title was Stellar Atmospheres: A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars

Her groundbreaking conclusion was initially rejected. In 1925, her theory ran counter to the prevailing idea that stars had a composition similar to that of the Earth, so her work was ignored. Four years later, Independent observations eventually proved she was correct.

In 1962, her thesis was famously described as the most brilliant PhD thesis ever written in the field of astronomy. Her work on the nature of variable stars was foundational to modern astrophysics.

Cecilia Payne began school in Wendover at a private school run by Elizabeth Edwards. She was 12 when her mother moved to London for the sake of the education of Cecilia’s brother Humfry. He later became an archaeologist. Cecilia attended St Mary’s College, Paddington, where she was unable to study much mathematics or science.

In  1918 she changed schools for St Paul’s Girl School. There she was urged to pursue a career in music, but she preferred to focus on science. The following year she won a scholarship that paid all her expenses at Newnham College, Cambridge University.

Her interest in astronomy began after she attended a lecture by Arthur Eddington on his 1919 expedition to the island of Príncipe in the Gulf of Guinea off the west coast of Africa to observe and photograph the stars near a solar eclipse as a test of Albert Einstein’s general theory of relativity. She said of the lecture:

“The result was a complete transformation of my world picture. My world had been so shaken that I experienced something very like a nervous breakdown.”

She completed her studies, but she was not awarded a degree because of her sex.  Cambridge did not grant degrees to women until 1948.

Payne realized that her only career option in the U.K. was to become a teacher, so she looked for grants that would enable her to move to the United States. She was introduced to Harlow Shapley, the Director of the Harvard College Observatory. Harlow had just established a graduate program in astronomy. Payne left England in 1923. This was made possible by a fellowship to encourage women to study at the observatory. 

Adelaide Ames was the first student on the fellowship in 1922. Payne was the second the following year. She was described by renowned astrophysicist   Lawrence H. Aller as one of the “most capable go-getters” in Shapley’s group.

After her doctorate, Payne studied stars of high luminosity to understand the structure of the Milky Way. Later she surveyed stars brighter than the tenth magnitude. She then studied variable stars, making over 1,250,000 observations with her assistants. This work later was extended to the Magellanic Clouds, adding a further 2,000,000 observations of variable stars. These data were used to determine the paths of stellar evolution.

She published her conclusions in her second book, The Stars of High Luminosity (1930). Her observations and analysis of variable stars, carried out with her husband, Sergei Gaposchkin, laid the basis for all subsequent work on such objects.

Payne-Gaposchkin remained scientifically active throughout her life, spending her entire academic career at Harvard. When she began, women were barred from becoming professors at Harvard, so she spent years doing less prestigious, low-paid research jobs. Her work resulted in several published books, including The Stars of High Luminosity (1930), Variable Stars (1938), and Galactic Structure (1954).

Shapley had made efforts to improve her position, and in 1938, she was given the title of “Astronomer.” Her title was later changed, at her request, to Phillips Astronomer. This was an endowed position, which would make her an “officer of the university”.

In order to get approval for her title, Shapley assured the university that giving Payne-Gaposchkin this position would not make her equivalent to a professor, but privately pushed for the position to be later converted into an explicit professorship as the “Phillips Professor of Astronomy”. She was elected a Fellow of the American Academy of Arts and Sciences in 1943. Her courses were not recorded in the Harvard University catalogue until 1945.

 When Donald Menzel became Director of the Harvard College Observatory in 1954, he tried to improve her appointment, and in 1956 she became the first woman to be promoted to full professor from within the faculty at Harvard’s Faculty of Arts and Sciences. She was appointed the Phillips Professor of Astronomy in 1958. Later, with her appointment to the Chair of the Department of Astronomy, she also became the first woman to head a department at Harvard.

Her students included Helen Sawyer HoggJoseph AshbrookFrank DrakeHarlan Smith and Paul W. Hodge, all of whom made important contributions to astronomy.  She also supervised Frank Kameny and Owen Gingerich.

Payne-Gaposchkin retired from active teaching in 1966. She was subsequently appointed Professor Emerita of Harvard. She continued her research as a member of staff at the Smithsonian Astrophysical Observatory, as well as editing the journals and books published by Harvard Observatory for ten years.

Payne’s career marked a turning point at Harvard College Observatory. The trail she blazed into the male-dominated scientific community was an inspiration to many. For example, she became a role model for astrophysicist Joan Feynman. Feynman’s mother and grandmother had dissuaded her from pursuing science, since they believed women were not physically capable of understanding scientific concepts.  Feynman was inspired by Payne-Gaposchkin when she came across her work in an astronomy textbook. Seeing Payne-Gaposchkin published research convinced Feynman that she could, in fact, follow her scientific passions.

 While accepting the Henry Norris Russell Prize from the American Astronomical Society, Payne spoke of her lifelong passion for research:

“The reward of the young scientist is the emotional thrill of being the first person in the history of the world to see something or understand something. Nothing can compare with that experience.  The reward of the old scientist is the sense of having seen a vague sketch grow into a masterly landscape.”

Cecilia Helena Payne-Gaposchkin died of lung cancer on December 7, 1979, at age 79.  She received several prestigious awards and honorary degrees throughout her career. Some posthumous recognitions include Asteroid 2039 Payne-Gaposchkin, the Payne-Gaposchkin Patera (volcano) on Venus, and the Institute of Physics Cecilia Payne-Gaposchkin Medal and Prize.

Her autobiography was first published in 1979, privately as The Dyer’s Hand and in 1984, publicly as Cecilia Payne-Gaposchkin: An Autobiography and Other Recollections.

We are privileged to include Cecilia Payne-Gaposchkin  in our ECG Hall of Fame – Women of Science.

Sources:

Wikipedia / Britannica / Space.com

 

 

Spotlight on Johannes Kepler: Much more than just an Astronomer

Johannes Kepler was born December 27, 1571, in Weil der Stadt, Württemberg [Germany]. He died November 15, 1630, Regensburg)

Kepler was a German astronomer, mathematician, astrologer, natural philosopher and writer on music. He was a key person of influence in the 17th-century Scientific Revolution.

Kepler is best known for his laws of planetary motion, and his books Astronomia novaHarmonice Mundi, and Epitome Astronomiae Copernicanae. 

His work was of great influence on Isaac Newton and many others. Kepler provided the foundational theory of universal gravitation. The variety and impact of his work made Kepler one of the founders of modern astronomy, the scientific method and natural science in general. 

Kepler’s God was a dynamic, creative being whose presence in the world was symbolized by the Sun’s as the dynamic force that continually moved the planets. The natural world was like a mirror that precisely reflected and embodied these divine ideas.

Inspired by Platonic notions of the soul, Kepler believed that the human mind was ideally created to understand the world’s structure.

“I used to measure the heavens,
now I shall measure the shadows of the earth.
Although my soul was from heaven,
the shadow of my body lies here”.

Kepler was not alone in believing that nature was a book in which the divine plan was written. He differed, however, in the original manner and personal intensity with which he believed his ideas to be embodied in nature. One of the ideas to which he was most strongly attached was the image of the

Christian Trinity as symbolized by a geometric sphere. The visible, created world, was literally a reflection of this divine mystery (God the Father: center; Christ the Son: circumference; Holy Spirit: intervening space).

One of Kepler’s favorite biblical passages came from John (1:14).

 

And the Word became flesh and lived among us.”

For him, this signified that the divine archetypes were literally made visible as geometric forms that configured the spatial arrangement of tangible entities.

Kepler was the astronomer who discovered the three major laws of planetary motion

    1. Planets move in elliptical orbits with the Sun at one focus.
    2. The time necessary to traverse any arc of a planetary orbit is proportional to the area of the sector between the central body and that arc (the “area law”).
    3. There is an exact relationship between the squares of the planets’ periodic times and the cubes of their mean distances from the Sun (the “harmonic law”). 

Kepler himself did not call these discoveries “laws”. It became the customary term after Isaac Newton derived them from a new and different set of general physical principles. He regarded them as celestial harmonies that reflected God’s design for the universe.

Kepler’s discoveries turned Nicolaus Copernicus’s Sun-centered system into a dynamic universe. He discovered that the Sun is actively pushing the planets around in non-circular orbits. It was Kepler’s notion of a physical astronomy that fixed a new problem for other important 17th century world-system builders, the most famous of whom was Newton.

Among Kepler’s many other achievements, he provided a new and correct account of how vision occurs. He developed a novel explanation for the behavior of light in the newly invented telescope.

The history of the telescope can be traced to before the invention of the earliest known telescope, which appeared in 1608 in the Netherlands. A patent was submitted by Hans Lippershey, an eyeglass maker. Although Lippershey did not receive his patent, news of the invention soon spread across Europe. The design of these early refracting telescopes consisted of a convex objective lens and a concave eyepiece. Galileo improved on this design the following year and applied it to astronomy.

In 1611, Kepler described how a far more useful telescope could be made with a convex objective lens and a convex eyepiece lens. By 1655, astronomers such as Christian Huygens were building powerful but unwieldy Keplerian telescopes with compound eyepieces.

Kepler discovered several new, semi-regular polyhedrons. He also offered a new theoretical foundation for astrology. The list of his discoveries, however, fails to convey the fact that they constituted for Kepler, part of a common body of knowledge. His matrix of theological, astrological, and physical ideas from which his scientific achievements emerged is unusual and fascinating in its own right.

The highly original nature of Kepler’s discoveries requires an act of intellectual empathy for modern science to understand. How could have such lasting results evolved from such an unlikely complex set of ideas. He is considered by the modern scientific community as a bit of a scientific enigma.

Although his scientific work was centered primarily on astronomy, it was classified as part of a wider subject of investigation called “the science of the stars.”

The science of the stars was regarded as a mixed science consisting of a mathematical and a physical component. It bore a kinship to other like disciplines, such as music (the study of ratios of tones) and optics (the study of light). It also was subdivided into theoretical and practical categories.

Kepler believed the theoretical principles of astrology had a corresponding practical part that dealt with the making of annual astrological forecasts about individuals, cities, the human body, and the weather. Within this framework, Kepler made astronomy an integral part of natural philosophy, but he did so in an unprecedented way.

Astronomers looking to the sky — Scanned 1870 Engraving

There was no “scientific community” as such in the late 16th century. All schooling in Germany, as elsewhere, was under the control of church institutions. This was primarily Roman Catholic or Protestant. Local rulers used the churches and the educational systems as a means to consolidate the loyalty of their populations.

One means to this end was a system of scholarships for poor boys who, once having been trained in the schools of the duchy (territory of the duke), would feel strong loyalty to the local ruler. 

Kepler came from a very modest family in a small German town called Weil der Stadt and was one of the beneficiaries of the ducal scholarship. This made possible his attendance at the Lutheran Stift, or seminary, at the University of Tübingen, in 1589. It was expected that the boys who graduated from these schools would go on to become schoolteachers, ministers, or state functionaries. Kepler had planned to become a theologian.

 People have always named things after people who have done great things. Most people with an interest in science and Astronomy have heard of the Kepler telescope (image on left) launched by NASA in 2009 but is no longer in service today. Here is a list of just some of the many other things that were named after Kepler out of respect for his contributions to Science and Astronomy:

Kepler conjecture    Kepler triangle      Kepler–Bouwkamp constant    

Kepler–Poinsot polyhedron

Kepler’s laws of planetary motion 

Kepler’s equation      Keplerian elements   Kepler problem   

  Kepler problem in general relativity

Kepler space telescope   Kepler Launch Site

Kepler photometer   Keplerian telescope   Kepler refractor   Johannes Kepler ATV

Kepler (lunar crater)   Kepler (Martian crater)   Kepler Dorsum   1134 Kepler

Kepler orbit   Kepler Object of Interest   Kepler-11   Kepler-22     Kepler-22b

Kepler’s Supernova   Kepler Follow-up Program        Kepler Input Catalog

Kepler scientific workflow system   Kepler Mire   Kepler Museum   Kepler Track

Kepler College   Johannes Kepler University Linz     

Kepler clearly made his mark on the scientific community. The ECG is proud to include Johannes Kepler in our Hall of Fame Library

Sources:

Wikipedia

The Editors of Encyclopedia Britannica

Earth Magnetism & Wormholes During Equinox Events

I have authored two books on the subject of extraterrestrial (ET) communication. Extraterrestrial Communication Code was published in February of 2021. The other, Angel Communication Code, will be published before the end of 2023. Each book demonstrates that it is possible for wormholes to appear at a specific location on the earth during equinox events.

This how it is possible to close the gap in time and distance necessary to establish ET communication. It is also how ETs have been able to come and go from earth for hundreds if not thousands of years.

 

ET communication is one of the primary motivators in why we continue to experiment and explore the universe.

The problem is that the existence of wormholes in the universe remains a theoretical construct based on the equations of Einstein.

“Wormholes” are cosmic tunnels that can connect two distant regions of the universe. They have been popularized by the dissemination of theoretical physics and by works of science fiction. 

By using present-day technology, it would seemingly be impossible to create a gravitational wormhole. The field would have to be manipulated with huge amounts of gravitational energy, which no one knows how to generate. In electromagnetism, however, advances in metamaterials and invisibility have allowed researchers to put forward several designs to achieve this.

Scientists in the Department of Physics at the Universitat Autònoma de Barcelona have designed and created, in the laboratory, the first experimental wormhole. They actually connected two regions of space magnetically. The experiment consisted of a tunnel that transferred a magnetic field from one point to the other while keeping it undetectable and invisible all the way.

Researchers used metamaterials and metasurfaces to build the tunnel experimentally, so that the magnetic field from a source, such as a magnet or an electromagnet, appears at the other end of the wormhole as an isolated magnetic monopole.

This result is strange as magnetic monopoles or magnets with only one pole do not exist in nature to the best of our current knowledge. The overall effect is that of a magnetic field which appears to travel from one point to another through a dimension that lies outside the conventional three dimensions. [1]

Science has long believed that:

  1. Magnetism and magnetic fields could somehow be involved in how space craft can traverse lightyears of distance.
  1. Wormholes are a necessary construct for (physical) intergalactic space travel.
  1. ET spacecrafts are probably constructed of materials not known to us on earth or “metamaterials”.

One of the hurdles in going universal with this wormhole creation idea is the need for huge amounts of gravitational force in conjunction with the metamaterials and huge magnetic field. Perhaps the huge magnetic field problem can be solved via the changing magnetic field of the earth during equinox events.

We have used the earth’s gravity to launch space craft since the beginning of human space travel. It is called the slingshot effect.

When a spacecraft launches on a mission to another planet it must first break free of the Earth’s gravitational field. Once it has done that, it enters interplanetary space, where the dominant force is the gravitational field of the Sun.

The spacecraft begins to follow a curving orbit, around the Sun, which is similar to the orbit of a comet. When this orbit brings it close to its target destination the spacecraft must fire a retrorocket to slow down and allow itself to be captured by the gravitational field of its target. The smaller the target, the more the spacecraft must slow down.

Sometimes passing a planet can result in the spacecraft being accelerated, even without the spacecraft firing any of its thrusters. This is known as the ‘slingshot’ effect. 

Such ‘gravity assist’ maneuvers are now a standard part of spaceflight and are used by almost all interplanetary missions. They take advantage of the fact that the gravitational attraction of the planets can be used to change the trajectory and speed of a spacecraft.

The amount by which the spacecraft speeds up or slows down is determined by whether it is passing behind or in front of the planet as the planet follows its orbit.  When the spacecraft leaves the influence of the planet, it follows an orbit on a different course than before.

For example, the Rosetta mission launched in 2004 and is using slingshot maneuvers to reach its destination, Comet 67P/Churyumov-Gerasimenko, in 2014. It has received gravitational ‘kicks’ from close flybys of Mars (2007) and Earth (2005, 2007 and 2009). Rosetta has also made close flybys of two asteroids.

Now let us put solar events here on earth into our wormhole recipe. The energy of the sun is too great to not be involved in this somehow and in some way.

An equinox is an event in which a planet’s subsolar point passes through its Equator. The equinoxes are the only time when both the Northern and Southern Hemispheres experience roughly equal amounts of daytime and nighttime.

On Earth, there are two equinoxes every year: one around March 21 and another around September 22. Sometimes, the equinoxes are nicknamed the “vernal equinox” (spring equinox) and the “autumnal equinox” (fall equinox), although these have different dates in the Northern and Southern Hemispheres.[2]

The vernal equinox is a time when cracks are known to open in Earth’s magnetic field. Researchers have long known that during weeks around equinoxes fissures form in Earth’s magnetosphere. Solar wind can pour through the gaps to fuel bright displays of Arctic lights.

During these displays, streams of solar wind barely graze Earth’s magnetic field. At these times of year, that’s all it takes. Even a gentle gust of solar wind can breach our planet’s magnetic defenses.

This is called the “Russell-McPherron effect,” named after the researchers who first explained it. The cracks are opened by the solar wind itself.  South-pointing magnetic fields inside the solar wind oppose earth’s north-pointing magnetic field. The two, N vs. S, partially cancel one another, weakening our planet’s magnetic defenses.

This cancellation can happen at any time of year, but it happens with greatest effect around the equinoxes. A 75-year study shows that March is the most geomagnetically active month of the year, followed closely by September-October as direct result of “equinox cracks.”

NASA and European spacecraft have been detecting these cracks for years. Small ones are about the size of California, and many are wider than the entire planet. While the cracks are open, magnetic fields on earth are connected to those on the sun.

Theoretically, it would be possible to pick a magnetic field line on the ground and follow it all the way back to the solar surface. There is no danger to people on earth because our atmosphere protects us, intercepting the rain of particles. The afterglow of this shielding action is called the “aurora borealis.” [3]

We have all seen pictures and video of the Aroura from earth. This is what it can look like from outer space. Looks a lot like a wormhole does it not?

Click the arrow to toggle the video on / off.

Earth’s magnetic field creates a ‘bubble’ around Earth that helps protect our planet from some of the more harmful effects of energetic particles streaming out from the sun in the solar wind. Some of the earliest hints of this interaction go back to the 1850s with the work of Richard Carrington, and in the early 1900s with the work of Kristian Birkeland and Carl Stormer.

That this field might form a type of ‘bubble’ around Earth was hypothesized by Sidney Chapman and Vincent Ferraro in the 1930s. The term ‘magnetosphere’ was applied to magnetic bubble by Thomas Gold in 1959. It wasn’t until the Space Age, when we sent the first probes to other planets, that we found clear evidence of their magnetic fields (though there were hints of a magnetic field for Jupiter in the 1950s, due to observations from radio telescopes).

The Voyager program, two spacecraft launched in 1977, and successors to the Pioneer 10 and 11 missions, completed flybys of the giant outer planets. They became the implementation of the ‘Grand Tour’ of the outer planets originally proposed in the late 1960s. The Voyagers provided some of the first detailed measurements of the strength, extent and diversity of the magnetospheres of the outer planets.

The visualizations below present simplified models of these planetary magnetospheres, designed to illustrate their scale, and basic features of their structure and impacts of the magnetic axes offset from the planetary rotation axes.

For this Earth visualization, note that the north magnetic pole points out of the southern hemisphere. For these visualizations, the magnetic field structure is represented by gold/copper lines. Some additional glyphs are provided to indicate some key directions in the field model.

  • The Yellow arrow points towards the sun. The magnetotail is pointed in the opposite direction.
  • The Cyan arrow represents the magnetic axis, usually tilted relative to the rotation axis. The arrow indicates the NORTH magnetic pole (convention has field lines moving north to south as the north pole of bar magnet (and compass pointer) points to the south magnetic pole).
  • The Blue arrow represents the north rotation axis. It is part of the 3-D axis glyph (red, green, and blue arrows) included to make the planetary rotation more apparent.
  • The semi-transparent grey mesh in the distance represents the boundary of the magnetosphere.

Click the arrow to toggle the video on / off.

Earth’s magnetosphere near the time of the equinox.

Earth’s magnetosphere near the time of the summer solstice

Earth’s magnetosphere near the time of the winter solstice

NASA Scientific Visualization Studio                                    Earth’s Magnetosphere

It certainly appears that the bulk of the ingredients necessary for a wormhole to occur are all around us every day. Putting all of it together in just the right portions seems to be the issue. To find the wormhole, we must look in the right places and at the right times, in the right direction.  Knowing all this certainly strengthens the methodology presented in my books.  It is clearly possible that during equinox events, at certain locations on earth, everything comes together that makes a wormhole open.

[1] SciTechDaily. Physicists Create a Magnetic Wormhole for the First Time. By Universitat Autònoma  de    Barcelona. September 3, 2015

[2] National Geographic. Encyclopedia Entry: Equinox

[3] Spaceweatherarchive.com. “Equinox Cracks” Forming in Earth’s Magnetic Field. Dr. Tony Phillips. March 2018

 

Marie (Madam) Curie

For centuries, women have made significant contributions to science. They’ve discovered life-saving remedies, devised world-altering inventions, and produced far-reaching research. In many cases their invaluable advances are minimized or neglected.

Women have always made significant contributions specifically to the study of astronomy throughout history. Unfortunately, they have not often been recognized for their achievements with the same publicity and reward received by male scientists throughout history.

 At ECG we offer the recognition, respect, and appreciation these women deserve for their important contributions. 

Spotlight on Marie Curie:

Maria Salomea Skłodowska (November 7, 1867 – July 4, 1934)

Marie (Madam) Curie was born in WarsawCongress Kingdom of Poland, a Russian Empire.  She died in Sallanches, France. Curie is most remembered in the scientific community for her work on radioactivity and twice a winner of the Nobel Prize. 

Curie was awarded the 1903 Nobel Prize for Physics, which was the third Nobel awarded since the first in 1901. She was the sole winner of the 1911 Nobel Prize for Chemistry. Curie was the first woman to win a Nobel Prize, and she is the only woman to win the award in two different fields. 

From childhood, she was remarkable for her prodigious memory. At the age of 16, she won a gold medal on completion of her secondary education at the Russian lycée. Because her father, a teacher of mathematics and physics, lost his savings through bad investment. She had to take work as a teacher as a result. At the same time, she took part clandestinely in the nationalist “free university,” reading in Polish to women workers.

 At the age of 18, she took a post as governess, where she suffered an unhappy love affair. From her earnings, she was able to finance her sister Bronisława’s medical studies in Paris. 

She was appointed as lecturer in physics, at the École Normale Supérieure for girls in Sèvres (1900).  There she introduced a method of teaching based on experimental demonstrations. In December 1904, she was appointed chief assistant in the laboratory directed by Pierre Curie, her husband.

Their marriage (July 25, 1895) marked the start of a partnership that was soon to achieve results of world significance. Most notable was the discovery of polonium (so called by Marie in honor of her native land) in 1898. A few months later they discovered radium. 

Following Henri Becquerel’s discovery (1896) of a new phenomenon called “radioactivity”, Curie decided, as a subject for a thesis, to find out if the property discovered in uranium was to be found in other matter. She discovered that this was true for thorium. 

Marie Curie received her Doctor of Science in June 1903. With Pierre, she was awarded the Davy Medal of the Royal Society. Also in 1903, they shared with Becquerel the Nobel Prize for Physics for the discovery of radioactivity.

The death of Pierre Curie in 1906 was a bitter blow to Marie Curie. It was also a decisive turning point in her career. She was to devote all her energy to completing alone the scientific work that they had undertaken. On May 13, 1906, she was appointed to the professorship that had been left vacant on her husband’s death. She was the first woman to teach in the Sorbonne.

In 1908, she became titular professor, and in 1910, her fundamental treatise on radioactivity was published. She was awarded the Nobel Prize in 1911 in Chemistry, for the isolation of pure radium. In 1914, she saw the completion of the building of the laboratories of the Radium Institute (Institute du Radium) at the University of Paris.

Accompanied by her two daughters in 1921, Curie made a triumphant journey to the United States, where President Warren G. Harding presented her with a gram of radium bought as the result of a collection among American women. She gave lectures, especially in Belgium, Brazil, Spain, and Czechoslovakia. She was made a member of the International Commission on Intellectual Co-operation by the Council of the League of Nations.

In addition, she had the satisfaction of seeing the development of the Curie Foundation in Paris. The was also there for the inauguration of her sister Bronisława as director of the Warsaw of the Radium Institute in 1932. 

Throughout World War I, Curie, with the help of her daughter Irène, devoted herself to the development of the use of X-radiography. In 1918, the Radium Institute began to operate in earnest, and it was to become a universal center for nuclear physics and chemistry.

Curie, a member of the Academy of Medicine in 1922, committed her research to the study of the chemistry of radioactive substances and the medical applications of these substances.

Marie Curie, together with Irène Joliot-Curie, wrote the entry on radium for the 13th edition (1926) of the Encyclopedia Britannica.

One of Curie’s outstanding achievements was to have understood the need to accumulate intense radioactive sources.  The stockpile was needed not only to treat illness, but also to maintain an abundant supply for research in nuclear physics.  The resultant stockpile was an unrivaled instrument until the appearance after 1930 of particle accelerators.

The Paris at the Radium Institute ultimately accumulated a stock of 1.5 grams of radium over a period of several years. The stock of radium D and polonium made a decisive contribution to the success of the experiments undertaken in the years around 1930. In particular were of those performed by Irène Curie in conjunction with Frédéric Joliot, her husband. This work prepared the way for the discovery of the neutron by Sir James Chadwick and, above all, for the discovery in 1934 by Irène and Frédéric Joliot-Curie of artificial radioactivity.

A few months after this discovery, Marie Curie died of aplastic anemia caused by the action of radiation. Her contribution to physics had been immense, not only in her own work, the importance of which had been demonstrated by the award to her of two Nobel Prizes, but because of her influence on subsequent generations of nuclear physicists and chemists.

In 1995, Marie Curie’s ashes were enshrined in the Panthéon in Paris. She was the first woman to receive this honor for her own achievements.

 

 

Her office and laboratory in the Curie Pavilion of the Radium Institute are preserved as the Curie Museum.

We are privileged to include her in our ECG Library & Hall of Fame – Women of Science.

 

Sources: Britannica / Wikipedia / Nobel Prize.org

ECG Hall of Fame: Spotlight on Hipparchus – Astronomer

Astronomy and Astrology are recognized in the scientific community as “the first Science” of humanity. At ECG we recognize some of these “Hall of Fame” astronomers of all time and the contributions they have made to our modern understanding of the universe. Please visit our library as we continue to develop our roster of the great ones.

Spotlight on Hipparchus: (c. 190 – 120 BC)

 
  • Fields of study: Astronomy, Mathematics, Geography
  • Accomplishments and legacy: the Founder of Trigonometry, Greatest Astronomer of Antiquity

Hipparchus of Nicaea was a very well-known Greek astronomer. He made great contributions in the fields of mathematics and geography. He is the founder of trigonometry and is considered by many the “greatest astronomer of antiquity.” He has also been called the father of astronomy (as have others).

Hipparchus was known for his astronomical observations in Rhodes where he applied mathematical techniques for accuracy. Through them, he was able to compile the first extensive star catalog.

Hipparchus was the first mathematician known to have produced a trigonometric table. He used these tabulated values to compute the eccentricity of the Moon and Sun’s orbit. By comparing the position of stars with the observations of Timocharis of Alexandria 150 years earlier, Hipparchus discovered the precession of the equinoxes. In addition, he also devised a method to predict solar eclipses.

Only very little of the works of Hipparchus has survived through time. In geography, it is said that he was the first one to have used the geographic coordinate system in determining latitude on Earth from star observations. His star catalog and works in geography, among others, became the basis of other astronomers after him, like Claudius Ptolemy.

Source – The Planets.org