Buzz Aldrin Reveals: On the Moon We Were Ordered by Aliens To Move Away!
Here are the statements by the former astronauts:
Professor: What really happened out of Apollo 11?
Buzz Aldrin: An amazing thing, even though we have always known of this possibility. The fact is that they (aliens) have ordered us to turn away! .
Professor: What do you mean "warned to move away"?
Buzz Aldrin: I can not go into details, there are structures on the Moon, and not ours. I can only say that their ships were far superior to ours both in size and technology. Wow if you were big! … And menacing!
Professor: But NASA also sent to the moon missions after Apollo 11 ….
Buzz Aldrin: Naturally, NASA had already announced at that time, and could not risk panic on Earth.
According to the American ufologist Vladimir Azhazha, "Neil Buzz Aldrin said to Mission Control that two large unknown objects were watching him and...
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Some 540 million years ago, diverse life forms suddenly began to emerge from the muddy ocean floors of planet Earth. This period is known as the Cambrian Explosion, and these aquatic critters are our ancient ancestors.
All complex life on Earth evolved from these underwater creatures. Scientists believe all it took was an ever-so-slight increase in ocean oxygen levels above a certain threshold.
We may now be in the midst of a Cambrian Explosion for artificial intelligence (AI). In the past few years, a burst of incredibly capable AI programs like Midjourney, DALL-E 2 and ChatGPT have showcased the rapid progress we’ve made in machine learning.
AI is now used in virtually all areas of science to help researchers with routine classification tasks. It’s also helping our team of radio astronomers broaden the search for extraterrestrial life, and results so far have been promising.
Discovering alien signals with AI
As scientists searching for evidence of intelligent life beyond Earth, we have built an AI system that beats classical algorithms in signal detection tasks. Our AI was trained to search through data from radio telescopes for signals that couldn’t be generated by natural astrophysical processes.
When we fed our AI a previously studied dataset, it discovered eight signals of interest the classic algorithm missed. To be clear, these signals are probably not from extraterrestrial intelligence, and are more likely rare cases of radio interference.
Nonetheless, our findings – published today in Nature Astronomy – highlight hoBlack holes are among the most fascinating and mysterious objects in the universe. They are formed from the remnants of massive stars that have exhausted all their fuel and collapsed under their own gravity. The process of how a black hole is formed is complex and fascinating, and it involves some of the most fundamental principles of physics.
Gravity is the key to understanding how a black hole is formed. Gravity is the force that attracts objects with mass towards each other. The more massive an object is, the stronger its gravity. In the case of a black hole, the gravitational force is so strong that it becomes impossible for anything, including light, to escape its pull.
To understand how a black hole is formed,
we must first understand the life cycle of a star. A star is born when a cloud of gas and dust collapses under its own gravity. As the cloud collapses, it heats up and starts to glow. This process is known as nuclear fusion, and it is the process that powers the star.
Stars come in a range of sizes, from small ones like our sun to massive ones that can be dozens or even hundreds of times more massive. The more massive a star is, the faster it burns through its fuel. When a star like our sun exhausts all its fuel, it will become a white dwarf, which is a small, dense star that slowly cools over billions of years.
However, for more massive stars, the end is much more dramatic.
When a massive star exhausts all its fuel, it will undergo a catastrophic collapse, known as a supernova. During a supernova, the star’s core collapses under its own gravity, and the outer layers of the star are ejected into space.The core of the star is compressed to a point where its gravity becomes so strong that nothing can escape it. This is the birth of a black hole. The point of no return is known as the event horizon, and it is the point beyond which nothing can escape the black hole’s gravitational pull.
The process of how a black hole is formed
is governed by some of the most fundamental principles of physics. In particular, it is governed by Einstein’s theory of general relativity, which describes how gravity works in the universe. According to general relativity, massive objects warp the fabric of space-time around them, and this warping causes other objects to move towards them.
The formation of a black hole is a fascinating process that is governed by the laws of physics. It is a process that occurs at the end of the life cycle of a massive star, and it involves the collapse of the star’s core under its own gravity. The result is a singularity, a point of infinite density and gravity, surrounded by an event horizon, which marks the boundary beyond which nothing can escape. Black holes are some of the most mysterious and fascinating objects in the universe, and they continue to inspire scientists and astronomers to study them further.The closest star from Sun is located just over 4 light-years away in the Alpha Centauri star system. It is a binary star system, meaning that it is comprised of two stars that orbit around a common center of mass. The two stars are known as Alpha Centauri A and Alpha Centauri B, with a third star, Proxima Centauri, located even closer to Earth.
Alpha Centauri A and B are similar in size and brightness to our own sun. Alpha Centauri A is slightly larger and brighter than our sun, while Alpha Centauri B is slightly smaller and cooler. Both stars are located in the constellation Centaurus, which can be seen in the southern hemisphere.
Proxima Centauri, on the other hand, is a much smaller and cooler star known as a red dwarf. It is located just over 4.2 light-years away from Earth, making it the closest known star to our solar system. Despite its proximity, Proxima Centauri is much too faint to be seen with the naked eye and can only be detected with telescopes.
The discovery of the Alpha Centauri star system dates back to the early 19th century, when astronomers began using telescopes to observe the night sky in more detail. In 1832, Scottish astronomer Thomas Henderson measured the parallax of Alpha Centauri, which allowed him to calculate its distance from Earth. This discovery marked the first time that the distance to a star other than the sun had been accurately measured.
The Alpha Centauri system has been the subject of much scientific study and speculation over the years. In 2016, a team of astronomers discovered an Earth-sized planet orbiting Proxima Centauri, raising the possibility that there could be other habitable planets in the system. This discovery has sparked renewed interest in exploring the Alpha Centauri system in search of extraterrestrial life.
In recent years, there have been several initiatives to send spacecraft to the Alpha Centauri system, including the Breakthrough Starshot project, which aims to send a fleet of tiny spacecraft to the system using laser propulsion. While such missions are still in the planning stages, they represent an exciting possibility for exploring the closest star system to our own.
In conclusion, the closest star from Earth is located in the Alpha Centauri system, comprised of Alpha Centauri A and B, and the smaller red dwarf, Proxima Centauri. The discovery of this system has played a key role in our understanding of the universe, and ongoing efforts to explore it hold the promise of further scientific breakthroughs in the years to come.Looking up at the moon in the night sky, you would never imagine that it is slowly moving away from Earth. But we know otherwise. In 1969, NASA’s Apollo missions installed reflective panels on the moon. These have shown that the moon is currently moving 3.8 cm away from the Earth every year.
If we take the moon’s current rate of recession and project it back in time, we end up with a collision between the Earth and moon around 1.5 billion years ago. However, the moon was formed around 4.5 billion years ago, meaning that the current recession rate is a poor guide for the past.
Along with our fellow researchers from Utrecht University and the University of Geneva, we have been using a combination of techniques to try and gain information on our solar system’s distant past.
We recently discovered the perfect place to uncover the long-term history of our receding moon. And it’s not from studying the moon itself, but from reading signals in ancient layers of rock on Earth.
Reading between the layers
In the beautiful Karijini National Park in western Australia, some gorges cut through 2.5 billion year old, rhythmically layered sediments. These sediments are banded iron formations, comprising distinctive layers of iron and silica-rich minerals once widely deposited on the ocean floor and now found on the oldest parts of the Earth’s crust.
Cliff exposures at Joffre Falls show how layers of reddish-brown iron formation just under a metre thick are alternated, at regular intervals, by darker, thinner horizons.The darker intervals are composed of a softer type of rock which is more susceptible to erosion. A closer look at the outcrops reveals the presence of an additionally regular, smaller-scale variation. Rock surfaces, which have been polished by seasonal river water running through the gorge, uncover a pattern of alternating white, reddish and blueish-grey layers.
In 1972, Australian geologist A.F. Trendall raised the question about the origin of the different scales of cyclical, recurrent patterns visible in these ancient rock layers. He suggested that the patterns might be related to past variations in climate induced by the so-called "Milankovitch cycles."
Cyclical climate changes
The Milankovitch cycles describe how small, periodic changes in the shape of the Earth’s orbit and the orientation of its axis influence the distribution of sunlight received by Earth over spans of years.
Right now, the dominant Milankovitch cycles change every 400,000 years, 100,000 years, 41,000 years and 21,000 years. These variations exert a strong control on our climate over long time periods.
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