Matthew M. Radmanesh
DOI: 10.37421/2329-6542.2023.11.248
Rhawn Gabriel Joseph* and Rudolph Schild
For thousands of years there have been reports of extra-terrestrial beings and “sky boats” that have visited Earth as recounted in ancient texts from India, Egypt and Greece. During WWII five UFOs appeared above Los Angeles and were impervious to attack and pilots from “allied” and “enemy” countries were repeatedly harassed by extra-terrestrial craft referred to as “Foo Fighters.” In 2023 the U.S. Congress heard testimony that military pilots have repeatedly encountered UFOs and UAPs and those government agencies have obtained the wreckage of and bodies from extra-terrestrial spacecraft. In this report we provide a sample of official NASA Mars photographs of what appears to be the wreckage and debris from extra-terrestrial spacecraft, partially buried bones, the body of a “humanoid” stretched out on a “cushion;” the head of a “humanoid” possibly wearing a metal device on the front of its “face” and adjacent to a cratered debris field, two “humanoid” skulls including one that is atop what may be a raised elongated burial mound, UAPs/UFOs photographed in the skies of Mars and a silver-saucer shaped structure upon the ground. We hypothesize that government agencies refuse to acknowledge any evidence for extra-terrestrial life, be it UAPs or fungi on Mars, because they fear that religious and government authority will be challenged and undermined.
Bamberg Carmen*
Black hole mergers have become a cornerstone of modern astrophysics, revealing profound insights into the nature of gravity, spacetime, and the fundamental processes governing the universe. Observations from the Laser Interferometer Gravitational-Wave Observatory and the Virgo collaboration have revolutionized our understanding of these cosmic events, providing direct evidence of gravitational waves and opening a new window into the cosmos. The groundbreaking detection of gravitational waves in by LIGO marked a pivotal moment in science. For the first time, ripples in spacetime caused by the collision of two massive black holes were observed, confirming a key prediction of Albert Einstein’s general theory of relativity. This event, designated GW150914, occurred approximately 1.3 billion light-years away and involved the merger of two black holes with masses about 29 and 36 times that of the Sun. The energy released in the form of gravitational waves during this cataclysmic event was equivalent to three solar masses, briefly outshining the entire visible universe in gravitational wave luminosity.
Carsten Blanco*
The Cosmic Microwave Background (CMB) is the afterglow of the Big Bang, a faint cosmic radiation filling the universe and providing a snapshot of the cosmos as it was about 380,000 years after its birth. This relic radiation is a crucial tool for cosmologists, offering insights into the early universe's conditions, composition, and evolution. Recent data from various space missions and ground-based observatories have significantly advanced our understanding of the CMB, leading to profound implications for our knowledge of the early universe. One of the most significant advancements in CMB research came from the Planck satellite, launched by the European Space Agency. Planck provided the most detailed map of the CMB to date, capturing tiny temperature fluctuations across the sky. These fluctuations, known as anisotropies, reflect the density variations in the early universe that eventually led to the formation of galaxies and large-scale structures. The high-resolution data from Planck has allowed scientists to refine their measurements of key cosmological parameters, such as the universe's age, composition, and rate of expansion.
Kenneth King*
The James Webb Space Telescope (JWST), launched, has significantly advanced our understanding of exoplanetary atmospheres. As a successor to the Hubble Space Telescope, JWST has brought unparalleled capabilities for observing the universe, particularly in the infrared spectrum. This capability is crucial for studying exoplanets, as it allows astronomers to peer into the atmospheres of distant worlds and analyze their composition, structure, and potential habitability. The latest findings from JWST have provided remarkable insights into the nature of these alien atmospheres, revealing the diversity and complexity of planets beyond our solar system. One of the primary methods JWST uses to study exoplanetary atmospheres is transit spectroscopy. This technique involves observing a planet as it passes in front of its host star, allowing the starlight to filter through the planet's atmosphere. By analyzing the resulting spectrum, astronomers can identify the chemical constituents of the atmosphere. JWST's infrared sensitivity is particularly well-suited for detecting key molecules such as water vapor, carbon dioxide, methane, and other potential biomarkers.
Pounds Andrew*
Galactic collisions or interactions between galaxies, offer profound insights into the dynamics, evolution, and growth of galaxies. These cosmic events, though often violent and chaotic, play a crucial role in shaping the structure and content of the universe. By studying interacting galaxies, astronomers gain valuable knowledge about the processes that drive galaxy formation and evolution, as well as the fundamental forces at play in the cosmos. When galaxies collide, they do not simply smash into each other like solid objects; instead, they pass through each other, causing complex gravitational interactions. These interactions lead to significant changes in the structure and dynamics of the galaxies involved. The gravitational forces exerted during a collision can trigger a cascade of events, including the compression of gas, the formation of new stars, and the redistribution of stellar and gas components. Observations of these processes provide key insights into the life cycles of galaxies and the mechanisms behind their growth and transformation.
Lisa Meredith*
Brant Rhys*
Stevenson Becca*
John Mills*
Catherine Waring*
Fitzsimons Abigail*
DOI: DOI: 10.37421/ 2329-6542.2022.10.220
According to Stephen Hawking, black hole create and emit particles thereby evaporating and losing their mass slowly with time. As it loses its mass, the wavelength of the emitted particles decreases and the energy of the black hole radiation increases. The wavelength of Hawking radiation is related to the curvature of space-time continuum near the event horizon by the equation
where λHR is the wavelength of the Hawking radiation. Also, by subtracting this equation from the net energy content of the black hole before emission, we can get the energy of the black hole after emission. Since black holes emit radiation that has immense pressure when it’s mass tends to zero then due to radiation pressure exerted on a body will prevent it from crossing the event horizon which is a property of white holes. In this way a black hole may behave as a white hole.
Yanbikov Vildan Shavkyatovich*
Applying the wave model of gravity, the density is calculated the physical vacuum. An unusually high virtual density is obtained states of physical vacuum. Following the wave model of gravity, protons A and B re-emit the gravitational energy of the cosmos into the surrounding space. Is represented (for convenience of calculations) a physical vacuum
consisting of virtual protons, so that in at any given time, there are n protons in the elementary volume of the dV vacuum
K M Sanid
Time is still an unknown fact to human, but we use time to define every motion and to describe objects. The time is connected with gravity, as the gravity increase the time starts to dilate in space and also we know that as the speed of an object increase the time starts to move slower. The light has the maximum speed in the space.
Astrophysics & Aerospace Technology received 114 citations as per Google Scholar report
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