Former AREA 51 Engineer Breaks His Silence: "There is an Extraterrestrial Race Working With US"
For a long time, Area 51 has been the focus of different conspiracy theories, especially because it is highly secret and hidden so that only people with official access can reach it. However, recently one of the biggest scandals involving this place came to light, especially because it was an engineer who worked in Area 51 that provided classified information. And although it seems incredible, many experts in the field agree that the information has all the veracity.
What happens in Area 51?
Testimonials that directly involve this place have been constantly revealed by people who had access, as the fact that in this place works with amazing technology to discover all kinds of mysteries in the universe that have to do mainly with aliens . It is something that, obviously, has resulted in endless conspiracy theories.
In addition, it has also been claimed that in this place some experiments have been done that...
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ust over 300 light-years away is a star that’s a lot like a very young version of our Sun, with multiple exoplanets orbiting it. That’s an interesting find in itself. But what makes the system truly dazzling is that it just became the first of its kind to be directly imaged, planets and all.
On the night of 16 February 2020, astronomers using the Very Large Telescope in Chile were able to obtain direct observations of two enormous exoplanets on extremely large orbits around the star named TYC 8998-760-1.This image, captured by the SPHERE instrument on ESO’s Very Large Telescope, shows the star TYC 8998-760-1 accompanied by two giant exoplanets, TYC 8998-760-1b and TYC 8998-760-1c. This is the first time astronomers have directly observed more than one planet orbiting a star similar to the Sun. (ESO/Bohn et al.)
Directly imaging exoplanets is challenging, to say the least. They are very dim compared to their host stars, and very far away from us. Most of the over 4,000 exoplanets confirmed to date have only been detected via indirect means – such as faint, regular dips in the star’s light as the exoplanet passes in front of it, or a slight wobble in the star’s position due to the exoplanet’s gravity.
Because these signals are easier to detect when the planet is very large and very close to the star, the majority of confirmed exoplanets are large and on close orbits. But exoplanets on very close orbits are difficult to image directly, because they tend to be vastly outshone by their host stars; and distantly orbiting planets in older systems are too cool for infrared detection.
To date, only a few tens of exoplanets have been directly imaged, and only two other multi-planet systems – both around stars very different from the Sun.
But last year, using direct imaging, a team of astronomers led by Alexander Bohn of Leiden University in the Netherlands found an unusual planet orbiting TYC 8998-760-1.
It was a gas giant around 14 times the mass of Jupiter, orbiting the star at a distance of around 160 astronomical units. To put that in perspective, Pluto orbits the Sun at an average distance of 39 astronomical units.
So Bohn and his colleagues decided to take a closer look, using the Very Large Telescope’s exoplanet-imaging SPHERE instrument. They took several observations over the last year, and added them to data dating back to 2017.When all the data were put together, they held a surprise. Clear and bright, there was the exoplanet they expected to see, TYC 8998-760-1 b. But, at a much greater distance of 320 astronomical units, the astronomers found another bright dot.
Careful analysis and comparison of images taken at different times revealed this wasn’t a star or glitch, but a second, smaller exoplanet, clocking in at about six times the mass of Jupiter. It’s been named TYC 8998-760-1 c.
Such images aren’t just wonderful achievements of science and technology, they can also help us to better understand planetary systems.
For one thing, TYC 8998-760-1 is young, only 16.7 million years old. Studying the exoplanets that orbit young Sun-like stars can give us valuable insight into the formation of planetary systems like our own.
The orbital distance the team detected is already quite interesting, because one model of planetary system formation posits that giant planets form at a distance before migrating inwards towards their host star.
For another, direct images of exoplanets can help us in the search for habitability. Detailed spectroscopic images – breaking down the spectrum of light reflected off an exoplanet – can reveal the presence of an atmosphere, and even the composition of that atmosphere. Photometry, or studying the exoplanets’ brightness and variability thereof, can reveal information about cloud cover and abundance.
We’re not quite at that stage yet, but future instruments, such as the James Webb Space Telescope, and the European Southern Observatory’s ground based Extremely Large Telescope, ought to be sensitive enough to start making such detections.
And they might even be able to find smaller, closer planets in this system that SPHERE may have missed.
The research has been published in The Astrophysical Journal Letters.A team modeling the behavior of has concluded that the masses of the universe’s densest objects are quantized, similar to how electrons orbiting atoms can only have specific energies. Furthermore, just as particles can exist in multiple places at the same time (a phenomenon known as superposition), the authors of a new paper claim black holes can have two masses, each of which is a probability. Don’t worry if you’re having trouble grasping these concepts; even the authors of a paper admit it wasn’t what they expected.
"We all know e=mc2," Dr Magdalena Zych of the University of Queensland told IFLScience. "If we look at how atoms are formed from elementary particles summing the mass of the nucleons does not give the total mass of the atom. The atom’s mass also includes some binding energy, and that energy is quantized." This means the mass of the atom cannot be any value because there are only certain amounts the binding energy can be.
Because macroscopic objects are made up of atoms, their masses are also limited. "For macroscopic objects like us the difference is so tiny it is irrelevant," Zych said, but that may not be the case for black holes. The impossible masses, in particular, may be quite important during their formation and when they evaporate due to Hawking Radiation.
The team arrived at their conclusion by considering the behavior of a particle outside of a black hole and how it would interact with the black hole’s gravitational force without breaking any known laws. However, it is a long way to the nearest black hole to actually conduct a test.
The fact that certain black hole masses may be disallowed may be something non-physicists don’t find too hard to swallow, but the other aspect to this work is something else. "Imagine you’re both broad and tall, as well as short and skinny at the same time – it’s a situation which is intuitively confusing since we’re anchored in the world of traditional physics," said first author PhD student Joshua Foo in a statement. Yet if the team is right, it’s true for black holes, just as Schrödinger’s cat can be simultaneously alive and dead.
"The universe is revealing to us that it’s always more strange, mysterious and fascinating than most of us could have ever imagined," Zych said.
What the team doesn’t know yet, according to Zych, is whether superpositions involve masses that are so similar to each other that they make no difference outside of idealized conditions, or if large differences are possible.
Zych acknowledged the work is just mathematical modeling at this stage and will be hard to test. "The next step is to look into the implications for black holes we are studying," Zych said, whether those be relatively nearby, or the supermassive black holes at the heart of other galaxies.
If the research holds up to scrutiny, it could affect the search for quantum gravity, which aims to bring together the two great theories of the twentieth century, General Relativity and Quantum Mechanics. "If so, any model of quantum gravity would have a very tight restriction," Zych told, "Particularly in the final stages of evaporation. It’s one of the most mind-bending projects."
The findings were published in Physical Review Letters.Currently, 2022 AP7 crosses Earth’s orbit while our planet is on the opposite side of , but scientists believe that over thousands of years, the asteroid and Earth will gradually begin to cross the same point closer together, increasing the chances of a catastrophic collision. The asteroid, discovered alongside two other near-Earth asteroids at Chile’s Cerro Tololo Inter-American Observatory, was described in a study published in The Astronomical Journal on September 29.
"So far we have found two large near-Earth asteroids [NEAs] that are about 1 km [0.6 mile] across, a size that we call planet killers," lead study author Scott Sheppard, an astronomer at the Carnegie Institution for Science in Washington, D.C., said in a statement. "Planet killer" asteroids are space rocks that are big enough to cause a global mass extinction event if they were to smash into Earth.
The astronomers used the Cerro Tololo Victor M. Blanco 4-meter Telescope’s Dark Energy Camera to search for asteroids in the inner solar system. Because the sun’s glare makes observations impossible for most of the day, the researchers only had two 10-minute windows of twilight each night to make their observations.