Former CIA Pilot John Lear Says "There Are Millions Of Aliens Living On The Moon"

A former CIA pilot shocked the public with his statement that the Moon is actually a livable place with over 250 million citizens.

The former CIA pilot, John Lear, has been quite famous among the conspiracy theorists.

"Everything you heard about the Moon is a lie," exclaimed Mr. Lear.

He said he has discovered secret structures on the Moon and furthermore, showed some images that allegedly show proof of these artificial formations.

Amateur astronomers have recently recorded something that looks like a holograph projection of the Moon’s surface.

There are many people that believe that some kind of a science or technology is hiding the structures on the moon. So, this holographic technology might actually be the one that covers them up.

The first visits to the Moon most probably happened thanks to the Tesla’s anti-gravity craft.

I can prove this...

CONTINUE READING
.

.

.

.

.

.

.

.

.

.

.

.

.

.

.

.

.

READ MORE
.

.

.

.

.

.

.

.

.

.

.

.

Tags: science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science, science, astronomy, UFOs, aliens, space, space science, science, Earth, Earth science, science, breaking news, science,

Astronomers estimate that our galaxy has about one exoplanet for every star. Of course, some stars have many planets, such as our Sun, which has eight. And some stars have none. However, if a star lives long enough, planet formation appears to be the rule rather than the exception.

That doesn’t mean astronomers will be able to map all of those billions of stars. The number of exoplanets that have been measured or counted in some way is much smaller.

As of this writing, the total number of confirmed exoplanets stands at 5,108. Astronomers, on the other hand, are surprisingly good at figuring out what they can’t see. They are aware that their telescopes are insufficiently powerful or precise to detect the most elusive planets – those that are very small, very far from their stars, or orbit stars very far from Earth. And conversely, there are regions of space where astronomers are pretty confident they’ve found all the planets within a certain range.

By combining the knowledge of what they can see – the known exoplanets – with the knowledge of what they can’t see – the parts of space currently beyond our ability to investigate – astronomers end up at the approximation of one planet per star.

Astronomers believe they have discovered the first extragalactic exoplanet beyond our own galaxy. The binary system M51-ULS-1, located 28 million light-years away near the heart of the Whirlpool Galaxy (M51), consists of either a neutron star or a black hole tangoing with a more typical companion star.

Astronomers used X-ray data rather than more traditional visual observations to locate the distant planet hidden in this system. "We are trying to open up a whole new arena for finding other worlds by searching for planet candidates at X-ray wavelengths, a strategy that makes it possible to discover them in other galaxies," said study lead Rosanne Di Stefano of the Harvard-Smithsonian Center for Astrophysics in a press release.

The new study,

which was published in Nature Astronomy, looked at three galaxies: M51, M101, and M104. Using the Chandra X-ray Observatory and the European Space Agency’s XMM-Newton, the team targeted more than 200 total star systems within these galaxies. They discovered only one exoplanet in all of those systems.So far, researchers have primarily used two methods to identify the over 4,000 confirmed exoplanets. The radial velocity method determines how much a star wobbles when an orbiting planet gently tugs on its stellar host. Even though stars have far more mass than the planets that orbit them, even a small planet can cause its star to move slightly, leaving an imprint in the star’s light.

In contrast, the transit method takes advantage of a planet passing in front of its star. This temporarily dims the starlight by a noticeable amount. Even though planets are much smaller than stars, researchers can detect these delicate but detectable variations in brightness.

Although both the radial velocity and transit methods are clearly effective, they can only find planets up to about 3,000 light-years from Earth. That is still well within the bounds of our Milky Way galaxy, which spans approximately 100,000 light-years

To find the first extragalactic planet,

scientists decided to look for passing planets within X-ray binaries. A white dwarf, neutron star, or black hole would pull material from a companion star in these systems. When this material collides with the exotic stellar remnant, it becomes superheated and emits X-rays.

Unlike optical light transits, where a relatively small planet only blocks a tiny amount of starlight, the area where X-rays are produced in such binary systems is small enough that even a planet can block a significant portion (if not all) of the X-ray light. This means that X-ray transits can be found at much greater distances than visual transits.

The black hole or neutron star

in the M51-ULS-1 system is closely orbited by a star 20 times the mass of the Sun. This makes the system one of the most visible X-ray binaries in M51. Using Chandra data, researchers discovered that the X-rays typically emitted by the system dropped to zero for 3 hours. The researchers believe that a Saturn-sized exoplanet is orbiting the compact object at a distance of 19.2 astronomical units (AU; where 1 AU is the average distance between Earth and the Sun). That is roughly twice the distance between Saturn and the Sun.

Of course, an exoplanet isn’t the only possibility for why the X-ray signal was disrupted. A cloud of dust passing in front of an X-ray source can also obscure it. The researchers did consider this explanation, too, but they ultimately concluded it was less likely than an exoplanet.

Unfortunately, it will take a long time to confirm the extragalactic detection. Because of its large orbit, the candidate will not pass in front of the source for another 70 years.

Rough past

If M51-ULS-1 is a planet, the Saturn-sized object has a turbulent past.

The presence of a neutron star or black hole indicates that the system once housed not only the current companion star, but also another dying star. This doomed star would have used up all of its fuel before exploding as a supernova, bathing any nearby planets in intense radiation.

And, because the system’s massive current companion star is still alive and well, it’s entirely possible that this extragalactic exoplanet will be forced to survive another destructive supernova in the future.

The James Webb Space Telescope (JWST) has already pushed humanity’s vision deeper into time and space than ever before, providing a breathtaking preview of the deepest and sharpest infrared image of the early Universe to date.

Now, NASA has just unveiled five more stunning full-color images captured by the most ambitious telescopes humanity has ever built.

Feast your eyes on these incredible visions, which are clearer and more detailed than anything we’ve ever seen.

If you aren’t already blown away, consider that this is only five days’ worth of images!! It is the result of decades of hard work by many people all over the world, and it is only the beginning.

The Southern Ring Nebula

What you see here are spectacular death waves from the Southern Ring Nebula – shells of gas shuddered off dying stars.

The Southern Ring Nebula, also known as NGC 3132, is a beautiful, glowing blob in the southern constellation of Vela located approximately 2,500 light-years away.

It has two stars in the center. The fainter one is a white dwarf, which is the collapsed core of a dead star that once had up to eight times the mass of the Sun. It died, blew off its outer layers, and the core collapsed into an ultradense object: up to 1.4 times the mass of the Sun packed into an object the size of Earth. Although it still shines, it is only due to residual heat. It will cool to a dark, dead object over billions of years.

JWST has revealed for the first time that this star is shrouded in dust. The brighter star is further along in its evolution and will eventually explode into its own nebula.

"Webb will allow astronomers to dig into many more specifics about planetary nebulae like this one," explains NASA. "Understanding which molecules are present, and where they lie throughout the shells of gas and dust will help researchers refine their knowledge of these objects."

Read more about the image of the Southern Ring Nebula.

WASP-96b, a hot puffy world so close to its star that its orbit is only 3.5 Earth days, was one of JWST’s targets. It’s whirling around 1,150 light-years away, around a Sun-like star.

WASP-96b has a mass less than half that of Jupiter and a diameter 1.2 times that of Jupiter, making it much puffier than any gas giant in our Solar System – and much hotter, with a temperature of more than 1,000 degrees Fahrenheit (538 degrees Celsius).

What’s fascinating is that JWST has been able to detect evidence of clouds and haze in the exoplanet’s atmosphere, capturing "the distinct signature of water".

JWST was able to reveal the presence of specific gas molecules around the planet by observing tiny decreases in the brightness of specific colors of light over a 6.4-hour period on June 21. This is the most detailed analysis of an exoplanet’s atmosphere that we’ve ever received.

How does it work? When an exoplanet passes between us and its host star, a small, very small amount of the star’s light should pass through the star’s atmosphere, if it has one. Scientists can examine the spectrum of that light to look for brighter or dimmer wavelengths from light absorbed and re-emitted by atmospheric elements. This can help us figure out what those elements are.

What’s interesting is that previous observations suggested WASP-96b had a cloudless atmosphere. So we still have a lot to learn about this strange exoplanet.

The Hubble Space Telescope detected water in an exoplanet’s atmosphere in 2013, but Webb’s detection is faster and far more detailed, and only hints at the potential of what lies ahead for our understanding of alien worlds.

Read more about the WASP-96b observations.

Stephan’s Quintet

Stephan’s Quintet is a group of galaxies locked in a cosmic dance of collisions and the birth of new stars (the red areas in the image below).

The new JWST image of Stephan’s Quintet is enormous, covering one-fifth of the Moon’s diameter (as seen from Earth) and containing over 150 million pixels. It was created using approximately 1,000 image files and helps in understanding how these dramatic galactic interactions shape galaxy evolution.

Read more about the image here.

The Carina Nebula

Last but not least, we have the stunning Carina Nebula as we’ve never seen it before, complete with hundreds of brand new stars. This breathtaking image depicts the edge of a nearby young star-forming region known as NGC 3324.

The incredible detail in the infrared JWST image creates an incredible sense of depth and texture, and there are many mysterious new structures to investigate.The tallest peak in this image, known as the ‘Cosmic Cliffs,’ is a staggering 7 light-years high, with blue ionized gas steamed off it by intense radiation.

The top is where newborn stars erupt, and the stellar wind they generate pushes the orange-y gasses away, which in turn ignites new stars or can snuff them out before they form.

What’s amazing is that we’re all made up of the same star stuff as seen in this image.