God’s final argument. Aliens are just that.
Introduction:
There are some things astronomers prefer not to publicize. Not because they hide them – they just don’t think about them.
That’s what happens when you look at photos of supernova explosions, not through the lens of textbooks, but with your own eyes…
Chapter 1: My discovery. Well, like mine, allowed to me.
Zabolotsky’s Question and Answer, or Zabolotsky’s Question. (Fermi analogy)
If globular star clusters, according to astronomers, are one of the most uncomfortable places for life, much less intelligent life and here’s the thing, there is no interstellar gas in globular star clusters and astronomers admit they don’t know why this is so.
Now we look at the place where we live and we find out that, according to the same astronomers, the neighborhood of the solar system is a pretty dusty place, lots of interstellar gas. Well, you can look at the Milky Way, the naked eye can see giant dense areas of cold clouds of gas, they are, according to scientists
in the disk of our galaxy about 5 thousand to 1 million solar masses.
So, globular star clusters no life, no dust (gas), look out the window, there is life, and intelligent, look in the sky dust (gas) is very much. Conclusion, dust, interstellar gas is a trace, a by-product, a marker accompanying intelligent life. The cosmos is not silent, it is shouting, often in matte about intelligent life.
Once again, briefly.
Globular star clusters no life, no dust (gas), the neighborhood of the solar system, for example, a volume of 1000 light years, there is intelligent life, there is dust (gas).
We can see with the naked eye traces of intelligent life in the Milky Way (our galaxy) with telescopes in the Magellanic clouds, in the disks of other galaxies, and in some galaxies visible from the edge
interstellar gas is expanding downward upward in the photo (or rather both sides of the galaxy disk edge)
so the disk of the galaxy is said to be teeming with intelligent life.
It should be noted that there is no dust even in some dwarf galaxies, for example, the satellite of our galaxy dwarf galaxy Leo-I, or Leo A is almost devoid of interstellar medium, the stellar body is visible, but there is no interstellar gas. And at the same time we see dwarf galaxies with masses of interstellar gas. And astronomers admit that they don’t know why this is so. And the explanation is that intelligent life hasn’t had time to get to a dwarf galaxy with no interstellar gas. The distances are great.
But that’s not all. There are other stars in the halo of our galaxy.
These are old, metal-deficient stars that move in elongated orbits around the center of the galaxy, often crossing the disk. Their properties are similar to those of globular cluster stars. Visible halo stars in the Milky Way range from 100 million to 1 billion, but the exact number is unknown because of the difficulty of observation. Indirect methods, including statistics and modeling, are used to study them.
The lifetime of the supernova explosion remnant in the Milky Way halo (outside the disk plane) depends on the medium, but because of the extremely low gas density, it is much longer than in the disk. Total “lifetime” of the supernova explosion remnant in the halo:
Minimum: ~1 million years (if there are weak external influences).
Maximum: 10—50 million years (in a perfectly rarefied environment).
For comparison: in the disk of a supernova explosion remnant disappears in 50,000—300,000 years.
Visible halo stars in the Milky Way – from 100 million to 1 billion and no, not one supernova in the period from 1 to 50 million years, when the supernova remnant in the halo of the Milky Way will be visible to us.
If you think there’s one, at least there’s a confirmed one. You’re wrong.
To date, there are no confirmed supernova remnants (SNR) in the Milky Way halo, despite hundreds of millions of stars and theoretical lifetimes of remnants up to 50 million years.
Then 100 million to 1 billion stars, 1 to 50 million years and equal to zero supernova explosion in the Milky Way halo (outside the disk plane). At a minimum 100 million stars 1 million years and zero, ZERO Carl.
If we take for the sake of comparison the neighborhood of the solar system in a sphere with a diameter of 6500 light years (up to the Crab Nebula) and for 1000 years the explosion of 1 star in the Crab Nebula, where there are approximately 500—800 million stars in a sphere with a diameter of 6500 light years. Then it is possible to calculate in how many times for 1 million years supernovae have exploded more in the neighborhood of solar system in sphere in diameter of 6500 light years (up to Crab Nebula) than supernovae have exploded in halo
of the Milky Way (outside the disk plane).
Comparison of supernova explosion frequencies.
In the neighborhood of the Solar System:
1000 supernovae in 1 million years (for 650 million stars).
In the halo:
0 supernovae in 1 million years (even for 100 million stars).
