No LMSCorvetteGT you have not answered anything and I have not ignored anything.
But like I said I am not an expert but I am not a dummy either, studied engineering from 99-2006. I know the big picture about our world but when something like this is making its way on the internets you cant ignore it, to new and interesting
That is why I want your thoughts about, I dont ask actually, rather I want you to think for yourself to see if it sound simple and logically. If I would really need an answerer then I would just open up my books
Just think for a moment, there is a vacuum/emptiness around you and you blow with your mouth. Would it be enough for you to change direction or not? How I am thinking now is that the air you are blowing out is just released as it does not push against you or a another object but away from you. You are just realising air into the emptiness. Of course I am questioning "basic science" that is the point with stuff like this. After all it is a conspiracy thingy. Like I said If I wanted to not think I would just read on in my books but this is more like, what if it is like this up there.
And then we have Iss or anything else up there, how does it not get overheated not get overheated as the particles in the iss will transfer heat to each other but cant dissipate the heat because of the vacuum. Just like a thermos, you said it used radiation before to cool down.
What happens on earth is totally different thing, the earth is massive full of particles and have atmosphere to reflect the radiations back to the ground.
below is just a little link from wikipedia about temps in the thermosphere and why it is not that warm but a big object will probably heat up over there and the cooling in my mind should not be enough to dissipate the heat away from the iss.
The
thermosphere is the layer of the
Earth's atmosphere directly above the
mesosphere and directly below the
exosphere. Within this layer of the atmosphere,
ultraviolet radiation causes
photoionization/photodissociation of molecules, creating ions in the
ionosphere. Taking its name from the
Greek θερμός (pronounced
thermos) meaning heat, the thermosphere begins about 85 kilometres (53 mi) above the Earth.
[1] At these high altitudes, the residual atmospheric gases sort into strata according to
molecular mass (see
turbosphere). Thermospheric
temperatures increase with altitude due to absorption of highly energetic
solar radiation. Temperatures are highly dependent on solar activity, and can rise to 2,000 °C (3,630 °F). Radiation causes the atmosphere particles in this layer to become electrically charged (see
ionosphere), enabling
radio waves to be refracted and thus be received beyond the horizon. In the exosphere, beginning at 500 to 1,000 kilometres (310 to 620 mi) above the Earth's surface, the atmosphere turns into
space.
The highly diluted gas in this layer can reach 2,500 °C (4,530 °F) during the day. Even though the temperature is so high, one would not feel warm in the thermosphere, because it is so near vacuum that there is not enough contact with the few atoms of gas to transfer much heat. A normal
thermometer might be significantly below 0 °C (32 °F), at least at night, because the energy lost by thermal radiation would exceed the energy acquired from the atmospheric gas by direct contact. In the
anacoustic zone above 160 kilometres (99 mi), the density is so low that molecular interactions are too infrequent to permit the transmission of sound.
The dynamics of the thermosphere are dominated by
atmospheric tides, which are driven by the very significant
diurnal heating. Atmospheric waves dissipate above this level because of collisions between the neutral gas and the ionospheric plasma.
The
International Space Station orbits the Earth within the middle of the thermosphere, between 330 and 435 kilometres (205 and 270 mi) (decaying by 2 km/month and raised by periodic reboosts), whereas the
Gravity Field and Steady-State Ocean Circulation Explorer satellite at 260 kilometres (160 mi) utilized
winglets[2] and an innovative
ion engine to maintain a stable orientation and orbit.
[3]