Yes that animation is very good aid for one who does not know all that already. My only fauting of it is it did not explain the * was used to indicate the atom or molecule it was attached to was in and excited state. If it is the nucleus that is in an excited state, typically that is indicated by an m following the atomic symbol. For example the meta-stable isotope of T99, which is used to make whole body scan for cancer spread into the bones is written T99m.... That You Tube on Ozone production if watched will tell you the answer we were looking for. There was momentarily a high energy ozone that was unstable. It either broke up or collided with another atom and transferred its excess energy. So the energy package was transferred by contact with another atom.
Of course. I mentioned as qualifying notes, that the energy radiation could carry away might be removed instead by a collision. In fact that is the ONLY way radiation can heat a gas. I.e. the excitation energy is first shaired by the two colliding atoms and they with many more collision, with others, so that the average RANDOM kinetic energy is very slghtly increased - i.e. the gas is warmed to a higher temperature.... Had you ever heard of this {non-radiative de-excitation of an excited state} before?
If every gas atom (or molecule) that is excited by a photon is only in the excited state (typically for less than a ms) before it radiates that energy again, etc. then there is no heating of the gas.
No in the top of the atmosphere were O2* or O3 or O3* is formed by UV it typically will return to the ground state (O2, or O3) in tiny fracion of a second by collison or radiation. Note the energy transfered by collsion has a random velocity (Is thermal) and the re-radiated photon has equal probability to be traveling in any direction - no memory of what was the direction of travel of the photon that was absorbed to make the excited state. The only imbalance in absorption torques is the one I mentioned earlier. There are very slightly more UV photons that can ionize on the limb moving towards the sun as some are "blue shifted" to have just barely the ionization potential energy.... Reactions of this type could be unbalanced on either side of the planet Venus so on one side the energy remains in the form of broken bond energy (it takes energy to break bonds) and on the other kinetic energy (when the ozone remains stable after transferring excess kinetic energy). The energy side driving the wind (for the momentum of the photon is not lost).
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