Helio in post #33 says "Comets that have a close perihelion will disintegrate more and more with each swing near the Sun. But a long period comet with a perihelion outside that of, say, Pluto — very close to the Sun given an aphelion if at least 10,000 AU — will hold its volatiles and survive for billions of years, IMO."
Applying the Galileo standard of direct observation like the Galilean moons, which comet(s) is documented showing what you just said? Example, Halley's comet? This does not fit. What about this comet, NEOWISE (C/2020 F3)? I observed that back in July 2020 with my telescope. There was also C/2020 M3 Atlas that I viewed with my telescope back in November 2020.
Do you have a specific comet(s) here or is this just a long age model interpretation without objective observations (of real comets) to support the statement? The comet example used in post #33 appears to assume it originated in the Oort cloud and returns to the Oort cloud perhaps. I need to see a real comet example and how many observations were made of the comet(s) like observations of the Galilean moons.
Comet NEOWISE is a good example,
https://en.wikipedia.org/wiki/Comet_NEOWISE, reports 376 observations made but an orbital period perhaps 4400 to 6700 years. There is no way to show the comet completed > 600,000 perihelion passages in the past to match with the radiometric ages of meteorites. Even if NEOWISE completes perihelion passage every 11,000 years, still > 400,000 revolutions in the past required.
I used Jean Meeus algorithms and calculated an orbital period for a model comet with a = 5,000 au, e=0.999, mass ~ 6 x 10^17 g. Perihelion ~ 5.0 au, aphelion ~ 9995 au, P ~ 354,000 years so in 4.5 billion years, ~ 12700 revolutions around the Sun. Demonstrating that a comet like this (if documented by observations like NEOWISE) completed many thousands of past revolutions around the Sun is not observable but an extrapolation.