As the 1st post, I would like to ask about the concept of unscoopable stars, I figure the gasses are not compatible with the fuel requirements, aren't stars hydrogen/helium based?
It depends on the star's spectral class. The stars in the scoopable classes - O B A F G K M - are all abundant in hydrogen, the non-scoopable classes aren't. That's either because they've never undergone hydrogen fusion, or because they have expended all their hydrogen.
Going through the list of non-scoopable classes, we have:
Neutron Stars, White Dwarfs, Black Holes - these are stellar remnants; the remains of stellar cores that stopped fusing hydrogen millions of years before they exploded in supernovae (for NS and BH) or shed their outer layers over time (for WD). There's no hydrogen to be found here anymore as it all fused to much heavier elements like iron and so on.
Class Y, T and L Brown Dwarfs - these are sub-stellar objects that are basically gas giant planets that didn't have enough mass to fuse hydrogen and become stars. Y class dwarfs are so small and cold they're really difficult to distinguish from gas giants - there are gas giants larger and hotter than some Y class dwarfs. Generally brown dwarfs can go to to around 70x the mass of Jupiter. Around 70-80 Jupiter masses is when hydrogen fusion is likely to kick in. There's gaseous hydrogen here, but no plasma from fusion, so no fuel.
T-Tauri and Herbig Ae/Be - These are proto-stars, at less than 10 million years old, they're too young to have started fusing hydrogen, but they have the mass for it. T-Tauri stars will become main sequence stars of spectral classes M, G, K, or F. Herbig Ae/Be stars will join the main sequence as A or B class stars and will have a much shorter life.
Carbon Stars - These are typically Red Giant or Supergiant stars that have much more carbon than oxygen in their atmospheres; they're exceedingly rare, and they are reaching the end of their lives. The abundance of carbon is due to helium fusion which dredges all the heavier elements to the surface. This is because these stars alternate between burning hydrogen and helium for long periods (millions of years). You can't scoop a carbon star because it's not currently burning hydrogen.
Wolf-Rayet Stars - These are massive stars that have depleted their hydrogen supply and have more carbon, oxygen, nitrogen, helium and silicon. Most of them will be primarily Nitrogen or Carbon/Oxygen. Very interesting and rare purple glowing stars, but no hydrogen for fuel here.
S-Type stars - These are a type of cool class M carbon star with equal amounts of carbon and oxygen in their atmospheres and an abundance of zirconium oxide. Again, no hydrogen to scoop here.
Hope that helps
