As far as I know, the big damage from Nuclear Weapons planetside is the massive blastwave that can pretty much scour the earth, with radiation and thermal damage bringing up the rear.

But in space there is no atmosphere to create a huge concussive and scouring blast wave, which means a nuclear weapon would have to rely on its all-directional thermal and radiation to do damage… but is that enough to actually be usful as a weapon in space, considering ships in space would be designed to handle radiation and extreme thermals due to the lack of any insulative atmosphere?

I know a lot of this might be supposition based on imaginary future tech and assumptions made about materials science and starship creation, but surely at least some rough guess could be made with regards to a thernonuclear detonation without the focusing effects of an atmosphere?

  • FireRetardant@lemmy.world
    link
    fedilink
    arrow-up
    3
    arrow-down
    1
    ·
    6 months ago

    Chances are there isnt enough air to make a significant difference and any ship large enough to have enough air would have air lock systems as a safety net.

    • R0cket_M00se@lemmy.world
      link
      fedilink
      English
      arrow-up
      16
      ·
      6 months ago

      Right, but the ship itself would allow the shockwave, metal is still matter for vibrations to follow.

      • piecat@lemmy.world
        link
        fedilink
        arrow-up
        1
        ·
        6 months ago

        That would have to be a big ship to feel a shock wave without being consumed by the ball of plasma

        • R0cket_M00se@lemmy.world
          link
          fedilink
          English
          arrow-up
          2
          ·
          6 months ago

          Where would that come from? According to a posted article in this thread thermal energy can’t transfer either unless by direct connection and radiation would be the biggest factor, with increasing size compared to on the surface due to lack of atmosphere “attenuating” the distance it travels.