I assumed so, but for me it just wasn't that interesting since I couldn't play around with it much. Anyway, I tried to parse my Journal files and looked at each and every Neutron star I've visited (285 in total, ugh), also those in orbit around black holes. I simply couldn't find it anymore. The closest I've discovered appears to be in [
this system]. But with a semi-major axis of 49.1765Ls and an eccentricity of 0.080786, this world simply can't qualify at all. It's just too far away, and meets its periapsis at 45.2Ls, so that's a rather circular orbit as well. Plus it's a gas giant, not the terrestrial world I seem to remember, and that one was also too recent.
Not sure if I've been dreaming or whatever... To test my parsing, I looked for a class IV gas giant on a very eccentric orbit around a class M star I've found 1 or 2 weeks ago, and it appears I [
found that one] just fine. Comes as close as 3.6Ls to its star.
So I thought, maybe I'd mistaken that Neutron star for a white dwarf? Quite unlikely, but hey... Even after inspecting all white dwarfs I've discovered however, I could only come up with [
this] - disappointing.
So it appears I have to retract the statement about that close orbiter. I simply can't prove it. Since I'm not usually prone to sudden hallucinations (
) I wonder whether I could've somehow misinterpreted something. But I wouldn't know how.