Some comments:
Sounds really good on first viewing. a few questions.
1) when you have a secondary star system say 300,000 ls + away from the main star, how easy will it be to detect it?, not moaning at all about this, you can argue that there's real skill involved now in find those!
WC: I'd expand on that question and ask if/how we can discern bodies orbiting such secondary stars - will we have to get closer, or can they also be identified from the main star?
2) how will you know that you've found everything in a system? maybe a gravitational mass counter like indicator
WC: This one is implicitely answered - notice the 38% and 51% "system bodies mapped" statistic in the bottom left of the screenshots in post #1. Though one may ask for a distiction between bodies identified (=ADS scan) and mapped (=DSS scan).
3) what does the honk now give you?, if you haven't actually detected anything yet, as need to find them manually withe scanner, what are you actually selling?
WC: There was a "limited" response to this question that you still get some value to sell, but not further detailed. But it was also said that you get the main star scanned (today ~3kcr for your regular star). In the bubble you also get space stations and outposts, as well as USSs, but those have no value in selling system data.
4) hopefully it's relatively easy to synthesise the probes and they can be made from planetary materials only (no data or components please, they're pretty hard to find thousands of light seconds away from the bubble!)
as there's now 90 odd pages maybe a FAQ might be required here!
WC: Qohen Leth already collected the FD responses from last night in one post on page 75.
Keith
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