When to Use the Proxima Centauri System 3D Explorer - Best Sessions and Limits
Open Proxima Centauri System 3D Explorer when you want to see exactly how close Proxima b, d, and c orbit the Sun's nearest star and why a flare-prone red dwarf complicates the "closest star has a habitable planet" headline - not to model atmosphere retention or a flare's actual radiation dose.
A closest-star session
A session starts by watching the two close-in planets, b and d, and toggling the habitable-zone band to see that b falls inside it while d, orbiting even closer, does not - then triggers a flare to see the radiation-complication story reach every planet at once, and reads the facts panel for the exact distances, periods, and masses.
Sessions this explorer does not fit
Sessions this page does not fit are studying a distant 7-planet resonant-chain system - use the TRAPPIST-1 3D Explorer for that - or modeling actual atmosphere-retention odds under stellar radiation, which no visualization on this site attempts. Walk the controls in the step-by-step guide.
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