MHD-Int Nearby Systems Trio — Wolf 1061, Tau Ceti and GJ 667 C
Solaris Core — MHD-INT
Where do the numbers come from?
NASA Exoplanet Archive (queried October 2026), Astudillo-Defru et al. 2017, Wright et al. 2016, Feng et al. 2017, Bonfils et al. 2013, Anglada-Escudé et al. 2013, Chen & Kipping 2017, Kopparapu et al. 2014. Full list in CREDITS.md.
Which Blender version do I need?
Blender 4.2 LTS or newer. Older versions (3.x) are not supported.
Does it work with EEVEE?
It has only been tested with Cycles. Materials and lighting were tuned for Cycles.
Can I use the renders commercially?
Yes. Images, animations and scenes you create are yours, including for commercial projects. The script itself is GPL-3.0-or-later.
Do I need an add-on?
No. Everything is procedural and generated by the included script; no add-on and no external textures are required.
Why three .blend files?
One per system, so each opens already built and ready to render. All three share the same engine and camera keys.
Are the planet sizes measured?
No. None of these planets transits. Radii are estimated from minimum mass (Chen & Kipping 2017) and labelled as estimates.
Why is Tau Ceti e missing?
It is considered a false positive, so it is not drawn.
Why are some planets labelled "controversial"?
Because the NASA Exoplanet Archive flags them that way: their signals are disputed. The scene shows them with that label instead of presenting them as certain.
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| Published | 11 days ago |
| Blender Version | 4.2 - 5.0 |
| Render Engine Used | Cycles |
| License | GPL |