White Glaze
Description:
When star fusion processes occur near high concentrations of silicate dust, such as those found in interstellar ice fields, the substance known as White Glaze is formed. White Glaze is extremely high in nitrogen-14 and other stable nitrogen isotopes, and is thus a necessity for the sustained operation of certain kinds of control tower.
Available in 1.0 security status solar systems or lower.
Available in 1.0 security status solar systems or lower.
Structure and speed:
- Mass: 1000 kg
- Volume: 1000 m3
- Cargo capacity: 0 m3
Required skills:
- 16281 1
Graphics:
- Asteroid radius size multiplier 80
- Asteroid unit radius 1000
- Stasis Webifier Resistance 0
- Reprocessing Skill 18025
Manufacturing
Base materials:
- Heavy Water: 69
- Liquid Ozone: 35
- Strontium Clathrates: 1
- Nitrogen Isotopes: 414