Type ID | 7 | |
Published | False | |
Volume | 1 m3 | |
Mass | 1.00E18 kg | |
Radius | 10,000 |
Capacity | 0 m3 |
Type ID | 7 |
Graphic ID | 21459 |
Sound ID | 20095 |
Group ID | Sun [6] |
Yellow-orange and orange stars of this type are rather stable and believed to take tens of billions of years to burn through their core hydrogen reserves in a process of thermonuclear fusion.
This stability and long life, combined with the common presence of planetary systems marks these as viable candidates for colonization and exploration efforts.