| Revision for Poritt's Twins | ||
| Previous Revision, by CMDR Sheehy [2023-02-13 08:00:03] | → | Selected revision, by CMDR Sheehy [2023-02-13 13:00:53] |
| DISCOVERER | ||
| CMDR Sheehy | → | CMDR Sheehy |
| NAME | ||
| Poritt's Twins | → | Poritt's Twins |
| SYSTEMNAME | ||
| Scheareou LI-H d11-27 | → | Scheareou LI-H d11-27 |
| CATEGORY | ||
| Stellar Features | → | Stellar Features |
| CATEGORY 2 | ||
| → | ||
| REGION | ||
| Sagittarius Carina Arm | → | Sagittarius Carina Arm |
| LATITUDE | ||
| → | ||
| LONGITUDE | ||
| → | ||
| CALLSIGN | ||
| → | ||
| SUMMARY | ||
| Twin close binaries provide a heart-stopping arrival and beautiful views from twin planets. | → | Twin close-orbiting binaries provide a heart-stopping arrival and beautiful views from binary planets. |
| DESCRIPTION | ||
| → | ||
The arrival at Scheareou LI-H d11-27 is hair raising! The primary Class-A star has a companion orbiting at 1.5 million kilometers.
The secondary binary has a Class-F with a Class-K orbiting at 1.2 million kilometers.
Around the CD pair are binary landable planets, from which you can observe the spectacle. However, I would not recommend walking out on the surface as the temperature exceeds your suit's limits.
Ian Poritt, a New Zealander amateur astronomer, was the first to discover a planet around a binary system. It was previous thought that binary systems would be too unstable to support a planet. A brief video tour of these binaries can be found here. | → | The arrival at Scheareou LI-H d11-27 is hair raising! The primary Class-A star has a companion orbiting at 1.5 million kilometers.
The secondary binary has a Class-F with a Class-K orbiting at 1.2 million kilometers.
Around the CD pair are binary landable planets, from which you can observe the spectacle. However, I would not recommend walking out on the surface as the temperature exceeds your suit's limits.
Ian Poritt, a New Zealander amateur astronomer, was the first to discover a planet around a binary system. It was previous thought that binary systems would be too unstable to support a planet. A brief video tour of these binaries can be found here. |
| JOURNAL | ||
| → | ||
| OBSERVATORY | ||
| → | ||
