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==Test Case: New Intrasystem Surveys== | ==Test Case: New Intrasystem Surveys== | ||
Intrasystem surveys are completed by vessels as they approach the target star system, usually within the Oort orbit of that system. The survey takes 1d10 days, usually to the maximum length when there are indications of additional planetary bodies not fully identified. The ship typically does not need to enter the system in order to complete the survey. | Intrasystem surveys are completed by vessels as they approach the target star system, usually within the Oort orbit of that system. The survey takes 1d10 days, usually to the maximum length when there are indications of additional planetary bodies not fully identified. The ship typically does not need to enter the system in order to complete the survey. | ||
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===Part 3: Assigning Orbits to Zones=== | |||
===Part 4: Planet Classes per Zones=== | |||
Reference: [[Starfleet Command:Planetary Classifications|Planetary Classifications]] | Reference: [[Starfleet Command:Planetary Classifications|Planetary Classifications]] | ||
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Revision as of 11:44, 14 August 2014
Test Case: New Intrasystem Surveys
Intrasystem surveys are completed by vessels as they approach the target star system, usually within the Oort orbit of that system. The survey takes 1d10 days, usually to the maximum length when there are indications of additional planetary bodies not fully identified. The ship typically does not need to enter the system in order to complete the survey.
Part 1: Maximum Number of Planets
| A. Main Sequence Stars | Roll for number of planets: |
| O (Blue) | none |
| B (Blue-white) | 3d6 |
| A (White) | 3d6-1 |
| F (Yellow-white) | 3d6-1 |
| G (Yellow) | 3d6-2 |
| K (Orange) | 3d6-2 |
| M (Red) | 3d6-2 |
| B. UV Sequence Stars | Roll: |
| 3d6/2 (and all are charred rockballs) | |
| C. IR Sequence Stars/Blackholes | none |
Part 2: Bode's Law
Bode's Law is a hypothesis that the bodies in some orbital systems, including Sol's, orbit at semi-major axes in a function of planetary sequence. In other words, it can be used to determine how far out from a star each planet would orbit.
Step 1: The first orbit lies at a distance of (1d6*0.1) astronomical units (AU) from the star, regardless of star class. Therefore, around any given star, the first orbit could lie anywhere from 0.1 to 0.6 AUs from the center of the star's mass. This distance (D) is also used in determining the orbital distances of all other planets.
Part 3: Assigning Orbits to Zones
Part 4: Planet Classes per Zones
Reference: Planetary Classifications
| Roll 1d100 | Planet Class |
|---|---|
| 01 - 07 | A |
| 08 - 14 | B |
| 15 - 21 | C |
| 22 - 28 | D |
| 29 - 40 | E |
| 41 - 46 | J |
| 47 - 49 | K |
| 50 - 82 | N |
| 83 - 85 | Y |
| 86 - 00 | Z |
| Roll 1d100 | Planet Class |
|---|---|
| 01 - 03 | A |
| 04 - 06 | B |
| 07 - 09 | C |
| 10 - 24 | D |
| 25 | E |
| 26 - 27 | F |
| 28 - 30 | G |
| 31 - 35 | H |
| 36 - 43 | I |
| 44 - 50 | J |
| 51 - 60 | K |
| 61 - 65 | L |
| 66 - 77 | M |
| 78 - 82 | O |
| 83 - 87 | P |
| 88 - 91 | Q |
| 92 - 93 | S |
| 94 | T |
| 95 - 00 | Z |
| Roll 1d100 | Planet Class |
|---|---|
| 01 - 02 | A |
| 03 - 05 | B |
| 06 - 11 | C |
| 12 - 39 | D |
| 40 | E |
| 41 - 42 | F |
| 43 - 45 | G |
| 46 - 58 | I |
| 59 - 66 | J |
| 67 - 71 | K |
| 72 - 76 | L |
| 77 - 79 | N |
| 80 - 85 | P |
| 86 - 91 | S |
| 92 - 94 | T |
| 95 - 00 | Z |