tidalRadius_pc
P56976
predicate
Indicates the radius, measured in parsecs, within which an object (such as a star cluster or satellite) remains gravitationally bound before external tidal forces dominate.
Observed surface forms (3)
| Surface form | Occurrences |
|---|---|
| hasTidalRadius | 4 |
| hasTidalRadius_pc | 1 |
| tidalRadius_ly | 1 |
Sample triples (9)
| Subject | Object |
|---|---|
| Open cluster M25 | ~7.7 ⓘ |
| Messier 54 | about 150 via predicate surface "tidalRadius_ly" ⓘ |
| Beehive Cluster | about 12 ⓘ |
| Messier 44 | about 39 light-years via predicate surface "hasTidalRadius" ⓘ |
| Messier 41 | about 26 light-years via predicate surface "hasTidalRadius" ⓘ |
| NGC 2362 | about 10 light-years via predicate surface "hasTidalRadius" ⓘ |
| Melotte 88 | about 12 via predicate surface "hasTidalRadius_pc" ⓘ |
| NGC 2632 | about 12 ⓘ |
| M30 | about 18.3 arcminutes via predicate surface "hasTidalRadius" ⓘ |