redshift
P22645
predicate
Indicates that the observed wavelength of light or other electromagnetic radiation from an object is shifted toward longer (redder) wavelengths, typically due to relative motion away from the observer or cosmic expansion.
All labels observed (4)
| Label | Occurrences |
|---|---|
| redshift canonical | 188 |
| redshift_approx | 3 |
| backgroundGalaxiesRedshiftRange | 1 |
| redshiftApprox | 1 |
Description generation (PDg)
The one-sentence description above was generated by prompting gpt-5.1 with the predicate name and this instruction.
Instruction
Given a predicate that represents a relationship or action between entities, generate a one-sentence description explaining its meaning. # Instructions Focus on describing the relationship, not the entities themselves. # Response Format Begin the description with \' Indicates...\'
Input
Predicate: redshift
Generated description
Indicates that the observed wavelength of light or other electromagnetic radiation from an object is shifted toward longer (redder) wavelengths, typically due to relative motion away from the observer or cosmic expansion.
Sample triples (193)
| Subject | Object |
|---|---|
| 3C 84 | 0.0176 ⓘ |
| SC 1327-312 | approximately 0.048 ⓘ |
| Abell 347 | 0.018 ⓘ |
| M66 Group | 0.002 via predicate surface "redshiftApprox" ⓘ |
| Ursa Major Cluster | approximately 0.003 ⓘ |
| Abell 3562 | ~0.048 ⓘ |
| Abell 400 | approximately 0.024 ⓘ |
| Abell 3556 | ~0.047 ⓘ |
| M96 Group | approximately 0.003 ⓘ |
| Abell 3554 | approximately 0.048 ⓘ |
| NGC 4631 Group | approximately 0.002 ⓘ |
| NGC 5866 Group | approximately 0.002–0.003 ⓘ |
| Fornax Cluster | 0.0046 ⓘ |
| Abell 3572 | approximately 0.04 ⓘ |
| Abell 3575 | nonzero cosmological redshift ⓘ |
| Abell 1736 | 0.046 ⓘ |
| Abell 3578 | nonzero cosmological redshift ⓘ |
| Caldwell 57 | z = −0.000191 ⓘ |
| Pleiades reflection nebulae | approximately zero (Galactic object) ⓘ |
| Messier 77 | 0.003793 ⓘ |
| NGC 1055 | approximately 0.0033 ⓘ |
| NGC 45 | 0.001494 ⓘ |
| NGC 1073 | 0.004037 ⓘ |
| And XX | approximately 0 ⓘ |
| Abell 3558 | 0.048 ⓘ |
| Abell 539 | approximately 0.02 ⓘ |
| Coma Cluster | 0.023 ⓘ |
| And XXVII | approximately 0 ⓘ |
| NGC 1042 | 0.0045 ⓘ |
| NGC 247 | 0.000533 ⓘ |
| Andromeda XXXI | low redshift galaxy ⓘ |
| NGC 4709 | ~0.011 ⓘ |
| NGC 4696 | 0.0099 ⓘ |
| A3526 | 0.0104 ⓘ |
| GW150914 | about 0.09 ⓘ |
| NGC 7173 | 0.0087 ⓘ |
| NGC 7174 | approximately 0.009 ⓘ |
| NGC 7176 | approximately 0.009 ⓘ |
| NGC 7172 | 0.0087 ⓘ |
| IC 4617 | ~0.036 ⓘ |
| Abell 2151 | 0.036 ⓘ |
| NGC 6207 | 0.0016 ⓘ |
|
Hercules Cluster (Abell 2151)
surface form:
Hercules Cluster
|
0.036 ⓘ |