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 |
Sample triples (193)
| Subject | Object |
|---|---|
| Triangulum Galaxy | z ≈ −0.000597 ⓘ |
| Small Magellanic Cloud | about 0.000527 ⓘ |
| SMACS 0723 galaxy cluster | approximately 0.39 ⓘ |
| SMACS 0723 galaxy cluster | includes galaxies with redshift greater than 8 via predicate surface "backgroundGalaxiesRedshiftRange" ⓘ |
| Andromeda IV | 0.000854 ⓘ |
| M81 Group | approximately 0.0001 to 0.0002 ⓘ |
| M32 | −0.000459 ⓘ |
| IC 10 | approximately -0.0013 ⓘ |
| NGC 6822 | −0.000163 ⓘ |
| Andromeda III | approximately −0.0011 ⓘ |
| Andromeda V | near 0 ⓘ |
| Centaurus A/M83 Group | z ≈ 0.001–0.002 (typical member range) ⓘ |
| NGC 224 | −0.001001 ⓘ |
| M31* | approximately -0.001 ⓘ |
| Andromeda IX | approximately −0.001 (approaching) ⓘ |
| NGC 598 | about −0.000597 ⓘ |
| Andromeda X | approximately −0.001 ⓘ |
| Andromeda XI | approximately −0.001 ⓘ |
| PGC 3085 | about 0.00053 ⓘ |
| Leo II Dwarf Galaxy | about 0.00026 ⓘ |
| Andromeda XIII | near zero ⓘ |
| Hydra–Centaurus Supercluster | approximately 0.01–0.03 ⓘ |
| IC 1613 | −0.000527 ⓘ |
| Andromeda XV | approximately −0.0007 ⓘ |
| Virgo Cluster | 0.0036 ⓘ |
| Norma Cluster | approximately 0.016 ⓘ |
| Andromeda XXIX | near zero (Local Group object) ⓘ |
| Andromeda XVI | near zero (Local Group object) ⓘ |
| Andromeda XVIII | approximately −0.0011 ⓘ |
| Andromeda XIX | approximately −0.001 ⓘ |
| Andromeda XXI | approximately −0.001 ⓘ |
| Andromeda XXII | very low redshift consistent with Local Group membership ⓘ |
| Andromeda XXIII | approximately −0.001 ⓘ |
| Andromeda XXIV | near zero ⓘ |
| Andromeda XXV | approximately 0 (Local Group object) ⓘ |
| Andromeda XXVI | approximately 0 ⓘ |
| Andromeda XXVIII | approximately 0 ⓘ |
| Centaurus Cluster | 0.0104 ⓘ |
| Hickson Compact Group 92 | 0.0215 ⓘ |
| HCG 92 | ~0.021 ⓘ |
|
NGC 7317 is an elliptical galaxy
surface form:
NGC 7317
|
~0.022 ⓘ |
|
NGC 7318A is an elliptical galaxy
surface form:
NGC 7318A
|
approximately 0.022 ⓘ |
|
NGC 7318B is a spiral galaxy
surface form:
NGC 7318B
|
non-zero (recessional velocity indicating cosmological distance) ⓘ |
|
NGC 7320 is a spiral galaxy
surface form:
NGC 7320
|
z ≈ 0.0027 ⓘ |
| NGC 7317 | ~0.022 ⓘ |
| NGC 7320 | z ≈ 0.0027 ⓘ |
| NGC 2403 | 0.000445 ⓘ |
| NGC 3077 | 0.000043 ⓘ |
| Holmberg II | 0.00048 ⓘ |
| Holmberg IX | approximately 0.000158 ⓘ |