metallicity
P7287
predicate
Indicates the proportion of an object's mass that is made up of elements heavier than hydrogen and helium, typically used to describe the chemical richness of stars or galaxies.
All labels observed (26)
| Label | Occurrences |
|---|---|
| metallicity canonical | 200 |
| hasMetallicity | 58 |
| metallicityFeH | 57 |
| metallicity_FeH | 56 |
| metallicity_Fe_H | 39 |
| metallicity[Fe/H] | 14 |
| metallicityRelativeToSun | 12 |
| hasMetallicityFeH | 11 |
| hasMetallicity_FeH | 11 |
| metallicityClass | 6 |
| meanMetallicity | 3 |
| metallicity_Fe/H | 3 |
| hasMeanMetallicity | 2 |
| hasMetallicity[Fe/H] | 2 |
| hasTypicalMetallicity | 2 |
| metallicity_approx | 2 |
| gasMetallicity | 1 |
| hasMeanMetallicity_approx | 1 |
| hasMetallicity_Fe/H | 1 |
| meanMetallicity_Fe_H | 1 |
| metalRicherThan | 1 |
| metallicityIndicator | 1 |
| metallicity_FeH_approx | 1 |
| metallicity_Z | 1 |
| metallicity_mean_approx | 1 |
| metallicity_relativeToSun | 1 |
Sample triples (488)
| Subject | Object |
|---|---|
| Sun | about Z = 0.013–0.02 ⓘ |
| Sol | approximately 0.0134 via predicate surface "metallicity_Z" ⓘ |
| Triangulum Galaxy | sub-solar average metallicity ⓘ |
| Large Magellanic Cloud | lower than Milky Way average ⓘ |
| Small Magellanic Cloud | low compared to Milky Way ⓘ |
| Sagittarius Dwarf Spheroidal Galaxy | low average metallicity compared to the Sun ⓘ |
| Canis Major Dwarf Galaxy | metal-poor compared to the Sun ⓘ |
|
Aldebaran (foreground star, not a member)
surface form:
Aldebaran
|
about −0.15 via predicate surface "metallicity[Fe/H]" ⓘ |
|
23 Tauri (star traditionally named Merope)
surface form:
23 Tauri
|
near solar via predicate surface "metallicity_Fe_H" ⓘ |
| Tau Ceti | about −0.5 via predicate surface "metallicity_Fe_H" ⓘ |
| Epsilon Eridani | sub-solar via predicate surface "metallicity_Fe_H" ⓘ |
|
globular star cluster M13
surface form:
M13
|
[Fe/H] ≈ −1.5 ⓘ |
| Andromeda IV | low metallicity ⓘ |
| Open cluster M11 | near-solar ⓘ |
| Open cluster M25 | ~0.0 via predicate surface "metallicity_Fe_H" ⓘ |
| M110 | relatively metal-rich for a dwarf galaxy ⓘ |
| IC 10 | sub-solar ⓘ |
| NGC 6822 | low ⓘ |
| Andromeda I | low ⓘ |
| Kaus Australis | −0.04 via predicate surface "hasMetallicity_FeH" ⓘ |
| Andromeda III | low ⓘ |
| Andromeda V | low ⓘ |
| Messier 22 | [Fe/H] ≈ −1.7 ⓘ |
| Andromeda VI | [Fe/H] ≈ -1.3 via predicate surface "metallicity_mean_approx" ⓘ |
| LMC | ~0.5 via predicate surface "metallicity_relativeToSun" ⓘ |
| NGC 205 | sub-solar ⓘ |
| Andromeda VII | low ⓘ |
| Andromeda IX | low metallicity ⓘ |
| Messier 28 | low ⓘ |
| Magellanic Stream | sub‑solar via predicate surface "gasMetallicity" ⓘ |
| Andromeda X | low ⓘ |
| Messier 54 | -1.5 via predicate surface "metallicity_Fe_H" ⓘ |
| Leo I Dwarf Galaxy | -1.4 via predicate surface "metallicity_Fe_H" ⓘ |
| Andromeda XI | low metallicity ⓘ |
| Messier 55 | about −1.9 via predicate surface "metallicityFeH" ⓘ |
| SMC | low ⓘ |
| SMC | ~0.2 Z☉ via predicate surface "metallicityRelativeToSun" ⓘ |
| Nubecula Minor | low metallicity compared to Milky Way via predicate surface "hasMetallicity" ⓘ |
|
47 Tucanae (in its vicinity on the sky)
surface form:
47 Tucanae
|
relatively metal-rich for a globular cluster ⓘ |
| PGC 3085 | lower than Milky Way ⓘ |
| ESO 029- G 011 | lower than that of the Milky Way ⓘ |
| Leo II Dwarf Galaxy | low metallicity ⓘ |
| Andromeda XII | low ⓘ |
| Messier 69 | high ⓘ |
| Messier 69 | about −0.6 via predicate surface "metallicityFeH" ⓘ |
| SagDEG | [Fe/H] ≈ −1.0 to −1.5 via predicate surface "hasMeanMetallicity_approx" ⓘ |
| M54 | about −1.5 via predicate surface "metallicityFeH" ⓘ |
| Terzan 7 | metal-rich ⓘ |
| Terzan 7 | about −0.6 dex via predicate surface "metallicityFeH" ⓘ |
| Arp 2 | low-metallicity globular cluster ⓘ |