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A globular cluster is a spheroidal conglomeration of stars that is bound together by gravity, with a higher concentration of stars towards its center. It can contain anywhere from tens of thousands to many millions of member stars, all orbiting in a stable, compact formation. Globular clusters are similar in form to dwarf spheroidal galaxies, and though…
History, History of observations & Composition
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globular clusters cluster stars star milky core galaxy way galaxies mass many luminosity distance age tidal known may formation one
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Globular cluster | Average luminosity | ~25 000 L☉ | 1.00 | infobox |
| Globular cluster | Density | ~2 stars/cubic ly | 1.00 | infobox |
| Globular cluster | Discovered | Abraham Ihle, 1665 | 1.00 | infobox |
| Globular cluster | Mass range | 1K M☉ - >1M M☉ | 1.00 | infobox |
| Globular cluster | Size range | 10-300 ly across | 1.00 | infobox |
| Globular cluster | Type | Star cluster | 1.00 | infobox |
| Globular cluster | is a | spheroidal conglomeration of stars that is bound together by gravity | 0.90 | text |
| the Sun | instance of | compared with Population I stars | 0.80 | text |
| have a higher proportion of hydrogen | instance of | compared with Population I stars | 0.80 | text |
| helium | instance of | compared with Population I stars | 0.80 | text |
| a lower proportion of heavier elements | instance of | compared with Population I stars | 0.80 | text |
| the cool but luminous red giants.Constructing a H | instance of | The diagram also includes stars in later evolutionary stages | 0.80 | text |
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