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R136a1 (short for RMC 136a1) is the most massive and luminous star known, at around 291 solar masses (M☉) and around 7.2 million times the Sun's luminosity (L☉). It is a Wolf–Rayet star at the center of R136, the central concentration of stars of the large NGC 2070 open cluster in the Tarantula Nebula (30 Doradus) in the Large Magellanic Cloud. The…
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star stars mass core helium luminosity massive r136 surface cluster hydrogen around r136a spectrum 000 times temperature luminous r136a2 would
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| R136a1 | Apparent magnitude (V) | 12.23 | 1.00 | infobox |
| R136a1 | B−V color index | 0.03 | 1.00 | infobox |
| R136a1 | Constellation | Dorado | 1.00 | infobox |
| R136a1 | Declination | −69° 06′ 02.9″ | 1.00 | infobox |
| R136a1 | Evolutionary stage | Main sequence | 1.00 | infobox |
| R136a1 | Right ascension | 5h 38m 42.39s | 1.00 | infobox |
| R136a1 | Spectral type | WN5h | 1.00 | infobox |
| R136a1 | is a | most luminous star known | 0.90 | text |
| adaptive optics or speckle interferometry.South of about the 20th parallel south | instance of | and resolving R136a to detect R136a1 requires a space telescope or sophisticated techniques | 0.80 | text |
| the LMC is circumpolar | instance of | and resolving R136a to detect R136a1 requires a space telescope or sophisticated techniques | 0.80 | text |
| meaning that it can be seen | instance of | and resolving R136a to detect R136a1 requires a space telescope or sophisticated techniques | 0.80 | text |
| R136a1 that are not in hydrostatic equilibrium | instance of | The classical Eddington luminosity limit is not applicable to stars | 0.80 | text |
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