| Trumpler 27 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Right ascension | 17h 36m 20s [1] |
| Declination | −33° 31.0′ [1] |
| Apparent magnitude (V) | 6.7 [1] |
| Apparent dimensions (V) | 6′ × 6′ [1] |
| Physical characteristics | |
| True nature is unknown [2] | |
| Other designations | C 1732-334 [1] |
| Associations | |
| Constellation | Scorpius |
Trumpler 27 is a possible open cluster in the southern constellation Scorpius. If it exists, it is a few thousand light-years away from the Sun, with estimates ranging from 3,900 light-years (1,210 kiloparsecs) [3] to 6,800 light-years (2,100 kiloparsecs) [4] The name refers to Robert Julius Trumpler's catalog of open clusters, published in 1930. [5]
It was originally thought to be young open cluster in the outer edge of the Sagittarius Arm, still surrounded by interstellar matter. [5] The light from the stars is heavily extinguished and reddened by intervening interstellar dust. [4] The light coming from the stars is also significantly polarized. [6] However, a close study in 2012 could not confirm whether the stars truly form a cluster, or if they are a close alignment of bright stars. [2]
Several member stars have been studied in closer detail. Star #1 of Trumpler 27 is CD−33°12241, a red supergiant star with a spectral type of M0Ia. Stars #28 and #105 are Wolf-Rayet stars. [4] [7] Star #27, a blue giant star with a spectral type of O8III((f)), may be one of the most luminous stars known, with a bolometric magnitude of −10.5. [7] Star #102 is known as V925 Scorpii or HD 159378, [8] and is a rare yellow supergiant star. [9]
