Type | Open Cluster |
---|---|
Magnitude | 8.8 |
Size | 12' |
Right Ascension | 17h 40' 10" (2000) |
Declination | 36° 57' 42" S |
Constellation | Scorpius |
Description | Cl, pL, pRi, iR, *9...10 |
Classification | II2m |
Andrew Cooper
Jul 8, 2021 Waikoloa, HI (map)
20cm f/6 Newtonian, Cave Astrola @ 76x
Seeing: 7 Transparency: 6 Moon: 0%
A distinct faint cluster in rich galactic starfield, rich, partially resolved, about 10' in diameter, a notable chain of 10-12th magnitude stars radiates south from the cluster center, 1°20' east of Shaula
Andrew Cooper
Aug 7, 2020 Waikoloa, HI (map)
20cm f/6 Newtonian, Cave Astrola @ 76x
Seeing: 5 Transparency: 6 Moon: 0%
A conspicuous cluster in a rich galactic starfield, about 10' across, bright, rich, resolved
Andrew Cooper
Jun 29, 2019 Kaʻohe, Mauna Kea, HI (map)
20cm f/6 Newtonian, Cave Astrola @ 56x
Seeing: 8 Transparency: 7 Moon: 0%
A nice cluster beside the scorpion's tail, 10', rich, resolved, a pretty object for a low power telescope view
Harold Corwin
Here, coincidentally, is the next open cluster in the NGC after NGC 6396 (which see), and another object where John Herschel may have recorded the wrong wire -- his RA for the cluster is 40 seconds too small. In the sweep, he claims wire 2; if he actually observed the cluster leaving the field, his RA would be 17 40 06 for J2000, just six seconds of time off the actual RA.
As with NGC 6396, the cluster is too obvious to misidentify, even if John Herschel's mistake is not due to a wire error. He found this cluster, by the way, on 28 June 1834.― NGC Notes by Harold Corwin
Collinder 338 | HD 160668 | NGC 6396 |
NGC 6415 | PK350-2.1 | PK352-4.1 |
Q Scorpii | Ruprecht 127 | Shaula |
SL28 | SX Scorpii | Tonantzintla 2 |
Drawings, descriptions, and CCD photos are copyright Andrew Cooper unless otherwise noted, no usage without permission.
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