| NGC 6624 | |
|---|---|
The globular cluster NGC 6624. Credit Hubble Space Telescope
| |
| Observation data (J2000 epoch) | |
| Constellation | Sagittarius |
| Right ascension | 18h23m41s |
| Declination | −30° 21′ 39″ |
| Distance | 25.8 ± 1.1 kly (7.91 ± 0.34 kpc) |
| Apparent magnitude (V) | 7.6 |
| Apparent dimensions (V) | 8.8 arcminutes[1] |
| Physical characteristics | |
| Metallicity | ![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c) = -0.56 ± 0.27[2] dex |
| Other designations | ESO 457-11, GCl 93, CD−30 15631, CPD−30 5486, HD 168943[3] |
| See also: Globular cluster, List of globular clusters | |
NGC 6624 is a globular cluster in the constellation Sagittarius. It was discovered on 24 June 1784 by the astronomer William Herschel. It is given an apparent magnitude of 7.6 to 8.5.[4] Six pulsars are known in NGC 6624. The first of these to be discovered was PSR J1823-3021A. This globular cluster also contains 4U 1820-30, a low-mass X-ray binary with an orbital period of only 11.5 minutes.
NGC 6624 is visible as a hazy spot with a small telescope, and appears as a star-like object with binoculars. Its core appears significantly condensed.[1] It is located 0.8 degrees southeast of the star Delta Sagittarii,[5] and is about 1.17 kpc (3.8 kly) from the Galactic Center.[2]
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