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EntityQ597212· pop 37· linked from 906 articles

Also known as Caldwell 104

globular cluster in the Milky Way galaxy

Key facts

Class
III
Constellation
Tucana
Right ascension
01 03 14.26
Declination
−70 ° 50 ′ 55.6 ″
Distance
29.29 ± 0.20 kly (8.98 ± 0.06 kpc )
Apparent dimensions v
12.9′
Metallicity
[ Fe/H ] = –1.09 dex
Estimated age
11.0 ± 0.6 Gyr
Other designations
Melotte 4

via Wikipedia infobox

Wikidata facts

Distance from Earth
8.98
Image
Caldwell 104.jpg
Show 10 more facts
time of discovery or invention
1826-08-01
Commons category
NGC 362
metallicity
-1.33
catalog code
IRAS F01015-7106
right ascension component of proper motion
1.0
apparent magnitude
6.419
right ascension
15.809417
declination
-70.848778
radial velocity
27.0
declination component of proper motion
-16.0
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via Wikidata · CC0

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Article

NGC 362 (also known as Caldwell 104) is a globular cluster located in the constellation Tucana in the Southern Hemisphere, slightly north of the Small Magellanic Cloud, to which it is completely unrelated. It was discovered on August 1, 1826, by James Dunlop. It is visible to the naked eye in dark skies, and is an impressive sight in a telescope, although it is somewhat overshadowed by its larger and brighter neighbour 47 Tucanae.

Image of NGC 362 by Hubble Space Telescope The stars of NGC 362 have an average metallicity higher than the stars in most globulars. This implies that NGC 362 is a relatively young globular cluster. It also has an overabundance of binary stars, and an exceptionally tight core 13 light-years in diameter. The orbit of NGC 362 is highly eccentric, taking it to within 3,260 light-years of the Galactic Center.

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