Celestial hemisphere:  Southern  ·  Constellation: Tucana (Tuc)  ·  Contains:  47 Tuc Cluster  ·  NGC 104  ·  NGC 121
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NGC 104 - 47 Tucanae, Bruce Rohrlach
NGC 104 - 47 Tucanae
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NGC 104 - 47 Tucanae

Getting plate-solving status, please wait...
NGC 104 - 47 Tucanae, Bruce Rohrlach
NGC 104 - 47 Tucanae
Powered byPixInsight

NGC 104 - 47 Tucanae

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Description

Beautiful clear skies here in Melbourne after 11pm last night, allowing me to track down 47 Tucanae. Also known as NGC 104 and Caldwell Object 106, it is the second brightest globular cluster in our galaxy (after Omega Centauri). It is one of the most massive globular clusters within the M.Way galaxy, and contains around a million stars. At magnitude 4.0 it looks like a misty star to the naked eye observer, visually near the Small Magellanic Cloud (a dwarf satellite galaxy of the M.Way). Under ideal lighting conditions, the stars of the 47 Tucanae cluster are spread over an angular area equivalent to the full moon, even though the globular is around 13,400 light years away.

The core of 47 Tucanae has so many stars in such close proximity to each other, that if our sun and it's nearest star 'system' (the Alpha Centauri triple star) were placed within the core of 47 Tucanae, the night sky between the sun and Alpha Centauri would be lit by some 10,000 suns.

The result of this intense globular concentration of stars (of which only the tiniest fraction of the brightest are imaged here) is that there is intense gravitational interaction between the stars within the cluster, such that larger stars are shuffled inward whilst smaller stars are shuffled outward, in a process of stellar size sorting.

And finally - Hubble scanned some 34,000 stars within 47 Tucanae looking for Jupiter-sized transits - and came up empty handed, suggesting that globular clusters have very low levels of heavy elements.

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NGC 104 - 47 Tucanae, Bruce Rohrlach