Celestial hemisphere:  Southern  ·  Constellation: Tucana (Tuc)  ·  Contains:  47 Tuc Cluster  ·  NGC 104
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47 Tucanæ, Peter Hannah
47 Tucanæ
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47 Tucanæ

Getting plate-solving status, please wait...
47 Tucanæ, Peter Hannah
47 Tucanæ
Powered byPixInsight

47 Tucanæ

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Description

As I live in the northern hemisphere I cannot see 47 Tucanæ from home, but I was motivated to use a remote facility to image it following a trip to Chile, where I was able to observe 47 Tuc through the eyepiece of a 16″ Meade LX200 at the El Pangue observatory, not far from the town of Vicuña in central Chile. I do not recall the magnification used, but the view was stunning, the cluster almost filling the field of view.
For this image I used one of Telescope Live’s instruments, a 24″ Planewave CDK reflector located at their El Sauce observatory in the Rio Hurtado Valley, not far from El Pangue. I took just one sub of 10 minutes’ duration in each filter (red, green, blue and clear) to obtain the image.

47 Tucanæ is the second brightest globular cluster in the sky (the brightest being the Omega Centauri cluster, also a southern-hemisphere object though not so far south as 47 Tuc).

Globular clusters are enormous spherical conglomerations of stars, their shape being due to their self-gravity. They are found in a large halo surrounding our galaxy’s core, and have also been observed in other galaxies such as M31. The milky way has about 150 globulars in its halo and 47 Tuc is one of the largest, being about 120 light years across. It is about 13,000 light years distant and contains millions of stars. For a comparison of scale, the cluster as shown in this image is about the same size as the full Moon. In fact the cluster is even larger but an exposure long enough to reveal the outer regions would have resulted in the core being over-exposed.

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47 Tucanæ, Peter Hannah