47 Tuc Cluster
OVERVIEW
] STAR CLUSTER47 Tuc Cluster is a globular cluster in the constellation Tucana, 15 000 from Earth, shining at apparent magnitude 4.09 (). It is catalogued as 2MASX J00240535-7204531, C 106 and HD 2051, among 11 designations in total. It was discovered in 1751.
The second-brightest globular cluster in the sky and one of the densest, with a core so crowded that stars collide and merge into blue stragglers.
- WHAT IT IS
- Globular cluster
- HOW FAR
- 15 000
- HOW BIG ON THE SKY
- 31.8
- HOW BRIGHT (V)
The light arriving now left it that long ago.
About as wide as the full Moon.
Bright enough for the naked eye, under a sky dark enough.
IMAGES
] 2 FRAMESOBSERVING
] FROM WHERE YOU AREWhat it takes to see 47 Tuc Cluster for yourself. Everything in this part of the page is worked out for a real horizon, a real night and the equipment you say you have.
Say where you are, and this line says when 47 Tuc Cluster is worth going out for.
THROUGH AN EYEPIECE
] 150 MM TELESCOPE · 25 MM EYEPIECEBright enough to see with your eyes alone, once you are away from town lights. 47 Tuc Cluster covers 31.8′ of sky against a of 1.08°, so at 48× it is comfortably framed.
- 48×
- 1.08
- 1.25
- 13.0
- SIZE ON THE SKY
- 31.8
- FILLS OF THE FIELD
- 49% of the width
- APPARENT MAGNITUDE ()
- 4.09 · within reach
47 Tuc Cluster is not a point of light, so the limit above is the wrong one to hold it against: the same brightness spread over 31.8′ of sky is harder than a star of it, and goes first. Catalogued sizes are measured to a photographic contour, and the part an eye sees is usually smaller.
APPARENT PLACE
] EQUINOX J2026.7Where a telescope has to be pointed today, which is not quite where the catalogue records the object: the coordinate grid itself has turned since the year 2000 the catalogue is referred to.
- RIGHT ASCENSION
- DECLINATION
- GRID TURNED SINCE
- 10.5
- PROPER MOTION SINCE
- none published
Computed for 2026-08-27 00:00 UT. No proper motion is published for 47 Tuc Cluster, so nothing here moves the object; what separates this from the catalogued position above is the coordinate grid turning under it — about fifty arcseconds a year of precession since 2000, and the small nodding of the Earth’s axis on top of that. Aberration and refraction are not included, and neither is parallax; each is under an arcminute, which is also about as well as the catalogued position is known. The same figure for any date.
CATALOG DATA
] 14 FIELDSThe raw catalogue values, as the source published them, with the error bars where one was published — sorted by what each set of figures is about rather than by the order they happened to be stored in.
HOW BRIGHT IT IS
What the light adds up to, measured through one filter at a time. A magnitude is a brightness on a backwards scale — the smaller the number, the brighter the object.
- Apparent magnitude ()
- Apparent magnitude ()
- Apparent magnitude ()
- Apparent magnitude ( band)
- Apparent magnitude ()
WHERE IT IS AND HOW IT MOVES
Position, motion across the sky and the size it covers on it. These are measurements of the object as seen from here, so every one of them depends on where here is.
- Radial velocity
- −17
- Redshift (z)
- Major axis
- 31.8
WHEN IT WAS FOUND
Who first saw it, from where, and by what method.
- Discovered by
- Nicolas Louis de Lacaille
OTHER NAMES AND NUMBERS
The identifiers other catalogues file this object under, for anyone joining this data to theirs.
- Also known as
- ksi Tuc, ξ Tuc
- OpenNGC type code
- GCl
- Wikidata item
- Q14276
- Wikipedia article
- 47 Tucanae
WHERE THESE FIGURES CAME FROM
Which catalogue, paper or model each of the fields above was read from, where the source named one.
- Distance catalogue entry
- NGC 104
ALSO KNOWN AS
] 11 DESIGNATIONS- 2MASX 2MASX J00240535-7204531
- Caldwell C 106
- Common name 47 Tuc Cluster
- HD HD 2051
- HIP HIP 1902
- HR HR 95
- IAU cluster C 0021-723
- IRAS IRAS 00218-7221
- IRAS IRAS F00218-7221
- MWSC MWSC 38
- NGC NGC 104
LOOK IT UP ELSEWHERE
] 3 SERVICESEach link carries the identifier printed beside it. Nothing on this page is a measurement of our own, so a number that disagrees with one of these is worth reporting — and a service that has never catalogued this object under this name will say so plainly.
- SIMBADNGC 104
Cross-identifications, measured values and the reference behind each of them.
- ADSobject:"NGC 104"
Papers indexed against this object rather than against the string, newest first.
- VizieR600″ around 6.0223 -72.0814
Every published table with a row at this position, searched by coordinates rather than by name.
CITE THIS PAGE
] DR1This page is live and its numbers move when an upstream refreshes, so the citation names the release the rows belong to rather than the day you read them. The release itself is frozen, republished as a bundle, and is what a data-availability statement should point at.
SpaceCatalog. 47 Tuc Cluster [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/ngc-104
@misc{spacecatalog_ngc-104,
author = {{SpaceCatalog}},
title = {{47 Tuc Cluster}},
howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
year = {2026},
url = {https://spacecatalog.org/object/ngc-104},
note = {Catalogue entry, data release DR1 (2026-08-21). Values from OpenNGC.}
}The values above were taken from OpenNGC — CC-BY-SA-4.0. Citing this page does not replace citing that catalogue, and its licence is share-alike: the terms reach whatever you build from these rows.
RECENT ACTIVITY
] 3 ITEMS- Euclid: The convective-transition gap of 47 Tuc2026-06-26 · arXiv · PAPER · M. Libralato, M. Griggio, R. Gerasimov, L. R. Bedin, I. McDonald, B. Altieri
- Globular Clusters in the Time of the JWST. I. Survey Design and First Results on Multiple Populations and Beyond2026-06-18 · arXiv · PAPER · A. P. Milone, A. F. Marino, G. Cordoni, E. Dondoglio, M. V. Legnardi, T. Ziliotto
- Phase-Space Crystallization in Galactic Globular Clusters: A Gaia-Based Metric and Implications for Technosignature Searches2026-05-07 · arXiv · PAPER · Bo-Lun Huang, Zhen-Zhao Tao, Tong-Jie Zhang
arXiv · UPDATED DAILY