
In these pictures, a "city" of a million stars glitters like a New York City skyline. The images capture the globular cluster 47 Tucanae, located 15,000 light-years from Earth in the southern constellation Tucana.
Using NASA's Hubble Space Telescope, astronomers went hunting in this large city for planetary companions: bloated gaseous planets that snuggle close to their parent stars, completing an orbit in a quick three to five days. To their surprise, they found none. This finding suggests that the cluster's environment is too hostile for breeding planets or that it lacks the necessary elements for making them.
The picture at left, taken by a terrestrial telescope, shows most of the cluster, a tightly packed group of middle-aged stars held together by mutual gravitational attraction. The box near the center represents the Hubble telescope's view.
The image at right shows the Hubble telescope's close-up look at a swarm of 35,000 stars near the cluster's central region. The stars are tightly packed together: They're much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle-aged Sun. Most of the stars in the cluster are believed to have formed about 10 billion years ago. The bright, blue stars - thought to be remnants of stellar collisions and mergers - provide a few rejuvenated, energetic stars in an otherwise old system. The Hubble picture was taken in July 1999.
Credits
Hubble image: NASA and Ron Gilliland (Space Telescope Science Institute);Ground-based image: David Malin, © Anglo-Australian Observatory
About The Object | |
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Object Name | 47 Tucanae, NGC 104 |
Object Description | Globular Cluster |
R.A. Position | 00h 24m 5.19s |
Dec. Position | -72° 4' 49.9" |
Constellation | Tucana |
Distance | About 15,000 light-years (4.6 kpc) |
Dimensions | The width of the image is 120 arcseconds (~9 light-years). Diameter: About 200 light-years. Magnitude: V4.5, B-V0.88 |
About The Data | |
Data Description | Principal Astronomers: R. Gilliland (STScI), T. Brown (High Altitude Observatory), A. Burrows (U. Arizona), W. Cochran (U. Texas, Austin), P. Edmonds (SAO), S. Frandsen (Aarhus U.), P. GuhaThakurta (UCSC), D. Lin (UCSC), G. Marcy (UCB), M. Mayor (Observatoire de Geneve), E. Milone (U. Calgary), D. Naef (Observatoire de Geneve), A. Sarajedini (Wesleyan U.), S. Sigurdsson (PSU), D. VandenBerg (UVic), S. Vogt (UCSC), M. Albrow (STScI), N. Baliber (U. Texas, Austin), H. Bruntt (Aarhus U.), D. Charbonneau (High Altitude Observatory), P. Choi (UCSC), J. Howell (UCSC), R. Stagg (U. Calgary), M. Williams (U. Calgary). |
Instrument | AAT (left), and HST>WFPC2 (right) |
Exposure Dates | July 3 - 11, 1999, Exposure Time: 61.7 hours |
Filters | F336W (U), F555W (V), and F814W (I) |
About The Image | |
Color Info | Blue: F336W (U) Green: F555W (V) Red: F814W (I) |
About The Object | |
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Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
Object Description | The type of astronomical object. |
R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
About The Data | |
Data Description |
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Instrument | The science instrument used to produce the data. |
Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
Filters | The camera filters that were used in the science observations. |
About The Image | |
Image Credit | The primary individuals and institutions responsible for the content. |
Publication Date | The date and time the release content became public. |
Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |