Hubble Observes Infant Stars in Nearby Galaxy
Release Date: January 08, 2007 12:20PM (EST)
Read the Release: 2007-04
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About This Image
This new image taken with NASA's Hubble Space Telescope depicts bright, blue, newly formed stars that are blowing a cavity in the center of a star-forming region in the Small Magellanic Cloud.
At the heart of the star-forming region, lies star cluster NGC 602. The high-energy radiation blazing out from the hot young stars is sculpting the inner edge of the outer portions of the nebula, slowly eroding it away and eating into the material beyond. The diffuse outer reaches of the nebula prevent the energetic outflows from streaming away from the cluster.
Ridges of dust and gaseous filaments are seen towards the northwest (in the upper-left part of the image) and towards the southeast (in the lower right-hand corner). Elephant trunk-like dust pillars point towards the hot blue stars and are tell-tale signs of their eroding effect. In this region it is possible with Hubble to trace how the star formation started at the center of the cluster and propagated outward, with the youngest stars still forming today along the dust ridges.
The Small Magellanic Cloud, in the constellation Tucana, is roughly 200,000 light-years from the Earth. Its proximity to us makes it an exceptional laboratory to perform in-depth studies of star formation processes and their evolution in an environment slightly different from our own Milky Way.
Dwarf galaxies such as the Small Magellanic Cloud, with significantly fewer stars compared to our own galaxy, are considered to be the primitive building blocks of larger galaxies. The study of star formation within this dwarf galaxy is particularly interesting to astronomers because its primitive nature means that it lacks a large percentage of the heavier elements that are forged in successive generations of stars through nuclear fusion.
These observations were taken with Hubble's Advanced Camera for Surveys in July 2004.
Filters that isolate visible and infrared light were combined with a filter that samples the hydrogen and nitrogen emission from the glowing clouds.
| About The Object | |
|---|---|
| Object Name | NGC 602, N90 |
| Object Description | Cluster within Star-Forming Region in the Small Magellanic Cloud. |
| R.A. Position | 01h 29m 30.0s |
| Dec. Position | -73° 33' 59.99" |
| Constellation | Tucana |
| Distance | Approximately 196,000 light-years (61 kiloparsecs). |
| Dimensions | This image is roughy 3 arcminute (180 light-years or 55 parsecs) wide. |
| About The Data | |
| Data Description | The Hubble image was created from HST data from proposal 10248: A. Nota (STScI/ESA), M. Sirianni (STScI/ESA), E. Sabbi (University of Bologna), M. Tosi (INAF - Bologna Observ.), J. Gallagher (University of Wisconsin), M. Meixner (STScI), M. Clampin (Goddard Space Flight Center), S. Oey (University of Michigan), A. Pasquali (ETH, Zurich), L. Smith (University College London), and R. Walterbos (New Mexico State University). The science team also includes L. Carlson (Johns Hopkins University). |
| Instrument | HST>ACS/WFC |
| Exposure Dates | July 14/18, 2004 |
| Filters | F555W (V), F814W (I), F658N (Halpha+[N II]), and F814W (I) |
| About The Image | |
| Color Info | This image is a composite of many separate exposures made by the ACS instrument on the Hubble Space Telescope using several different filters. Two filters were used to sample broad wavelength ranges. One filter was used to sample narrow wavelength emission. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F555W (V) Green: F555W (V) + F814W (I) Red: F658N (Halpha+[N II]) + F814W (I) |
| Compass Image |  |
| About The Object | |
|---|---|
| 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 |
|
| 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. |