NASA's Hubble Space Telescope has pinpointed the source of one of the most puzzling blasts of high-energy radiation ever observed. It is at the very center of a small, distant galaxy, which appears to be sending a beam of radiation directly toward Earth.
The 3.8-billion-light-year-distant galaxy appears as a bright blob at the center of the Hubble picture.
This observation may support the idea that a supermassive black hole at the core of the galaxy has gravitationally torn apart and swallowed a bypassing star. As the star's gas falls onto the black hole, radiation is ejected along a narrow beam.
On March 28, 2011, NASA's Swift satellite, which looks for transient X-rays and gamma rays, detected the first of a string of powerful bursts of high-energy radiation that has lasted for a week.
More Hubble observations are planned to see if the core changes brightness. An armada of ground- and space-based telescopes is also watching the object from X-ray through radio wavelengths. The Hubble observations were taken in visible and near-infrared light on April 4, 2011, with the Wide Field Camera 3. This Hubble image was taken in visible light.
Credits
NASA, ESA, and A. Fruchter (STScI)| About The Object | |
|---|---|
| Object Name | GRB 110328A |
| Object Description | High-Energy Transient Event |
| R.A. Position | 16h 44m 49s.3 |
| Dec. Position | +57° 34' 51" |
| Constellation | Draco |
| Distance | About 3.8 billion light-years or 920 megaparsecs (z=0.35) |
| Dimensions | The image is 23.6 arcseconds wide. |
| About The Data | |
| Data Description | The image was created from Hubble data from proposal : A. Fruchter (STScI), J. Bloom and S. Cenko (University of California, Berkeley), J. Graham (Johns Hopkins University), A. Levan (University of Warwick, UK), K. Misra (STScI), D. Perley (California Institute of Technology), and N. Tanvir and K. Wiersema (University of Leicester, UK). |
| Instrument | HST>WFC3/UVIS |
| Exposure Dates | April 4, 2011, Exposure Time: 21 minutes |
| Filters | F606W (wide V) |
| About The Image | |
| Color Info | This image is a composite of separate exposures acquired by the WFC3/UVIS instrument on HST. A single filter (F606W) was used to sample a broad wavelength range. Color has been applied to represent brightness, mapping data values into a range of hues from black through red, orange and yellow, to white. |
| 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. |
