An Active Centre
This swirling mass of celestial gas, dust, and stars is a moderately luminous spiral galaxy named ESO 021-G004, located just under 130 million light-years away.
This galaxy has something known as an active galactic nucleus. While this phrase sounds complex, this simply means that astronomers measure a lot of radiation at all wavelengths coming from the centre of the galaxy. This radiation is generated by material falling inwards into the very central region of ESO 021-G004, and meeting the behemoth lurking there — a supermassive black hole. As material falls towards this black hole it is dragged into orbit as part of an accretion disc; it becomes superheated as it swirls around and around, emitting characteristic high-energy radiation until it is eventually devoured.
The data comprising this image were gathered by the Wide Field Camera 3 aboard the NASA/ESA Hubble Space Telescope.
Credit:ESA/Hubble & NASA, D. Rosario et al.
About the Image
Id: | potw1951a |
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Type: | Observation |
Release date: | 23 December 2019, 06:00 |
Size: | 3553 x 3472 px |
About the Object
Name: | ESO 021-G004 |
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Type: | Local Universe : Galaxy : Type : Spiral |
Distance: | 130 million light years |
Constellation: | Chamaeleon |
Category: | Galaxies |
Wallpapers
Coordinates
Position (RA): | 13 32 39.59 |
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Position (Dec): | -77° 50' 40.34" |
Field of view: | 2.35 x 2.29 arcminutes |
Orientation: | North is 59.1° right of vertical |
Colours & filters
Band | Wavelength | Telescope |
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Optical V | 606 nm |
Hubble Space Telescope
WFC3 |
Infrared H | 1.6 μm |
Hubble Space Telescope
WFC3 |