About the Object
270 million light years|
Picture of the Month
|Position (RA):||1 7 47.18|
|Position (Dec):||-17° 30' 19.68"|
|Field of view:||1.86 x 1.78 arcminutes|
|Orientation:||North is 98.1° left of vertical|
Colours & filters
|Infrared||1.5 μm||James Webb Space Telescope|
|Infrared||2.0 μm||James Webb Space Telescope|
|Infrared||3.56 μm||James Webb Space Telescope|
|Infrared||5.6 μm||James Webb Space Telescope|
|Infrared||15 μm||James Webb Space Telescope|
|Infrared||4.44 μm||James Webb Space Telescope|
|Infrared||7.7 μm||James Webb Space Telescope|
Webb Explores a Pair of Merging Galaxies
This image from the NASA/ESA/CSA James Webb Space Telescope depicts IC 1623, an entwined pair of interacting galaxies which lies around 270 million light-years from Earth in the constellation Cetus. The two galaxies in IC 1623 are plunging headlong into one another in a process known as a galaxy merger. Their collision has ignited a frenzied spate of star formation known as a starburst, creating new stars at a rate more than twenty times that of the Milky Way galaxy.
This interacting galaxy system is particularly bright at infrared wavelengths, making it a perfect proving ground for Webb’s ability to study luminous galaxies. A team of astronomers captured IC 1623 across the infrared portions of the electromagnetic spectrum using a trio of Webb’s cutting-edge scientific instruments: MIRI, NIRSpec, and NIRCam. In so doing, they provided an abundance of data that will allow the astronomical community at large to fully explore how Webb’s unprecedented capabilities will help to unravel the complex interactions in galactic ecosystems. These observations are also accompanied by data from other observatories, including the NASA/ESA Hubble Space Telescope, and will help set the stage for future observations of galactic systems with Webb.
The merger of these two galaxies has long been of interest to astronomers, and has previously been imaged by Hubble and by other space telescopes. The ongoing, extreme starburst causes intense infrared emission, and the merging galaxies may well be in the process of forming a supermassive black hole. A thick band of dust has blocked these valuable insights from the view of telescopes like Hubble. However, Webb’s infrared sensitivity and its impressive resolution at those wavelengths allows it to see past the dust and has resulted in the spectacular image above, a combination of MIRI and NIRCam imagery.
The luminous core of the galaxy merger turns out to be both very bright and highly compact, so much so that Webb’s diffraction spikes appear atop the galaxy in this image. The 8-pronged, snowflake-like diffraction spikes are created by the interaction of starlight with the physical structure of the telescope. The spiky quality of Webb’s observations is particularly noticeable in images containing bright stars, such as Webb’s first deep field image.
MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.
NIRSpec was built for the European Space Agency (ESA) by a consortium of European companies led by Airbus Defence and Space (ADS) with NASA’s Goddard Space Flight Center providing its detector and micro-shutter subsystems.
Results based on this observation of IC 1623 have been published in the Astrophysical Journal.
[Image description: The two galaxies swirl into a single chaotic object in the centre. Long, blue spiral arms stretch vertically, faint at the edges. Hot gas spreads horizontally over that, mainly bright red with many small gold spots of star formation. The core of the merging galaxies is very bright and radiates eight large, golden diffraction spikes. The background is black, with many tiny galaxies in orange and blue.]
- Image B
- Slider Tool
- Video: Webb’s Three Views of IC 1623
- Video: Pan of IC 1623
- Video: Hubble and Webb's Views of IC 1623
ESA/Webb, NASA & CSA, L. Armus & A. Evans
Acknowledgement: R. Colombari
About the Image
|Release date:||25 October 2022, 06:00|
|Size:||1774 x 1693 px|