Hubble image archive

FRB 20220610A Compass Image

A Hubble Space Telescope image of the host galaxy of an exceptionally powerful fast radio burst, FRB 20220610A. Hubble's sensitivity and sharpness reveals a compact group of multiple galaxies that may be in the process of merging. They existed when the universe was only 5 billion...

Date
Jan 10, 2024
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2024-001-01hk5hx6qze26s2ggqb4xxyv4t
By

A Hubble Space Telescope image of the host galaxy of an exceptionally powerful fast radio burst, FRB 20220610A. Hubble's sensitivity and sharpness reveals a compact group of multiple galaxies that may be in the process of merging. They existed when the universe was only 5 billion years old. FRB 20220610A was first detected on June 10, 2022, by the Australian Square Kilometer Array Pathfinder (ASKAP) radio telescope in Western Australia. The European Southern Observatory’s Very Large Telescope in Chile confirmed that the FRB came from a distant place.

Credits

Image

NASA, ESA, STScI, Alexa Gordon (Northwestern), Joseph DePasquale (STScI)

Image Details

About The Object
Object NameFRB 20220610A
Object DescriptionFast Radio Burst in a Compact Galaxy Group
R.A. Position23:24:17.59
Dec. Position23:24:17.59
ConstellationPiscis Austrinus
Distance7.886 billion light-years (z=1.017)
DimensionsImage is 1.6 arcmin across (about 3.7 million light-years)
About The Data
Data DescriptionThis image was created with Hubble data from proposal: (A. Gordon). Image Processing: Joseph DePasquale (STScI)
InstrumentWFC3
Exposure Dates26 April and 10 June 2023
FiltersF606W, F160W
About The Image
Color InfoThese images are a composite of separate exposures acquired by the Hubble Space Telescope using the WFC3 instrument. Two filters were used to sample broad wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Orange: F160W, Cyan: F606W

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Source

Image and source material are credited to the official mission archive linked below.

View on NASA.gov

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