Hubble image archive

Hubble Ultra Deep Field 2009-2010 and UDFj-39546284

The farthest and one of the very earliest galaxies ever seen in the universe appears as a faint red blob in this ultra-deep-field exposure taken with NASA's Hubble Space Telescope. This is the deepest infrared image taken of the universe. Based on the object's color, astronomers...

Date
Jan 1, 2011
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2011-05-2814-image
By

The farthest and one of the very earliest galaxies ever seen in the universe appears as a faint red blob in this ultra-deep-field exposure taken with NASA's Hubble Space Telescope. This is the deepest infrared image taken of the universe. Based on the object's color, astronomers believe it is 13.2 billion light-years away.

The most distant objects in the universe appear extremely red because their light is stretched to longer, redder wavelengths by the expansion of the universe. This object is at an extremely faint magnitude of 29, which is 500 million times fainter that the faintest stars seen by the human eye.

The dim object is a compact galaxy of blue stars that existed 480 million years after the Big Bang, only four percent of the universe's current age. It is tiny and considered a building block of today's giant galaxies. Over one hundred such mini-galaxies would be needed to make up our Milky Way galaxy.

Follow-up spectroscopic observations with the planned James Webb Space Telescope later in this decade will be needed to definitively confirm the object's distance.

The Hubble Ultra Deep Field infrared exposures were taken in 2009 and 2010, and required a total of 111 orbits or 8 days of observing. The new Wide Field Camera 3 has the sharpness and near-infrared light sensitivity that matches the Advanced Camera for Surveys' optical images and allows for such a faint object to be selected from the thousands of other galaxies in the incredibly deep images of the Hubble Ultra Deep Field.

Credits

NASA, ESA, G. Illingworth (University of California, Santa Cruz), R. Bouwens (University of California, Santa Cruz, and Leiden University), and the HUDF09 Team

Image Details

About The Object
Object NameHubble Ultra Deep Field, HUDF, and UDFj-39546284
Object DescriptionCosmological Survey and distant galaxy
R.A. Position03h 32m 38.99s
Dec. Position-27° 47' 29.04"
ConstellationFornax
DimensionsThe HUDF image is roughly 2.2 arcminutes wide.
About The Data
Data DescriptionThe image was created from Hubble data from proposal : G. Illingworth (University of California, Santa Cruz), R. Bouwens (University of California, Santa Cruz, and Leiden University), M. Carollo (Swiss Federal Institute of Technology, Zurich), M. Franx (Leiden University), I. Labbé (Carnegie Institution of Washington), D. Magee (University of California, Santa Cruz), P. Oesch (Swiss Federal Institute of Technology, Zurich), M. Stiavelli (STScI), M. Trenti (University of Colorado, Boulder), and P. van Dokkum (Yale University). The science team includes: R. Bouwens (University of California, Santa Cruz, and Leiden University), G. Illingworth (University of California, Santa Cruz), I. Labbé (Carnegie Institution of Washington), P. Oesch (Swiss Federal Institute of Technology, Zurich), M. Trenti (University of Colorado, Boulder), M. Carollo (Swiss Federal Institute of Technology, Zurich), P. van Dokkum (Yale University), M. Franx (Leiden University), M. Stiavelli (STScI), V. González and D. Magee (University of California, Santa Cruz), and L. Bradley (STScI).
InstrumentHST>WFC3/IR
Exposure DatesAugust 26, 2009 - September 14, 2010, Exposure Time: 87 hours
FiltersF105W (Y), F125W (J), and F160W (H)
About The Image
Color InfoThe image is a composite of separate exposures made by the WFC3 instrument on the Hubble Space Telescope. Three filters were used to sample broad wavelength ranges in the near infrared. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F105W (Y) Green: F125W (J) Red: F160W (H)

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Source

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

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