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Faint Compact Galaxy in the Early Universe

Faint Compact Galaxy in the Early Universe

This is a Hubble Space Telescope view of a very massive cluster of galaxies, MACS J0416.1-2403, located roughly 4 billion light-years away and weighing as much as a million billion suns. The cluster's immense gravitational field magnifies the image of galaxies far behind it, in a phenomenon called gravitational lensing.

The inset is an image of an extremely faint and distant galaxy that existed only 400 million years after the big bang. Hubble captured it because the gravitational lens makes the galaxy appear 20 times brighter than normal. The object is comparable in size to the Large Magellanic Cloud (LMC), a diminutive satellite galaxy of our Milky Way. It is rapidly making stars at a rate ten times faster than the LMC. The object might be the growing core of what was to eventually evolve into a full-sized galaxy. The research team has nicknamed the object Tayna, which means "first-born" in Aymara, a language spoken in the Andes and Altiplano regions of South America.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    04h 16m 9.89s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -24° 3' 58.0"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Eridanus
  • Distance
    DistanceThe 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.
    Redshift: z = 0.396

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    MACS J0416-2403, MACS J0416.1-2403 is part of the Frontier Fields Program. These data were observed via the HST proposals: 13496: J. Lotz (STScI) et al.; 12459: M. Postman (STScI) et al. Supplemental data were obtained by proposal 13386, PI: S. Rodney (JHU) et al. The science team comprises: L. Infante (Pontifica Universidad Católica de Chile), W. Zheng (JHU), N. Laporte and P. Troncoso (Pontifica Universidad Católica de Chile), A. Molino (University of São Paulo, Brazil/Instituto de Astrofisica de Andalucia/CSIC, Spain), J. Diego (University of Cantabria, Spain), F. Bauer (Millennium Institute of Astrophysics, Chile/Space Science Institute, Boulder), A. Zitrin (Caltech), J. Moustakas (Siena College, NY), X. Huang (University of Science and Technology of China), X. Shu (Anhui Normal University, China), D. Bina (IRAP/CNRS Toulouse, France), G. Brammer (STScI), T. Broadhurst (University of Basque Country/IKERBASQUE, Basque Foundation for Science, Spain), H. Ford (JHU), and S. Garcia and S. Kim (Pontifica Universidad Católica de Chile).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC and HST>WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    January 5 - September 28, 2014
  • Filters
    FiltersThe camera filters that were used in the science observations.
    ACS/WFC: F435W (I) and F606W (R); ACS/WFC: F814W (I) and WFC3/IR F105W (Y); WFC3/IR: F125W (J), F140W (JH), and F160W (H)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    MACS J0416.1-2403
  • Object Description
    Object DescriptionThe type of astronomical object.
    Strong-lensing cluster
  • Release Date
    December 3, 2015
  • Science Release
    NASA Space Telescopes See Magnified Image of the Faintest Galaxy from the Early Universe
  • Credits
    NASA, ESA, and L. Infante (Pontificia Universidad Católica de Chile)

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Faint Compact Galaxy in the Early Universe
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

This image is a composite of separate exposures acquired by the WFC3/IR and ACS/WFC instruments. Several filters were used to sample various wavelengths. 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: Blue: F435W (I) + F606W (R) Green: F814W (I) + WFC3/IR F105W (Y) Red: F125W (J) + F140W (JH) + F160W (H)

Compass and Scale
Compass and ScaleAn astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

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Details

Last Updated
Feb 17, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, MD
claire.andreoli@nasa.gov