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Lensing Close-up

Close-up of arc and line indicating area of maximum magnification

Detailed View: Star Earendel on the Line of Extreme Magnification

This detailed view highlights the star Earendel's position along a ripple in space-time (dotted line) that magnifies it and makes it possible for the star to be detected over such a great distance—nearly 13 billion light-years. Also indicated is a cluster of stars that is mirrored on either side of the line of magnification. The distortion and magnification are created by the mass of a huge galaxy cluster located in between Hubble and Earendel. The mass of the galaxy cluster is so great that it warps the fabric of space, and looking through that space is like looking through a magnifying glass—along the edge of the glass or lens, the appearance of things on the other side are warped as well as magnified.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    01:37:23.23
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -08:27:52.20
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Cetus
  • 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.
    The star is approximately 12.9 billion light-years away.

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.

    This Hubble image was created from HST data from proposals: 14096 (D. Coe) and 15842 (D. Coe). 

  • Instrument
    InstrumentThe science instrument used to produce the data.
    ACS/WFC, WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    7 June 2016, 17July 2016, 4 November 2019, and 27 November 2019
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F814W, F105W, F110W, F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Earendel
  • Object Description
    Object DescriptionThe type of astronomical object.
    Distant star
  • Release Date
    March 30, 2022
  • Science Release
    Record Broken: Hubble Spots Farthest Star Ever Seen
  • Credit
    NASA, ESA, Brian Welch (JHU), Dan Coe (STScI); Image Processing: NASA, ESA, Alyssa Pagan (STScI)

Downloads

  • Full Res, 625 × 491
    tif (8.81 MB)
  • Full Res, 625 × 491
    png (1.45 MB)
Close-up of arc and line indicating area of maximum magnification
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images are a composite of separate exposures acquired by the ACS/WFC and the WFC3/IR instruments on the Hubble Space Telescope. Several filters were used to sample narrow and wide 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: Blue: F814W Green: F105W Red: F110W + F160W

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Details

Last Updated
Mar 28, 2025
Contact
Media

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