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Hubble Spies Most Distant Supernova Ever Seen

Hubble Spies Most Distant Supernova Ever Seen

Using NASA's Hubble Space Telescope, astronomers pinpointed a blaze of light from the farthest supernova ever seen, a dying star that exploded 10 billion years ago.

The detection and analysis of this supernova, called 1997ff, is greatly bolstering the case for the existence of a mysterious form of dark energy pervading the cosmos, making galaxies hurl ever faster away from each other. The supernova also offers the first glimpse of the universe slowing down soon after the Big Bang, before it began speeding up.

This panel of images, taken with the Wide Field and Planetary Camera 2, shows the supernova's cosmic neighborhood; its home galaxy; and the dying star itself.

Astronomers found this supernova in 1997 during a second look at the northern Hubble Deep Field [top panel], a tiny region of sky first explored by the Hubble telescope in 1995. The image shows the myriad of galaxies Hubble spied when it peered across more than 10 billion years of time and space. The white box marks the area where the supernova dwells.

The photo at bottom left is a close-up view of that region. The white arrow points to the exploding star's home galaxy, a faint elliptical. Its redness is due to the billions of old stars residing there.

The picture at bottom right shows the supernova itself, distinguished by the white dot in the center. Although this stellar explosion is among the brightest beacons in the universe, it could not be seen directly in the Hubble images. The stellar blast is so distant from Earth that its light is buried in the glow of its host galaxy.

To find the supernova, astronomers compared two pictures of the "deep field" taken two years apart. One image was of the original Hubble Deep Field; the other, the follow-up deep-field picture taken in 1997. Using special computer software, astronomers then measured the light from the galaxies in both images. Noting any changes in light output between the two pictures, the computer identified a blob of light in the 1997 picture that wasn't in the original deep-field study. That blob turned out to be the supernova. The red background texture is an artifact of the process of isolating the supernova.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    12h 36m 48.26s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    62° 13' 1.99"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Ursa Major
  • 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.
    3 billion parsecs (10 billion light-years)

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.
    Principal Astronomers: A.G. Riess (STScI), R. Thompson (U Arizona), R. Gilliland (STScI), P. Nugent (LBNL), B. Schmidt (MSSSO), J.Tonry (U Hawaii), M. Dickinson (STScI), T. Budavari (JHU), M. Livio (STScI), H. Spinrad (UC Berkeley), D. Stern (UC Berkeley), D. Sanders (U Hawaii), and S. Veilleux (U Maryland) .
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>NICMOS and HST>WFPC2
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    December 23, 1997 - June 22, 1998, Exposure Time: ~ 6 days
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F814W (I), F110W (J), F160W (H)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Hubble Deep Field-North, HDF-N, SN1997ff
  • Object Description
    Object DescriptionThe type of astronomical object.
    Supernova Type Ia in Hubble Deep Field North Galaxy 4-403.0
  • Release Date
    April 2, 2001
  • Science Release
    Blast from the Past: Farthest Supernova Ever Seen Sheds Light on Dark Universe
  • Credit
    NASA, Adam Riess (Space Telescope Science Institute, Baltimore, MD)

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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