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SN 2017ein in NGC 3938

SN 2017ein in NGC 3938

Astronomers Find a Supernova's Progenitor Star in Hubble Images

This NASA Hubble Space Telescope image of the nearby spiral galaxy NGC 3938 shows the location of supernova 2017ein, in a spiral arm near the bright core. The exploded star is a Type Ic supernova, thought to detonate after its massive star has shed or been stripped of its outer layers of hydrogen and helium.

Progenitor stars to Type Ic supernovas have been hard to find. But astronomers sifting through Hubble archival images may have uncovered the star that detonated as supernova 2017ein. The location of the candidate progenitor star is shown in the pullout box at bottom left, taken in 2007. The bright object in the box at bottom right is a close-up image of the supernova, taken by Hubble in 2017, shortly after the stellar blast.

NGC 3938 resides 65 million light-years away in the constellation Ursa Major. The Hubble image of NGC 3938 was taken in 2007.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    11:52:53.19
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +44:07:25.63
  • 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.
    NGC 3938 is located 65 million light-years away from Earth.
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is about 2.5 arcmin across (31,000 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.
    The HST observations include those from programs 10877 (W. Li), 14645 (S. Van Dyk)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFPC2, WFC3
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    April 2007 and June 2017
  • Filters
    FiltersThe camera filters that were used in the science observations.
    WFPC2: F814W, F555W, WFC3: F438W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    SN 2017ein in NGC 3938
  • Object Description
    Object DescriptionThe type of astronomical object.
    Progenitor of Type Ic supernova
  • Release Date
    November 15, 2018
  • Science Release
    Astronomers Find Possible Elusive Star Behind Supernova
  • Credit
    NASA, ESA, S. Van Dyk (Caltech), and W. Li (University of California)

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SN 2017ein in NGC 3938
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 WFPC2 and WFC3 instruments on the Hubble Space Telescope. Several filters were used to sample narrow 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: Cyan: F555W Orange: F814W

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
Mar 28, 2025
Contact
Media

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