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SN 2013ge in NGC 3287
Hubble images of galaxy NGC 3287 show supernova 2013ge fading over time, revealing the steady source of ultraviolet light astronomers have identified as its binary companion star.
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.10:34:47.27
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.+21:38:54.04
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Leo
- DistanceDistanceThe 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.About 47 million light-years
- DimensionsDimensionsThe physical size of the object or the apparent angle it subtends on the sky.Image is about 2.26 arcmin across (about 31,000 light-years)
About the Data
- Data DescriptionData 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. - InstrumentInstrumentThe science instrument used to produce the data.WFC3/UVIS
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.Oct 2016, May 2019, Oct 2020
- FiltersFiltersThe camera filters that were used in the science observations.F555W, F814W
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.SN 2013ge in NGC 3287
- Object DescriptionObject DescriptionThe type of astronomical object.A spiral galaxy with a supernova.
- Release DateMay 5, 2022
- Science ReleaseHubble Reveals Surviving Companion Star in Aftermath of Supernova
- CreditNASA, ESA, Ori Fox (STScI); Image Processing: Joseph DePasquale (STScI)
These images are a composite of separate exposures acquired by the WFC3 instrument 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: F555WOrange: F814W

Related Images & Videos
Supernova and Remnant Star Illustration
This artist's illustration shows supernova 2013ge, with its companion star at lower right. The companion star is impacted by the blast wave from the supernova, but not destroyed. Over time astronomers observed the ultraviolet (UV) light of the supernova fading, revealing a...
Evolution Scenario for a Stripped Envelope Supernova Illustration
This infographic shows the evolution astronomers propose for supernova (SN) 2013ge. Panels 1-3 show what has already occurred, and panels 4-6 show what may take place in the future. 1) A binary pair of massive stars orbit one another. 2) One star ages into its red giant stage,...
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov