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Spitzer Image of N 63A

Spitzer Image of N 63A
Spitzer has imaged the supernova remnant, N 63A, at infrared wavelengths. Using the IRAC detector, the image shows infrared emission at 3.6 (blue), 4.5 (green), 5.8 (orange), 8.0 (red) microns.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 35m 42.99s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -66° 2' 31.99"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Dorado
  • 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 distance to the LMC is roughly 160,000 light-years (50 kpc).

About the Data

  • Instrument
    InstrumentThe science instrument used to produce the data.
    SST>IRAC
  • Filters
    FiltersThe camera filters that were used in the science observations.
    3.6 microns, 4.5 microns, 5.8 microns, 8.0 microns
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    LMC N 63A
  • Object Description
    Object DescriptionThe type of astronomical object.
    Supernova Remnant
  • Release Date
    June 7, 2005
  • Science Release
    Supernova Remnant Menagerie
    Read the release
  • Credit
    NASA/JPL-Caltech/Y.-H. Chu (UIUC)

Downloads

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Spitzer Image of N 63A
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

Blue: 3.6 microns Green: 4.5 microns Orange: 5.8 microns Red: 8.0 microns

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Supernova Remnant N 63A Menagerie

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Supernova Remnant N 63A

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Chandra 3-Color X-ray Image of N 63A

Chandra 3-Color X-ray Image of N 63A

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Supernova Remnant LMC N 63A in X-Ray, Optical and Radio Radiation

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Supernova Remnant Menagerie

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The Hubble Space Telescope's Wide Field Planetary Camera 2 (WFPC2) was used to obtain images of a violent and chaotic-looking mass of gas and dust known as N 63A. The dissolve sequence builds from a Spitzer telescope infrared image of the area, adding the Chandra X-ray image,...

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Last Updated
Mar 28, 2025
Contact
Media

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

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