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Supernova Remnant N 63A

Supernova Remnant N 63A
A color composite of Spitzer infrared, Chandra X-ray and ground-based Halpha. The color assignments are: Chandra (all bands) (blue), CTIO ground-based H-alpha (green), Spitzer 4.5 micron (yellow) and Spitzer 8.0 micron (red).

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, CXO>X-ray, CTIO>Curtis Schmidt
  • Filters
    FiltersThe camera filters that were used in the science observations.
    CXO: X-ray CTIO: H-alpha IRAC: 4.5 micro and 8.0 micron
  • 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/CXC/NOAO/AURA/NSF

Downloads

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

Blue: X-ray Green: H-alpha Yellow: 4.5 micro Red: 8.0 micron

Related Images & Videos

Supernova Remnant N 63A Menagerie

Supernova Remnant N 63A Menagerie

A violent and chaotic-looking mass of gas and dust is seen in this Hubble Space Telescope image of a nearby supernova remnant. Denoted N 63A, the object is the remains of a massive star that exploded, spewing its gaseous layers out into an already turbulent region. The supernova...

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.

Supergiant Shell LMC-4 in the Large Magellanic Cloud

Supergiant Shell LMC-4 in the Large Magellanic Cloud

An image of the Supergiant Shell LMC-4 in the Large Magellanic Cloud, taken with the Curtis Schmidt telescope at Cerro Tololo Inter-American Observatory (CTIO) as part of the Magellanic Clouds Emission Line Survey (MCELS).

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

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

Chandra's image of N63A shows material heated to about ten million degrees Celsius by a shock wave generated by the supernova explosion. The fluffy crescent-shaped X-ray features that appear around the edge of the remnant are thought to be fragments of high-speed matter shot out...

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

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

Chandra has imaged the glowing shell created by the destruction of a massive star. X-rays from Chandra (blue), combined with optical (green) and radio (red) data, reveal new details in the supernova remnant, LMC N 63A. The X-ray glow is from material heated to about ten million...

Supernova Remnant Menagerie

Supernova Remnant Menagerie

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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Details

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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