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Optical and X-ray Composite Image of SNR 0509-67.5

Colorful supernova remnant resembling a soap bubble.

This image of supernova remnant 0509-67.5 was made by combining data from two of NASA's Great Observatories. Optical data of SNR 0509-67.5 and its accompanying star field, taken with the Hubble Space Telescope, are composited with X-ray images from the Chandra X-ray Observatory. The result shows soft green and blue hues of heated material from the X-ray data surrounded by the glowing pink optical shell, which shows the ambient gas being shocked by the expanding blast wave from the supernova. Ripples in the shell's appearance coincide with brighter areas of the X-ray data.

The Type Ia supernova that resulted in the creation of SNR 0509-67.5 occurred nearly 400 years ago for Earth viewers. The supernova remnant lies in the Large Magellanic Cloud (LMC), a small galaxy about 170,000 light-years from Earth. The bubble-shaped shroud of gas is 23 light-years across and is expanding at more than 11 million miles per hour (5,000 kilometers per second).

Data from Hubble's Advanced Camera for Surveys, taken in 2006 with a filter that isolates light from glowing hydrogen, were combined with visible-light images of the surrounding star field that were taken with Hubble's Wide Field Camera 3 in 2010. These data were then merged with X-ray data from the Chandra X-ray Observatory taken with the Advanced CCD Imaging Spectrometer (ACIS) in 2000 and 2007.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 9m 31.69s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -67° 31' 18.0"
  • 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.
    170,000 light-years (52,000 parsecs)

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 optical image was created from Hubble data from proposals: 11015: J. Hughes, J. Warren, and L. Hovey (Rutgers University), C. Badenes (Weizmann Institute of Science, Israel), C. Smith (NOAO/CTIO), J. Vink (Space Research Organization, Netherlands), and P. Ghavamian (STScI); 12326: K. Noll, Z. Levay, M. Livio, H. Bond, C. Christian, L. Frattare, M. Mutchler, and T. Borders (Hubble Heritage Team/STScI). The X-ray data are from the CXO proposals: 776, 7635, 8554: NASA/CXC/SAO/ J.Hughes et al.
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC, HST>WFC3/UVISl, and Chandra>ACIS
  • Filters
    FiltersThe camera filters that were used in the science observations.
    HST: F475W (g), F555W (V), F658N (H-alpha+[N II]), and F814W (I) CXO: 0.2-1.5 keV and 1.5-7 keV
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    SNR 0509-67.5
  • Object Description
    Object DescriptionThe type of astronomical object.
    Supernova Remnant
  • Release Date
    January 11, 2012
  • Science Release
    Hubble Solves Mystery on Source of Supernova in Nearby Galaxy
  • Credit
    Science: NASA, ESA, and B. Schaefer and A. Pagnotta (Louisiana State University, Baton Rouge); Image: NASA, ESA, CXC, SAO, the Hubble Heritage Team (STScI/AURA), and J. Hughes (Rutgers University)

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Colorful supernova remnant resembling a soap bubble.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

This image is a composite of separate exposures acquired by the WFC3 and ACS instruments on HST, and the ACIS instrument on the Chandra X-ray Observatory. Several filters were used to sample broad and narrow wavelength ranges along with X-ray energy frequencies. 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: Orange: F814W (I) Red: F658N (H-alpha+[N II]) Light green: F555W (V) Purple: F475W (g) Green: 0.2-1.5 keV Blue: 1.5-7 keV

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