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M82 (Hubble and Webb)

Left: Messier 82 as imaged by NASA's Hubble Space Telescope. Right: A section of Messier 82 as imaged by NASA's James Webb Space Telescope.

Starburst galaxy M82 was observed by the Hubble Space Telescope in 2006, which showed the galaxy’s edge-on spiral disk, shredded clouds, and hot hydrogen gas. The James Webb Space Telescope has observed M82’s core, capturing in unprecedented detail the structure of the galactic wind and characterizing individual stars and star clusters.

The Webb image is from the telescope’s NIRCam (Near-Infrared Camera) instrument. The red filaments trace the shape of the cool component of the galactic wind via polycyclic aromatic hydrocarbons (PAHs). PAHs are very small dust grains that survive in cooler temperatures but are destroyed in hot conditions. The structure of the emission is similar to that of the ionized gas, suggesting PAHs may be replenished from cooler molecular material as it is ionized.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    09:55:52.0
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    69:40:48.99
  • 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.
    12 million light-years (3.7 Megaparsecs)

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.

    Left Image: This image was created from HST data from proposal 10776 M. Mountain (STScI), J. Gallagher (University of Wisconsin-Madison), P. Puxley (NSF), K. Noll, H. Bond, C. Christian, L. Frattare, F. Hamilton, Z. Levay, M. Mutchler, W. Januszewski, and T. Royle (Hubble Heritage Team/STScI/AURA)

    Right Image: This image was created with Webb data from proposal: 1701 (M. Marin). Image processing: Alyssa Pagan (STScI).

  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/WFC JWST>NIRCam
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    27-29 March 2006, 5 Janurary 2024
  • Filters
    FiltersThe camera filters that were used in the science observations.
    HST> F435W, F555W, F658N, F814W JWST> F164N, F250W, F335M
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    M82, NGC 3034
  • Object Description
    Object DescriptionThe type of astronomical object.
    Starburst Galaxy
  • Release Date
    April 3, 2024
  • Science Release
    NASA’s Webb Probes an Extreme Starburst Galaxy
  • Credit
    Image: NASA, ESA, CSA, STScI, Alberto Bolatto (UMD)

Downloads

  • Full Res (For Print), 16260 × 7030
    tif (206.37 MB)
  • Full Res (For Display), 16260 × 7030
    png (176.1 MB)
  • 2000 × 865
    png (3.01 MB)
Left: Messier 82 as imaged by NASA's Hubble Space Telescope. Right: A section of Messier 82 as imaged by NASA's James Webb Space Telescope.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

Left Image: This image is a composite of many separate exposures made by the ACS instrument on the Hubble Space Telescope using several different filters. Three filters sample broad wavelength ranges, one isolates the light of hydrogen. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: Blue: F435W, Green: F555W, Red-orange: F658N Red: F814W Right Image: This image is a composite of separate exposures acquired by the James Webb Space Telescope using the NIRCam instrument. Several filters were used to sample varying 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:  Blue: F164N, Green: F250W, Red: F335M

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
Aug 28, 2025
Contact
Media

Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Image Credit

NASA, ESA, CSA, STScI, Alberto Bolatto (UMD)