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M82 (NIRCam Image)

Astronomers used the James Webb Space Telescope to look toward M82’s center, where a galactic wind is being launched as a result of rapid star formation and subsequent supernovas. Studying the galactic wind can offer insight into how the loss of gas shapes the future growth of the galaxy.
This image from Webb’s NIRCam (Near-Infrared Camera) instrument shows M82’s galactic wind via emission from sooty chemical molecules known as 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 resembles that of hot, ionized gas, suggesting PAHs may be replenished by continued ionization of molecular gas.
In this image, light at 3.35 microns is colored red, 2.50 microns is green, and 1.64 microns is blue (filters F335M, F250M, and F164N, respectively).
About the Object
- R.A. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.09:55:52.0
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.69:40:48.99
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Ursa Major
- 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.12 million light-years (3.7 Megaparsecs)
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.This image was created with Webb data from proposal: 1701 (M. Marin). Image processing: Alyssa Pagan (STScI).
- InstrumentInstrumentThe science instrument used to produce the data.JWST>NIRCam
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.5 Janurary 2024
- FiltersFiltersThe camera filters that were used in the science observations.JWST> F164N, F250W, F335M
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.M82, NGC 3034
- Object DescriptionObject DescriptionThe type of astronomical object.Starburst Galaxy
- Release DateApril 3, 2024
- Science ReleaseNASA’s Webb Probes an Extreme Starburst Galaxy
- CreditImage: NASA, ESA, CSA, STScI, Alberto Bolatto (UMD)

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
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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov
NASA, ESA, CSA, STScI, Alberto Bolatto (UMD)