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Crab Nebula in Multiple Wavelengths

Crab Nebula in Multiple Wavelengths

This highly detailed image of the Crab Nebula was assembled by combining data from five telescopes spanning nearly the entire breadth of the electromagnetic spectrum: The Very Large Array (radio) in red; Spitzer Space Telescope (infrared) in yellow; Hubble Space Telescope (visible) in green; XMM-Newton (ultraviolet) in blue; and Chandra X-ray Observatory (X-ray) in purple.

The Hubble visible-light image offers a very sharp view of hot filamentary structures that permeate this nebula. The infrared image includes the glow of dust particles absorbing ultraviolet and visible light, and re-radiating at lower energies (longer wavelengths) in the infrared. An energetic cloud of electrons driven by a rapidly rotating neutron star, or pulsar, at its core glows brightly in ultraviolet radiation and X-rays. The neutron star’s fierce "wind" of charged particles energized the nebula, causing it to emit the radio waves. In this color scheme used for this set of images the background stars appear blue because they have the strongest signal in the ultraviolet-light exposure.

The Crab Nebula, the result of a supernova explosion seen by Chinese and other astronomers in the year 1054, is 6,500 light-years from Earth.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 34m 31.94s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +22° 00' 52.2"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Taurus
  • 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.
    6,500 light-years (2,000 parsecs)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Crab Nebula, M1, NGC 1952
  • Object Description
    Object DescriptionThe type of astronomical object.
    Supernova remnant
  • Release Date
    May 10, 2017
  • Science Release
    Observatories Combine to Crack Open the Crab Nebula
  • Credits
    NASA, ESA, G. Dubner (IAFE, CONICET-University of Buenos Aires) et al.; A. Loll et al.; T. Temim et al.; F. Seward et al.; VLA/NRAO/AUI/NSF; Chandra/CXC; Spitzer/JPL-Caltech; XMM-Newton/ESA; and Hubble/STScI

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Crab Nebula in Multiple Wavelengths
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

Red: VLA Radio Yellow: SST Infrared Green: HST Optical Blue: XMM Ultraviolet Purple: CXO X-ray

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 12, 2025
Contact
Media

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