Suggested Searches

1 min read

Trifid Nebula (Wide Field Camera 3 Image)

A tightly cropped Hubble view of a vast star-forming region known as the Trifid Nebula. The top left is bright blue. Brown and amber colors run from top right through the center in irregular, overlapping lines to the bottom-center. At bottom right, the view is almost black. Tiny, amber-colored stars appear throughout the scene. Toward the left there is a prominent brown shape that looks like a head with two horns. The left horn points left and is wavy. The right horn is triangular and points up. The brown dust continues, flowing down, as if along a back, and up toward the top right. A prominent line, about the same length as the left horn, appears below the middle of the body, and changes from orange to red. A small, separate semi-transparent pillar is left of the head. A few slightly larger, blue foreground stars with four diffraction spikes appear throughout.

The colors in this image from NASA's Hubble Space Telescope tell a story about density in the Trifid Nebula, a star-forming region about 5,000 light-years from Earth. The top left, where it is bright blue, has the smallest amount of dust. Here, powerful ultraviolet light stripped electrons from nearby gas, creating a glow, with winds creating a bubble by clearing out surrounding dust.

An example of active cloud destruction is toward the top of the head-shaped area with two “horns.” Bright yellow gas streams upward where gas and dust are being destroyed.

Thicker dust appears dark brown, like mud. In the far-right corner, which is nearly pitch black, the dust is the densest.

Fully formed stars — bright orange orbs — are scattered across the scene. Their light and stellar winds have also cleared the immediate areas around them.

Over millions of years, the gas and dust that make up this nebula (also known as Messier 20 or M20) will disappear and only stars will remain.

Compare the 2026 view to Hubble's 1997 observation.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    18:02:23
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -23:01:48
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Sagittarius
  • 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.
    5,000 light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is 2.7 arcmin across (about 4 light-years)

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.

    These images were created with Hubble data from proposal: 18209 (C. Britt).

  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    February 20-22, 2026
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F502N (OII), F656N (H-alpha), F673N (SIII)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Trifid Nebula, Messier 20
  • Object Description
    Object DescriptionThe type of astronomical object.
    Emission Nebula, H II region
  • Release Date
    April 20, 2026
  • Science Release
    NASA’s Hubble Dazzles With Young Stars in Trifid Nebula
  • Credit
    Image: NASA, ESA, STScI; Image Processing: Joseph DePasquale (STScI)

Downloads

  • Full Res (For Display), 4074 × 3943
    png (26.36 MB)
  • Full Res (For Print), 4074 × 3943
    tif (28.37 MB)
  • Full Res (JPG), 4074 × 3943
    jpg (5.48 MB)
  • 2000 × 1936
    jpg (994.05 KB)
A tightly cropped Hubble view of a vast star-forming region known as the Trifid Nebula. The top left is bright blue. Brown and amber colors run from top right through the center in irregular, overlapping lines to the bottom-center. At bottom right, the view is almost black. Tiny, amber-colored stars appear throughout the scene. Toward the left there is a prominent brown shape that looks like a head with two horns. The left horn points left and is wavy. The right horn is triangular and points up. The brown dust continues, flowing down, as if along a back, and up toward the top right. A prominent line, about the same length as the left horn, appears below the middle of the body, and changes from orange to red. A small, separate semi-transparent pillar is left of the head. A few slightly larger, blue foreground stars with four diffraction spikes appear throughout.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images were acquired by the WFC3/UVIS instrument on Hubble. The color results from assigning different hues (colors) to a monochromatic (grayscale) image. In this case, the assigned colors are: Blue: F502N, Green: F656N, Red: F673N

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.

Share

Details

Last Updated
Apr 20, 2026
Contact
Media

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