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Trifid Nebula (Wide Field Camera 3 Image)

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. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.18:02:23
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-23:01:48
- ConstellationConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.Sagittarius
- 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.5,000 light-years
- DimensionsDimensionsThe 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 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.These images were created with Hubble data from proposal: 18209 (C. Britt).
- InstrumentInstrumentThe science instrument used to produce the data.WFC3/UVIS
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.February 20-22, 2026
- FiltersFiltersThe camera filters that were used in the science observations.F502N (OII), F656N (H-alpha), F673N (SIII)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Trifid Nebula, Messier 20
- Object DescriptionObject DescriptionThe type of astronomical object.Emission Nebula, H II region
- Release DateApril 20, 2026
- Science ReleaseNASA’s Hubble Dazzles With Young Stars in Trifid Nebula
- CreditImage: NASA, ESA, STScI; Image Processing: Joseph DePasquale (STScI)

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

Related Images, Videos, & Articles

Image: Full Trifid Nebula (Rubin Image with Hubble Close-up)
A pullout shows where the Hubble Space Telescope’s close-up image is located within the wider Trifid Nebula. The image at left was taken by the NSF-DOE Vera C. Rubin Observatory in Chile. The color assignments in the images vary based on the filters in the telescopes’ cameras.
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov







