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Lagoon Nebula (Visible-light View vs. Infrared View)

Lagoon Nebula (Visible-light View vs. Infrared View)

Two Hubble Views of the Same Stellar Nursery

These NASA Hubble Space Telescope images compare two diverse views of the roiling heart of a vast stellar nursery, known as the Lagoon Nebula. The images, one taken in visible and the other in infrared light, celebrate Hubble’s 28th anniversary in space.

The colorful visible-light image at left reveals a fantasy landscape of ridges, cavities, and mountains of gas and dust. This dust-and-gas landscape is being sculpted by powerful ultraviolet radiation and hurricane-like stellar winds unleashed by a monster young star. Located at the center of the photo, the star, known as Herschel 36, is about 200,000 times brighter than our Sun. This hefty star is 32 times more massive and eight times hotter than our Sun. Herschel 36 is still very active because it is young by a star’s standards, only 1 million years old.

The blistering radiation and powerful stellar winds (streams of subatomic particles) are pushing dust away in curtain-like sheets. As the monster star throws off its natal cocoon of material, it is suppressing star formation around it.

However, at the dark edges of this dynamic bubble-shaped ecosystem, stars are forming within dense clouds of gas and dust. Dark, elephant-like “trunks” of material represent dense pieces of the cocoon that are resistant to erosion by the searing ultraviolet light and serve as incubators for fledgling stars.

The star-filled image at right, taken by Hubble in near-infrared light, reveals a very different view of the Lagoon Nebula compared to its visible-light portrait. Making infrared observations of the cosmos allows astronomers to penetrate vast clouds of gas and dust to uncover hidden gems. Hubble’s view offers a sneak peek at the dramatic vistas NASA’s James Webb Space Telescope will provide.

The most obvious difference between Hubble’s infrared and visible photos of this region is the abundance of stars that fill the infrared field of view. Most of them are more distant, background stars located behind the nebula itself. However, some of these pinpricks of light are young stars within the Lagoon Nebula. The giant star Herschel 36, near the center of the frame, shines even brighter in this infrared view.

Dark smudges known as Bok globules mark the thickest parts of the nebula, where dust protects still-forming stars and their planets. While Hubble cannot penetrate these dusty clumps, Webb will be able to see through them.

The Lagoon Nebula resides 4,000 light-years away. The image shows a region of the nebula measuring about 4 light-years across.

The observations were taken by Hubble’s Wide Field Camera 3 between Feb. 12 and Feb. 18, 2018.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    18:03:37.0
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -24:23:12.0
  • 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.
    The nebula is located 4,000 light-years away from Earth.
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is 3.5 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.
    The HST observations include those from program 15449 (M. Mutchler)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS; WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    12-18 February 2018
  • Filters
    FiltersThe camera filters that were used in the science observations.
    UVIS: F502N, F547M, F656N, F658N; IR: F125W, F160W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Lagoon Nebula (Messier 8)
  • Object Description
    Object DescriptionThe type of astronomical object.
    Emission Nebula
  • Release Date
    April 19, 2018
  • Science Release
    Celebrating 28 Years of the Hubble Space Telescope
  • Credits
    NASA, ESA, and STScI

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Lagoon Nebula (Visible-light View vs. Infrared View)
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These images are a composite of separate exposures acquired by the WFC3 instrument on the Hubble Space Telescope. Several filters were used to sample narrow 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: UVIS Blue: F502N Green: F656N Red: F658N Luminosity: F547M IR Cyan: F125W Orange: F160W

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Details

Last Updated
Mar 14, 2025
Contact
Media

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