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IMBH Candidate in Omega Centauri

This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image, middle, zooms in on details of the central region of this cluster, with a closer view of the individual stars. The third image, at right, zooms in further to show the location of the intermediate-mass black hole candidate in the cluster. A dark region is circled and labeled "likely location of black hole." A scale bar about one-sixth the width of the image is labeled "0.1 light-year."

An international team of astronomers has used more than 500 images from NASA's Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole (IMBH) tugging on them. Only a few other IMBH candidates have been found to date.

This image shows the location of the IMBH in Omega Centauri. If confirmed, at its distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, which is 26,000 light-years away. Besides the Galactic center, it would also be the only known case of a number of stars closely bound to a massive black hole.

This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image shows the details of the central region of this cluster, with a closer view of the individual stars. The third image shows the location of the IMBH candidate in the cluster.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    13:26:49.56
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -47:29:32.66
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Centaurus
  • 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.
    17,700  light-years
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is about 9.2 arcminutes across (47 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 programs 9442 (A. Cool), 10252 (J. Anderson), 10775 (A. Sarajedini), 12193 (J. Lee), 13066 (L. Smith), 13606 (J. Anderson), 15594 (V. Kozhurina-Platais), 15764 (N. Hathi), 15857 (A. Bellini), 16380 (M. Chiaberge), 16384 (Y. Cohen), 16520 (N. Hathi), 16968 (N. Hathi), 11452 (J. Quijano), 11011 (C. Kochnek), 12094 (L. Petro), 12339 (E. Sabbi), 12353 (V. Kozhurina-Platais), 12580 (A. Renzini), 12694 (K. Long), 12700 (A. Riess), 12714 (V. Kozhurina-Platais), 12802 (J. MacKenty), 13100 (V. Kozhurina-Platais), 13570 (V. Kozhurina-Platais), 14031 (V. Kozhurina-Platais), 14393 (V. Kozhurina-Platais), 14550 (V. Kozhurina-Platais), 14759 (T. Brown), 15000 (V. Kozhurina-Platais), 15593 (V. Kozhurina-Platais), 15594 (V. Kozhurina-Platais), 15733 (V. Kozhurina-Platais), 15857 (A. Bellini), 16117 (M. Reinhart), 16514 (R. Bohlin), 16441 (J. Anderson), 16588 (V. Kozhurina-Platais), 16777 (A. Seth), and 17023 (C. Martlin).

    This dataset contains HST observations of the globular cluster Omega Centauri out to its half-light radius. The data were selected to contain all available observations with filters suitable for high-precision astrometry (ACS/WFC: F435W, F475W, F555W, F606W, F625W, F775W, F814W; WFC3/UVIS: F336W, F390W, F438W, F555W, F606W, F775W, F814W). In addition, the filters ACS/WFC F658N and WFC3/UVIS F275W were added for photometric purposes as they also cover almost the entire half-light radius. The data were taken in the time spanning from June 2002 to March 2023. They have been collectively compiled here.

  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS, ACS/WFC
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    27 June 2002- 23 Feb 2024
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F275W, F336W, F438W, F606W, F625W, F658N, F814W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Omega Centauri, NGC 5139
  • Object Description
    Object DescriptionThe type of astronomical object.
    Globular cluster
  • Release Date
    July 10, 2024
  • Science Release
    NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri
    Read the release
  • Credit
    ESA/Hubble, NASA, Maximilian Häberle (MPIA)

Downloads

  • Full Res (For Print), 6648 × 2260
    tif (30.17 MB)
  • Full Res (For Display), 6648 × 2260
    png (25.52 MB)
  • 2000 × 680
    png (2.82 MB)
This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image, middle, zooms in on details of the central region of this cluster, with a closer view of the individual stars. The third image, at right, zooms in further to show the location of the intermediate-mass black hole candidate in the cluster. A dark region is circled and labeled "likely location of black hole." A scale bar about one-sixth the width of the image is labeled "0.1 light-year."
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/UVIS instrument on the Hubble Space Telescope. Several filters were used to sample various 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= F275W + F336W + F438W, Green= F606W + F625W, Red= F658N + F814W

Related Images & Videos

An image of the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space.

Omega Centauri

An international team of astronomers has used more than 500 images from NASA's Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri, the largest and brightest...

The central region of a globular cluster is shown, appearing as a collection of myriad stars colored red, white, and blue on the black background of space.

Omega Centauri (cropped)

An international team of astronomers has used more than 500 images from NASA's Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky....

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Details

Last Updated
Mar 28, 2025
Contact
Media

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

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