Suggested Searches

1 min read

NGC 1052-DF2

NGC 1052-DF2

Hubble Views ‘Ghostly’ Galaxy Lacking Dark Matter

This large, fuzzy-looking galaxy is so diffuse that astronomers call it a “see-through” galaxy because they can clearly see distant galaxies behind it.

The ghostly object, catalogued as NGC 1052-DF2, doesn’t have a noticeable central region, or even spiral arms and a disk, typical features of a spiral galaxy. But it doesn’t look like an elliptical galaxy, either. Even its globular clusters are oddballs: they are twice as large as typical stellar groupings seen in other galaxies.

All of these oddities pale in comparison to the weirdest aspect of this galaxy: NGC 1052-DF2 is missing most, if not all, of its dark matter. An invisible substance that makes up the bulk of our universe, dark matter is the underlying scaffolding upon which galaxies are built. It’s the glue that holds the visible matter in galaxies — stars and gas — together.

The galaxy contains at most 1/400th the amount of dark matter that astronomers had expected. But how it formed is a complete mystery.

The galactic oddball is as large as our Milky Way, but it had escaped attention because it contains only 1/200th the number of stars as our galaxy. Given the object’s large size and faint appearance, astronomers classify NGC 1052-DF2 as an ultra-diffuse galaxy.

Based on the colors of its globular clusters, NGC 1052-DF2 is about 10 billion years old. It resides about 65 million light-years away.

The image was taken Nov. 16, 2016, by Hubble’s Advanced Camera for Surveys.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    02:41:46.728
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -08:24:09.871
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Cetus
  • 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 galaxy is 62 million light-years away from Earth.
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    Image is 2.5 arcmin across (about 45,000 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 14644 (P. van Dokkum)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    ACS/WFC
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    16 Nov 2016
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F606W, F814W
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    NGC 1052-DF2
  • Object Description
    Object DescriptionThe type of astronomical object.
    Ultra Diffuse Galaxy
  • Release Date
    March 28, 2018
  • Science Release
    Dark Matter Goes Missing in Oddball Galaxy
  • Credit
    NASA, ESA, and P. van Dokkum (Yale University)

Downloads

  • 1000 × 666
    png (1.2 MB)
  • Full Res, 3000 × 2000
    tif (12.86 MB)
  • Full Res, 3000 × 2000
    png (11.82 MB)
  • 2000 × 1333
    png (5.1 MB)
NGC 1052-DF2
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 ACS/WFC 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: Blue: F606W Red: F814W

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
Mar 14, 2025
Contact
Media

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