Dark Matter Goes Missing in Oddball Galaxy

Stsci_2018-16a_1024

stsci_2018-16a March 28th, 2018

Credit: NASA, ESA, and P. van Dokkum (Yale University)

Galaxy was expected to contain 400 times more dark matter than observations show

Grand, majestic spiral galaxies like our Milky Way are hard to miss. Astronomers can spot these vast complexes because of their large, glowing centers and their signature winding arms of gas and dust, where thousands of glowing stars reside.

But some galaxies aren't so distinctive. They are big, but they have so few stars for their size that they appear very faint and diffuse. In fact, they are so diffuse that they look like giant cotton balls.

Observations by NASA's Hubble Space Telescope of one such galaxy have turned up an oddity that sets it apart from most other galaxies, even the diffuse-looking ones. It contains little, if any, dark matter, the underlying scaffolding upon which galaxies are built. Dark matter is an invisible substance that makes up the bulk of our universe and the invisible glue that holds visible matter in galaxies — stars and gas — together.

Called NGC 1052-DF2, this "ghostly" galaxy contains at most 1/400th the amount of dark matter that astronomers had expected. How it formed is a complete mystery. The galactic oddball is as large as our Milky Way, but the galaxy had escaped attention because it contains only 1/200th the number of stars as our 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.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2018/news-2018-16

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

Image Details Image Details

Image Type
Observation
Object Name
NGC 1052 DF2
Subject - Local Universe
Galaxy > Type > Irregular

Distance Details Distance

Universescale2
62,000,000 light years
Stsci_2018-16a_128
 

Position Details Position Details

Position (ICRS)
RA = 2h 41m 46.1s
DEC = -8° 24’ 43.4”
Orientation
North is 21.5° CW
Field of View
2.5 x 1.7 arcminutes
Constellation
Cetus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS/WFC) Optical (V) 606.0 nm
Red Hubble (ACS/WFC) Optical (I) 814.0 nm
Spectrum_base
Blue
Red
Stsci_2018-16a_1280
×
ID
2018-16a
Subject Category
C.5.1.6  
Subject Name
NGC 1052 DF2
Credits
NASA, ESA, and P. van Dokkum (Yale University)
Release Date
2018-03-28T00:00:00
Lightyears
62,000,000
Redshift
62,000,000
Reference Url
https://hubblesite.org/contents/news-releases/2018/news-2018-16
Type
Observation
Image Quality
Distance Notes
Facility
Hubble, Hubble
Instrument
ACS/WFC, ACS/WFC
Color Assignment
Blue, Red
Band
Optical, Optical
Bandpass
V, I
Central Wavelength
606, 814
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
40.44203344831, -8.41204329036
Reference Dimension
3000.00, 2000.00
Reference Pixel
1397.60359192714, 301.79356443329
Scale
-0.00001388640, 0.00001388640
Rotation
-21.48214812071
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p1816a-f-3000x2000.tif
Metadata Date
2022-07-06T00:00:00
Metadata Version
1.2
×

 

Detailed color mapping information coming soon...

×
Universescalefull
62,000,000 light years

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