Dark galaxy

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A dark galaxy is a hypothesized galaxy with no, or very few, stars. They received their name because they have no visible stars,[1] but may be detectable if they contain significant amounts of gas. Astronomers have long theorized the existence of dark galaxies, but there are no confirmed dark galaxies to date.[2] Dark galaxies are distinct from intergalactic gas clouds caused by galactic tidal interactions, since these gas clouds do not contain dark matter, so they do not technically qualify as galaxies. Distinguishing between intergalactic gas clouds and galaxies is difficult; most candidate dark galaxies turn out to be tidal gas clouds.[3] The best candidate dark galaxies to date include HI1225+01,[4] AGC229385,[5] and numerous gas clouds detected in studies of quasars.

Observational evidence[edit]

Large surveys with sensitive, but low resolution radio telescopes like Arecibo or the Parkes Telescope look for 21 cm emission from atomic hydrogen in galaxies. These surveys are then matched to optical surveys to identify any objects with no optical counterpart, i.e. sources with no stars. However, significant follow-up observations are required to show they have detected a dark galaxy. Astronomers need to demonstrate that the gas is rotating like a galaxy (i.e. that the galaxy has dark matter), and that the galaxy actually doesn't have any stars.

Another way astronomers search for dark galaxies is to look for hydrogen absorption lines in the spectra of background quasars. This technique has revealed many intergalactic clouds of hydrogen, but following up candidate dark galaxies is difficult, since these sources tend to be too far away, and are often optically drowned out by the bright light from the quasar.

Nature of dark galaxy[edit]


In 2000, astronomers found gas cloud VIRGOHI21 and attempted to determine what it was and why it caused such a gravitational pull from galaxy NGC 4254. After years of running out of other explanations, some have concluded that VIRGOHI21 is a dark galaxy, due to the massive effect it had on NGC 4254.[6]


The actual size of dark galaxies is unknown because they cannot be observed with normal telescopes. There have been various estimations, ranging from double the size of the Milky Way[7] to the size of a small quasar.


Dark galaxies are composed of dark matter. Furthermore, dark galaxies are theoretically composed of hydrogen and dust.[6] Some scientists support the idea that dark galaxies may contain stars.[8] Yet the exact composition of dark galaxies is unknown because there is no conclusive way to spot them so far. However, astronomers estimate that the mass of the gas in these galaxies is approximately 1 billion times that of the Sun.[9]

Methodology to observe dark bodies[edit]

Dark galaxies contain no visible stars, and are not visible using optical telescopes. The Arecibo Galaxy Environment Survey (AGES) is a current study using the Arecibo radio telescope to search for dark galaxies, which are predicted to contain detectable amounts of neutral hydrogen. The Arecibo radio telescope is useful where others are not because of its ability to detect the emission from this neutral hydrogen, specifically the 21 cm line.[10]

Alternative theories[edit]

Scientists do not have much explanation for some astronomic events, so some use the idea of a dark galaxy to explain these events. Little is known about dark galaxies, and some scientists believe a dark galaxy is actually a newly forming galaxy. One such candidate is in the Virgo cluster. This candidate contains very few stars. Scientists classify this galaxy as a newly forming galaxy, rather than a dark galaxy.[11] Recently, scientists have made some interesting discoveries. Scientists say that the galaxies we see today only began to create stars after dark galaxies. Based on numerous scientific assertions, dark galaxies played a big role in many of the galaxies astronomers and scientists see today. Martin Haehnel, from Kavli Institute for Cosmology at the University of Cambridge, claims that the precursor to the Milky Way galaxy was actually a much smaller bright galaxy that had merged with dark galaxies nearby to form the Milky Way we currently see. Multiple scientists agree that dark galaxies are building blocks of modern galaxies. Sebastian Cantalupo of the University of California, Santa Cruz, agrees with this theory. He goes on to say, "In our current theory of galaxy formation, we believe that big galaxies form from the merger of smaller galaxies. Dark galaxies bring to big galaxies a lot of gas, which then accelerates star formation in the bigger galaxies." Scientists have specific techniques they use to locate these dark galaxies. These techniques have the capability of teaching us more about other special events that occur in the universe; for instance, the “cosmic web”. This “web” is made of invisible filaments of gas and dark matter believed to permeate the universe, as well as “feeding and building galaxies and galaxy clusters where the filaments intersect.”[9]

Potential dark galaxies[edit]


Main article: HE0450-2958

HE0450-2958 is an unusual quasar (a star like object that may send out radio waves and other forms of energy). This one in particular has many large red shifts.[12] HE0450-2958 has no visible host galaxy (a galaxy surrounding the quasar) detected around it. It has been suggested that this may be a dark galaxy in which a quasar has become active. However subsequent observations revealed that a normal host galaxy is probably present. [13]

HVC 127-41-330[edit]

Main article: HVC 127-41-330

HVC 127-41-330 is a cloud rotating at high speed between the Andromeda and the Triangulum Galaxy. Astronomer Josh Simon considers this cloud to be a dark galaxy because of the speed of its rotation and its predicted mass.[14][15]

Smith's Cloud[edit]

Main article: Smith's Cloud

Smith's Cloud is a candidate to be a dark galaxy, due to its projected mass and survival of encounters with the Milky Way.[16]


Main article: VIRGOHI21

Initially discovered in 2000, VIRGOHI21 was announced in February 2005 as a good candidate to be a true dark galaxy.[8][17][18][19] It was detected in 21-cm surveys, and was suspected to be a possible cosmic partner to the galaxy NGC 4254. This unusual-looking galaxy appears to be one partner in a cosmic collision, and appeared to show dynamics consistent with a dark galaxy (and apparently inconsistent with the predictions of the Modified Newtonian Dynamics (MOND) theory).[20] However, further observations revealed that VIRGOHI21 was the an intergalactic gas cloud, stripped from NGC4254 by a high speed collision.[21][22][23] The high speed interaction was caused by infall into the Virgo cluster.

See also[edit]


  1. ^ "First evidence of dark galaxies from the early Universe spotted". Zmescience.com. 2012-07-11. Retrieved 2012-08-13. 
  2. ^ Cannon, John M.; Martinkus, Charlotte P.; Leisman, Lukas; Haynes, Martha P.; Adams, Elizabeth A. K.; Giovanelli, Riccardo; Hallenbeck, Gregory; Janowiecki, Steven; Jones, Michael (2015-02-01). "The Alfalfa ``Almost Darks Campaign: Pilot VLA HI Observations of Five High Mass-To-Light Ratio Systems". The Astronomical Journal 149: 72. arXiv:1412.3018. Bibcode:2015AJ....149...72C. doi:10.1088/0004-6256/149/2/72. ISSN 0004-6256. 
  3. ^ "Is GBT 1355+5439 a dark galaxy?". www.aanda.org. Retrieved 2015-09-29. 
  4. ^ "The Arecibo Legacy Fast ALFA Survey". egg.astro.cornell.edu. Retrieved 2015-09-29. 
  5. ^ Janowiecki, Steven; Leisman, Lukas; Józsa, Gyula; Salzer, John J.; Haynes, Martha P.; Giovanelli, Riccardo; Rhode, Katherine L.; Cannon, John M.; Adams, Elizabeth A. K. (2015-03-01). "(Almost) Dark HI Sources in the ALFALFA Survey: The Intriguing Case of HI1232+20". The Astrophysical Journal 801: 96. arXiv:1502.01296. Bibcode:2015ApJ...801...96J. doi:10.1088/0004-637X/801/2/96. ISSN 0004-637X. 
  6. ^ a b Fraser Cain (2007-06-14). "No Stars Shine in This Dark Galaxy". Universetoday.com. Retrieved 2012-08-13. 
  7. ^ "Arecibo Survey Produces Dark Galaxy Candidate". Spacedaily.com. 2006-04-07. Retrieved 2012-08-13. 
  8. ^ a b Stuart Clark. "Dark galaxy' continues to puzzle astronomers". New Scientist. Retrieved 2008-02-26. 
  9. ^ a b "First Direct Detection Sheds Light On Dark Galaxies". Zmescience.com. Retrieved 22 December 2012. 
  10. ^ in Astronomy (2009-12-23). "Invisible Dark-Matter Galaxy has Ten Billion Xs the Mass of the Sun". Dailygalaxy.com. Retrieved 2012-08-13. 
  11. ^ "Drexler's Dark Matter Prediction Confirmation Followed His New Book". Newsblaze.com. 2009-11-30. Retrieved 2012-08-13. 
  12. ^ Magain P.; et al. (2005). "Discovery of a bright quasar without a massive host galaxy". Nature 437 (7057): 381–4. arXiv:astro-ph/0509433. Bibcode:2005Natur.437..381M. doi:10.1038/nature04013. PMID 16163349. 
  13. ^ Merritt, David; et al. (2006). "The nature of the HE0450-2958 system". Monthly Notices of the Royal Astronomical Society 367 (4): 1746. arXiv:astro-ph/0511315. Bibcode:2006MNRAS.367.1746M. doi:10.1111/j.1365-2966.2006.10093.x. 
  14. ^ Josh Simon (2005). "Dark Matter in Dwarf Galaxies: Observational Tests of the Cold Dark Matter Paradigm on Small Scales" (PDF). Archived from the original (PDF) on 2006-09-13. 
  15. ^ Battersby, Stephen (2003-10-20). "Astronomers find first 'dark galaxy'". New Scientist. Retrieved December 22, 2012. 
  16. ^ "Dark galaxy crashing into the Milky Way" (2735). New Scientist. 22 November 2009. Retrieved 2009-12-12. 
  17. ^ Clark, Stuart (2005-02-23). "Astronomers claim first 'dark galaxy' find". NewScientist.com news service. Retrieved 2006-10-26. 
  18. ^ Shiga, David (2005-02-26). "Ghostly Galaxy: Massive, dark cloud intrigues scientists". Science News Online (Society for Science &#38) 167 (9): 131. doi:10.2307/4015891. JSTOR 4015891. Retrieved 2008-09-14. 
  19. ^ Britt, Roy (2005-02-23). "First Invisible Galaxy Discovered in Cosmology Breakthrough". Space.com. 
  20. ^ Funkhouser, Scott (2005). "Testing MOND with VirgoHI21". Monthly Notices of the Royal Astronomical Society 364: 237. arXiv:astro-ph/0503104. Bibcode:2005MNRAS.364..237F. doi:10.1111/j.1365-2966.2005.09565.x. 
  21. ^ Kent, Brian R.; Giovanelli, Riccardo; Haynes, Martha P.; Saintonge, Amélie; Stierwalt, Sabrina; Balonek, Thomas; Brosch, Noah; Catinella, Barbara; Koopmann, Rebecca A. (2007-08-01). "Optically Unseen H I Detections toward the Virgo Cluster Detected in the Arecibo Legacy Fast ALFA Survey". The Astrophysical Journal Letters 665: L15–L18. Bibcode:2007ApJ...665L..15K. doi:10.1086/521100. ISSN 0004-637X. 
  22. ^ Duc, Pierre-Alain; Bournaud, Frederic (2008-02-01). "Tidal Debris from High-Velocity Collisions as Fake Dark Galaxies: A Numerical Model of VIRGOHI 21". The Astrophysical Journal 673: 787–797. arXiv:0710.3867. Bibcode:2008ApJ...673..787D. doi:10.1086/524868. ISSN 0004-637X. 
  23. ^ Haynes, Martha P.; Giovanelli, Riccardo; Kent, Brian R. (2007). "NGC 4254: An Act of Harassment Uncovered by the Arecibo Legacy Fast ALFA Survey". Astrophysical Journal 665 (1): L19–22. arXiv:0707.0113. Bibcode:2007ApJ...665L..19H. doi:10.1086/521188. 

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