Dark galaxy

A dark galaxy is a hypothetical galaxy composed of dark matter.^[1] Dark galaxies receive their name because they have no detectable stars and are theoretically invisible.^[2] They are not able to generate stars because their density of gas is too low. Some scientists have theorized that dark galaxies were actually common in the early stages of the universe. Originally, these galaxies had trouble creating stars because of their density, but as time progressed galaxies began to create stars.^[3] An influential community of scientists conjecture the existence of dark galaxies to support theories based on other well-studied celestial bodies.^[4] There is experimental evidence^[5] to support the existence of dark galaxies, although scientists have no conclusive evidence and continue their research. Scientists have proposed a means to track down the dark dwarf galaxies that should be orbiting the Milky Way, saying they have now found evidence of one.^[6]

Observational evidence

Astronomers first suspected that there was an invisible dark galaxy upon observing galaxy NGC 4254. This unusual-looking galaxy appears to be one partner in a cosmic collision. The only evidence is the following: gas is being siphoned away into a tenuous stream, and one of its spiral arms is being stretched out. The other partner in this collision is nowhere to be seen. The researchers calculated that an object with a mass of 10¹¹ M_☉ made close passage with NGC 4254 within the last 100 million years creating the gas stream and tearing at one of its arms. This was the clue that an invisible dark matter galaxy might be nearby.^{[citation needed]}

Nature of dark galaxy

W. J. Sidis predicted in 1925 the existence of dark galaxies and that they consist of dark stars. "Our previous consideration on the production of radiant energy from the stars indicates that such production of radiant energy is only possible where the second law of thermodynamics is followed, that is, in a positive section of the universe. In a negative section of the universe the reverse process must take place; namely, space is full of radiant energy, presumably produced in the positive section of space, and the stars use this radiant energy to build up a higher level of heat. All radiant energy in that section of space would tend to be absorbed by the stars, which would thus constitute perfectly black bodies; and very little radiant energy would be produced in that section of space, but would mostly come from beyond the boundary surface. What little radiant energy would be produced in the negative section of space would be pseudo-teleologically directed only towards stars which have enough activity to absorb it, and no radiant energy, or almost none, would actually leave the negative section of space. The peculiarity of the boundary surface between the positive and negative sections of space, then, is, that practically all light that crosses it, crosses it in one direction, namely, from the positive side to the negative side. If we were on the positive side, as seems to be the case, then we could not see beyond such surface, though we might easily have gravitational or other evidence of bodies existing beyond that surface." The Animate and the Inanimate (http://www.sidis.net/ANIM12.htm)

Origin

In 2000 astronomers found a gas cloud VIRGOHI21 and tried to find a theory of what it was and or why it could cause such a gravitational pull from NGC 4254 galaxy. 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.^[1]

Size

The actual size of a dark galaxy is unknown, because they cannot be spotted with a normal telescope. There have been various estimations of the size of dark galaxies. Two potential sizes could be either double the size of the Milky Way^[7] or the size of a small quasar.

Structure

Dark galaxies are composed of dark matter. Furthermore, dark galaxies are theoretically composed of hydrogen and dust.^[1] Some scientists support the idea that dark galaxies may contain stars.^[6] 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.<ref name="^[3]

Methodology to observe dark bodies

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.^[8]

Alternative theories

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 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.^[9] 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.”^[3]

Potential dark galaxies

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.^[10] 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. ^[11]

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.^[12][13]

VIRGOHI21

The discovery of VIRGOHI21 was announced in February 2005, and it was the first good candidate to be a true dark galaxy.^{[4][6][14][15]} It was found when AGES was looking for the 21 cm-wavelength radio waves emitted by hydrogen (H). Its dynamics are apparently inconsistent with the predictions of the Modified Newtonian Dynamics (MOND) theory.^[16] Some researchers have since discounted the possibility of VIRGOHI21 being a dark galaxy and believe it is more likely a "tidal tail"^[17] of nearby galaxy NGC 4254, which is experiencing gravitational perturbations as it enters the Virgo cluster.

See also

References

External links

• Universe Today, Some Galaxies Are Made Almost Entirely of Dark Matter

v t e Dark matter Forms of dark matter Baryonic dark matter Cold dark matter Hot dark matter Light dark matter Mixed dark matter Warm dark matter Self-interacting dark matter Hypothetical particles Axino Axion Chameleon particle Holeum LSP Minicharged particle Neutralino Sterile neutrino SIMP WIMP Theories and objects Cuspy halo problem Dark fluid Dark galaxy Dark matter halo Dark radiation Dark star Dwarf galaxy problem ELKO field Halo mass function Massive compact halo object Mirror matter Navarro–Frenk–White profile Scalar field dark matter Search experiments ADMX AMS-02 ANAIS ArDM ATIC CAST CDMS COUPP CRESST DAMA/LIBRA DAMA/NaI DarkSide DEAP DMTPC DRIFT EDELWEISS EURECA KIMS LUX MOA Multidark OGLE PAMELA PICASSO PVLAS SIMPLE SNOLAB UKDMC WARP XENON ZEPLIN-III Potential dark galaxies HE0450-2958 HVC 127-41-330 Smith's Cloud VIRGOHI21