Exploring the Cosmic Ocean: Water Vapor Around a Feeding Black Hole

In summary, two teams of astronomers have discovered the largest and farthest reservoir of water ever detected in the universe, surrounding a huge, feeding black hole more than 12 billion light-years away. This water, equivalent to 140 trillion times all the water in the world's oceans, is distributed in a gaseous region around the black hole, indicating that the quasar is bathing the gas in X-rays and infrared radiation. The discovery of this water, which is five times hotter and 10 to 100 times denser than typical gas in galaxies, suggests that the black hole may continue to grow in size.
  • #1
JonDE
I have read that it is possible that primordial black holes could have formed in many different sizes, from micro black holes to hundreds of solar masses, my question is this.
What is the smallest black hole that could survive from this time until now, without being destroyed by hawking radiation, and would it be small enough that we could perform experiments on it that we would not be able to perform on the much larger black holes (those above the chandresekhar limit)
 
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  • #2
JonDE said:
I have read that it is possible that primordial black holes could have formed in many different sizes, from micro black holes to hundreds of solar masses, my question is this.
What is the smallest black hole that could survive from this time until now, without being destroyed by hawking radiation, and would it be small enough that we could perform experiments on it that we would not be able to perform on the much larger black holes (those above the chandresekhar limit)

See:

http://library.thinkquest.org/C007571/english/advance/core8.htm

for an elementary treatment. The answer is a bit less than 10^12 kilograms.

Here is peer reviewed reference quoting Hawking at the beginning with a similar figure for minimum mass for a surviving primordial black hole:

http://arxiv.org/abs/0710.3438
 
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  • #3
JonDE said:
I have read that it is possible that primordial black holes could have formed in many different sizes, from micro black holes to hundreds of solar masses, my question is this.
What is the smallest black hole that could survive from this time until now, without being destroyed by hawking radiation, and would it be small enough that we could perform experiments on it that we would not be able to perform on the much larger black holes (those above the chandresekhar limit)
Well, our best bet for detecting these things is through their evaporation. Some people think they may see a teeny tiny signature in current gamma ray bursts that could be primordial black holes, but the evidence looks pretty sketchy to me so far:
http://arxiv.org/abs/1105.5363
 
  • #4
I saw some recent black hole news involving water vapour!

Black hole sucks in 140 trillion times the world's oceans:

http://news.yahoo.com/black-hole-sucks-140-trillion-times-worlds-oceans-163503124.html
 
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  • #5
Tanelorn said:
I saw some recent black hole news involving water vapour!

Black hole sucks in 140 trillion times the world's oceans:

http://news.yahoo.com/black-hole-sucks-140-trillion-times-worlds-oceans-163503124.html

I think I have to go to the bathroom after reading that.
 
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  • #6
Regarding Tanelorn's Yahoo article, I did locate the Jet Propulsion Laboratory's article, Astronomers Find Largest, Most Distant Reservoir of Water, dated July 22, 2011:

Two teams of astronomers have discovered the largest and farthest reservoir of water ever detected in the universe. The water, equivalent to 140 trillion times all the water in the world's ocean, surrounds a huge, feeding black hole, called a quasar, more than 12 billion light-years away.

"The environment around this quasar is very unique in that it's producing this huge mass of water," said Matt Bradford, a scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "It's another demonstration that water is pervasive throughout the universe, even at the very earliest times." Bradford leads one of the teams that made the discovery. His team's research is partially funded by NASA and appears in the Astrophysical Journal Letters.

A quasar is powered by an enormous black hole that steadily consumes a surrounding disk of gas and dust. As it eats, the quasar spews out huge amounts of energy. Both groups of astronomers studied a particular quasar called APM 08279+5255, which harbors a black hole 20 billion times more massive than the sun and produces as much energy as a thousand trillion suns.

Astronomers expected water vapor to be present even in the early, distant universe, but had not detected it this far away before. There's water vapor in the Milky Way, although the total amount is 4,000 times less than in the quasar, because most of the Milky Way's water is frozen in ice.

Water vapor is an important trace gas that reveals the nature of the quasar. In this particular quasar, the water vapor is distributed around the black hole in a gaseous region spanning hundreds of light-years in size (a light-year is about six trillion miles). Its presence indicates that the quasar is bathing the gas in X-rays and infrared radiation, and that the gas is unusually warm and dense by astronomical standards. Although the gas is at a chilly minus 63 degrees Fahrenheit (minus 53 degrees Celsius) and is 300 trillion times less dense than Earth's atmosphere, it's still five times hotter and 10 to 100 times denser than what's typical in galaxies like the Milky Way.

Measurements of the water vapor and of other molecules, such as carbon monoxide, suggest there is enough gas to feed the black hole until it grows to about six times its size. Whether this will happen is not clear, the astronomers say, since some of the gas may end up condensing into stars or might be ejected from the quasar.

Bradford's team made their observations starting in 2008, using an instrument called "Z-Spec" at the California Institute of Technology's Submillimeter Observatory, a 33-foot (10-meter) telescope near the summit of Mauna Kea in Hawaii. Follow-up observations were made with the Combined Array for Research in Millimeter-Wave Astronomy (CARMA), an array of radio dishes in the Inyo Mountains of Southern California.

The second group, led by Dariusz Lis, senior research associate in physics at Caltech and deputy director of the Caltech Submillimeter Observatory, used the Plateau de Bure Interferometer in the French Alps to find water. In 2010, Lis's team serendipitously detected water in APM 8279+5255, observing one spectral signature. Bradford's team was able to get more information about the water, including its enormous mass, because they detected several spectral signatures of the water.

Other authors on the Bradford paper, "The water vapor spectrum of APM 08279+5255," include Hien Nguyen, Jamie Bock, Jonas Zmuidzinas and Bret Naylor of JPL; Alberto Bolatto of the University of Maryland, College Park; Phillip Maloney, Jason Glenn and Julia Kamenetzky of the University of Colorado, Boulder; James Aguirre, Roxana Lupu and Kimberly Scott of the University of Pennsylvania, Philadelphia; Hideo Matsuhara of the Institute of Space and Astronautical Science in Japan; and Eric Murphy of the Carnegie Institute of Science, Pasadena.

Funding for Z-Spec was provided by the National Science Foundation, NASA, the Research Corporation and the partner institutions.

http://www.jpl.nasa.gov/news/news.cfm?release=2011-223

574348main_universe20110722-43_full.jpg

"Quasar Drenched in Water Vapor
This artist's concept illustrates a quasar, or feeding black hole, similar to APM 08279+5255, where astronomers discovered huge amounts of water vapor. Gas and dust likely form a torus around the central black hole, with clouds of charged gas above and below. X-rays emerge from the very central region, while thermal infrared radiation is emitted by dust throughout most of the torus. While this figure shows the quasar's torus approximately edge-on, the torus around APM 08279+5255 is likely positioned face-on from our point of view."
http://www.nasa.gov/topics/universe/features/universe20110722-image.html

It appears that Astrobiology also covered the subject matter:
Galactic Ocean of Water Vapor Encircles a Black Hole
http://www.astrobio.net/pressrelease/4111/galactic-ocean-of-water-vapor-encircles-a-black-hole

Very fascinating information.:smile:
 
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1. What is the size range for black holes?

The size of black holes can vary greatly, from small micro black holes with a diameter of less than a nanometer, to supermassive black holes with diameters of billions of kilometers. The smallest known black hole is less than one mile in diameter, while the largest known black hole is estimated to be over 40 billion kilometers in diameter.

2. Can black holes have sizes in between the smallest and largest known sizes?

Yes, it is possible for black holes to have sizes in between the smallest and largest known sizes. However, due to their gravitational pull, smaller black holes are much harder to detect and study. Scientists are still researching and discovering new black holes of various sizes.

3. How does the size of a black hole affect its properties?

The size of a black hole can greatly affect its properties. Smaller black holes have a stronger gravitational pull and can distort space-time more than larger black holes. Additionally, the size of a black hole can determine how it was formed and what type of radiation it emits.

4. Are there any theories about the maximum size a black hole can reach?

Currently, there is no known maximum size for black holes. Some theories suggest that black holes can continue to grow as they absorb matter and merge with other black holes. However, there are also theories that suggest there may be a limit to how large a black hole can become.

5. Is there a relationship between the size of a black hole and its lifespan?

There is no direct relationship between the size of a black hole and its lifespan. Smaller black holes may evaporate faster due to the emission of Hawking radiation, while larger black holes may have a longer lifespan. However, the lifespan of a black hole is also affected by other factors such as its mass and environment.

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