Wednesday, July 1, 2015

V404 Cygni





This photograph was produced by European Southern Observatory (ESO). (an artist's rendition)


http://finance.yahoo.com/news/nearby-black-hole-just-emitted-220730283.html?soc_src=mediacontentstory&soc_trk=ma

A nearby black hole just erupted for the first time in 26 years and scientists are ecstatic

Business Insider
By Jessica Orwig 

Lurking 8,000 light years from Earth is a black hole 12 times more massive than our sun. It's been peacefully sleeping for 26 years.But on June 15, astronomers detected something signaling that it had woken up.Now, scientists around the world are using highly sophisticated instruments to learn as much as they can about this mysterious beast of nature before the black hole returns to its slumber, which will be soon.Black holes are very dense, massive objects in space that have an immensely powerful gravitational field that traps anything and everything that comes too close, including light. But on occasion they'll spit out material as well as suck it in.On June 15, one of NASA's satellites picked up a torrent of x-rays all coming from a single source: the black hole."Relative to the lifetime of space observatories, these black hole eruptions are quite rare," said Neil Gehrels, the principal investigator for Swift, the NASA satellite that first identified the eruption in a NASA press release. "So when we see one of them flare up, we try to throw everything we have at it, monitoring across the spectrum, from radio waves to gamma rays."

A deadly companion

This black hole is just one half of a two-body system called V404 Cygni. Its partner is a star slightly smaller than our sun, and it's been nourishing the black hole for at least 77 years. The x-rays that astronomers observed on June 15 were the heated guts from the companion star that had spiraled into the mouth of the black hole.When black holes in binary systems, like V404 Cygni, feed, they do so by gravitationally attracting a single thread of gas from the star. The black hole is 12 times more massive than its companion and therefore has a much stronger gravitational grip which slowly pulls gas from the star as the star orbits around it, like in the animation below:.As the gas gets pulled in, it orbits around the black hole, forming a disc. The closer the gas gets to the black hole, the stronger gravitational force it feels and so the faster it moves, heating up to searing-hot temperatures. When the gas reaches temperatures of more than 1.7 million degrees Fahrenheit, it emits a jet of high-energy particles, which satellites like NASA's Swift instrument then detect — albeit 8,000 years later because of the time it takes light to travel from the V404 Cygni to Earth.But there isn't always a steady stream of gas falling into the black hole, which is why it takes such long naps in between feedings.
That disc has two regions: an inner, hot region, and an outer cool region. You need a lot of gas to provide enough pressure and push to cross this barrier, which takes time to generate. Once the black hole has consumed all of the gas in the inner region, which it does in a few days, it has to wait for more. But scientists don't understand the details of how much gas is necessary or exactly how long it takes to build up. That's why this event is so exciting because it gives astronomers a chance to better understand the mechanism that's driving these eruptions. 

A once-in-a-professional-lifetime opportunity

.(European Southern Observatory on Flickr) V404 Cygni's black hole has erupted before.However, when astronomers first saw the outbursts more than 77 years ago, in 1938, they didn't have half of the instruments that are around today. The black hole erupted again in 1956, and then again in 1989. While the eruption of 1989 was studied with a handful of instruments, the outburst wasn't studied in half the detail compared to this year's event.Outbursts like this usually only last for a few weeks to months, so astronomers have culminated a total of nine instruments in space and on the ground to study the black hole in all wavelengths, from very low energy like radio waves to the most energetic like gamma rays, before time runs out.Some of the instruments they're using include the Chandra X-ray Observatory, the European Space Agency's INTEGRAL satellite, Japan's MAXI, and the 10.4-meter Gran Telescope Canarias operated by Spain in the Canary Islands."It is definitely a 'once in a professional lifetime' opportunity," said Erik Kuulkers, the INTEGRAL project scientist in the NASA press release. 

15 comments:

  1. V404 Cygni being a distance of 8000 light years from earth...means that the light we are presently observing from this source was emited 8000 years ago (yes, we are viewing an event wch ocurred 8000 years ago in the past),and has taken 8000 years to traverse the intervening space to finally reach us. 

    8,000 light years = 47,018,804,310,000,000 miles
    =4.7 X 10^16 miles

    ReplyDelete
    Replies
    1. It may help to give some perspective 
      to note that
      it takes light approximately 11.1 hours to travel from one edge of our solar system to the other.(using Pluto's mean distance from the Sun as the radius of the solar system...or 12 billion km).

      Compare that to tbe 8000 years it takes light to travel between V404 Cygni and earth!

      Delete
  2. Trying to wrap my head around this...just hurts my head!

    ReplyDelete
  3. It hurts because a head is a small confining space.
    One has to break out of the shell of one's cranium. ..
    and embrace(become one with) the universe

    ReplyDelete
  4. Previously invisible Black Holes detected by NuStar:

    http://sciconcilium.com/exploring-hidden-supermassive-black-holes/

    ReplyDelete
    Replies
    1. Using gravitational lensing to see previously invisible objects:

      http://www.cnet.com/news/using-the-gravity-of-the-universe-to-peer-into-a-black-hole/

      Delete
    2. Some cool video:

      http://www.popsugar.com/tech/GIF-Two-Merging-Black-Holes-36827039

      Delete
  5. http://m.space.com/29893-supermassive-black-hole-too-big-galaxy.html

    ***********************

    Science 10 July 2015: Vol. 349 no. 6244 pp. 168-171 DOI: 10.1126/science.aaa4506

    An over-massive black hole in a typical star-forming galaxy, 2 billion years after the Big Bang

     Authors

    Black hole out of kilter with theory

    It is believed that black holes and their host galaxies coevolve, with the feedback from the black hole inducing star formation. Such a scenario requires certain timing and mass constraints for the black hole and the star-forming gas. Trakhtenbrot et al. looked at high–red shift galaxies, when the universe was only about 2 billion years old. They found a black hole that developed to maturity much earlier than would be expected and was about 10% of the total galactic mass—much more than expected. Moreover, star formation continued after it would have been expected to stop.Science, this issue p. 168

    Abstract

    Supermassive black holes (SMBHs) and their host galaxies are generally thought to coevolve, so that the SMBH achieves up to about 0.2 to 0.5% of the host galaxy mass in the present day. The radiation emitted from the growing SMBH is expected to affect star formation throughout the host galaxy. The relevance of this scenario at early cosmic epochs is not yet established. We present spectroscopic observations of a galaxy at redshift z = 3.328, which hosts an actively accreting, extremely massive BH, in its final stages of growth. The SMBH mass is roughly one-tenth the mass of the entire host galaxy, suggesting that it has grown much more efficiently than the host, contrary to models of synchronized coevolution. The host galaxy is forming stars at an intense rate, despite the presence of a SMBH-driven gas outflow.

    Received for publication 10 December 2014.
    Accepted for publication 29 May 2015.

    ReplyDelete
  6. Every galaxies has a Black Hole at their center.

     The black hole located in the galaxy CID-947, is among the most massive black holes ever found. It measures nearly 7 billion solar masses (a solar mass is equivalent to the mass of our sun). The black hole at the center of the Milky Way is equivalent to 4 million solar masses...and accounts for 0.5% of its galaxy's mass.
    CID-947's black hole accounts for 10% of its galaxy's total mass.
    This black hole has roughly one-tenth of the mass of its host galaxy.
    This black hole therefore has the entire mass of a typical normal-sized galaxy.


    Over time—billions of years—these black holes continue to expand and grow as they consume more and more of their galaxy's mass. Eventually their growth is halted when they slurp up 100% of their galaxy's mass...at wch point there is no galaxy because only the black hole exists.
    It is impossible to know how many of these solitary black holes are out there...because they are invisible.
    Theory predicts they have a mass equivalent to the mass of a whole galaxy.
    Could this invisible mass account for the elusive "dark matter/energy"?

    ReplyDelete
    Replies
    1. Once it has consumed all the mass within its own galaxy,does it then attract and feed on neighboring galaxies that come within range of its gravitational influence?

      Delete
    2. Yeah,I guess it just sits there dormant and inactive until sometjing comes within range...and then it swallows it up.
      Presumably bigger black holes feed on littler ones until all the mass of the universe is confined within one Mother of a BH!
      ...then what?
      Is that the end...or a new beginning?
      Perhaps when it reaches a critical mass density
      it explodes to form a new universe.

      Delete
    3. Is there a maximum size/mass to a black hole?

      All galaxies eventually collapse into their center.
      Black holes don't just prey on stars;they swallow whole galaxies ...and other black holes!
      When two galaxies collide, the black holes at their centers coalesce(merge onto one).


      The largest black hole in the universe:
      http://youtu.be/xp-8HysWkxw

      The black hole at the center of NGC 1277 consists of  17 billion Solar masses(one solar mass equals
      approx. 2×10^30 kilograms).
      , or a whopping 14% of the stellar mass of the entire galaxy!
       ...and the ultra-distant
      OJ 287 has a black hole of 18 billion solar masses.,
      But these two galaxies still do not
      house the largest black holes in the Universe.


      List of most massive black holes:
      https://en.m.wikipedia.org/wiki/List_of_most_massive_black_holes

      Holmberg 15A. 170,000,000,000 solar masses

      S5 0014+813. 40,000,000,000 solar masses.
      (A 2010 paper suggested that a funnel collimates the radiation around the jet axis, creating an optical illusion of very high brightness, and thus a possible overestimation of the black hole mass.[7]

      SDSS J102325.31+514251.0. 33,100,000,000 solar masses

      Black hole at center of quasar of H1821+643 30,000,000,000 solar masses

      Astronomers in 2014 identified H1821+643 as the most massive black hole with a precisely measured mass, at 30 billion solar masses.[1] 
      Several other black holes are possibly more massive, but they have less accurate mass estimates. The Schwarzschild diameter of this black hole is about 172 billion kilometres, 28 times the diameter of Pluto's orbit.

      https://en.m.wikipedia.org/wiki/H1821%2B643


      The Largest Galaxy in the Universe: IC 1101
      http://youtu.be/UE8yHySiJ4A
      Is it not reasonable to assume that the largest galaxy in the universe would have the largest black hole in the universe at its center?

      Delete
    4. According to the Big Bang theory of creation all the mass/energy of the universe exploded out of a single point source.
      If all that mass were condensed into such a tiny space/volume, it would have been more than sufficient to meet the criteria of a Black Hole....and since nothing can escape a Black Hole because of its immense gravity, the Big Bang event could not have ocurred!
      And if it did happen, that would mean that under certain conditions (e.g. a critical mass density) Black Holes can explode!

      Delete
  7. How is the spin rate of a black hole related to its mass?

    ReplyDelete
  8. compressing mass into Black Holes

    "In order to turn the Sun into a black hole, you must compress all of the matter you see in the flaming ball of plasma into a certain size -- which is called the Schwarzschild’s radius, or Gravitation radius.
    (Extremely simple. You just multiply by two the gravitational constant G (6,674 * 10^-11), then multiply it with the object’s mass divide by the speed of light (299, 792, 458 m/s) squared.)

    The concept of this term is pretty simple: If you compress a given sphere into its Schwarzschild’s radius, the escape velocity from the surface of the sphere would be equal with the speed of light --therefore, forming what we all know as a black hole.
    If you were to compress the Sun into its Schwarzschild’s radius, it will be a ball with a diameter of 3 kilometers.
    And if you try to compress Earth, you’ll have a black hole the diameter of 9mm.

    Now meet S5 0014+81.It’s the largest black hole ever discovered and is heavier than our Sun by 40 billion times (40, 000, 000, 000).If you plug in the equation above, you’ll find that this black hole has a Schwarzschild radius of about… 119 billion kilometers, and a diameter of about 236,39 billion km. S5 0014+81 is 47 times larger in diameter than the distance from Pluto to the Sun"

    The above is from an article in: https://www.yahoo.com/news "Black Holes Are Bigger Than You Thought" Matthew Clifford International Business Times April 23, 2017

    The writer extrapolates backward to calculate the theoretical size of the sun that had to collapse to form
    S5 0014+81...and concludes that sun had to have the diameter of the entire MilkyWay galaxy!
    A sun the size of a galaxy?!
    How large can a sun be?
    How large is tbe largest sun actually observed?

    Of course it is far more reasonable to assume that S5 0014+81 grew to its present massive size by absorbing billions of individual suns the sum of whose masses equals the entire mass of a galaxy.
    In other words, S5 0014+81 has devoured an entire galaxy!

    ReplyDelete