Serendipitous observations reveal rare event in life of distant quasar

October 21, 2008

A bit of serendipity has given astronomers a surprise view of a never-before-observed event in the birth of a galaxy.

University of Florida and University of California-Santa Cruz astronomers are the first to discover the onset of a huge flow of gas from a quasar, or the super-bright core of an extremely remote young galaxy still being formed. The gas was expelled from the quasar and its enormous black hole sometime in the space of four years around 10 billion years ago – an extremely brief and ancient blip noticed only by a sharp-eyed undergraduate and the unlikely convergence of two separate observational efforts.

"It was completely serendipitous," said Fred Hamann, a UF astronomy professor. "In fact, the only way it could have happened is through serendipity."

A paper about the research appeared online this month in the Letters of the Monthly Notices of the Royal Astronomical Society.

Quasars are enormously bright cores of very distant galaxies thought to contain "super-massive" black holes a billion times larger than our sun. They are seen only in the centers of very distant galaxies that formed long ago — galaxies whose light is just now reaching Earth after billions of years in transit. The quasar in question occurred about 10.3 billion years ago.

The black holes within quasars are invisible, but the cosmic material cascading toward them builds up and forms hot "accretion" disks, the source of quasars' intense light. Some of the incoming material also can be expelled from quasars to form enormous gas clouds that zoom out at extremely high speeds. With the quasar in question, the gas is flowing at an astonishing rate of 58 million mph, Hamann said.

But while astronomers had observed the presence of such gas clouds with other quasars, they had never witnessed one actually coming into being — until now.

Hamann said the discovery was initiated when Kyle Kaplan, an undergraduate at UC-Santa Cruz, earlier this spring noticed peculiarities in the spectra, or wavelengths of light, that had been observed and recorded from the quasar. The spectra were gathered in 2006 as part of an effort to study the galaxies between the quasar and Earth.

UC-Santa Cruz Professor Jason Prochaska was aware of Hamann's work on quasars and asked him to take a look.

When Hamann and other astronomers checked the spectra against the spectra of the same region recorded in a separate sky survey in 2002, they were surprised to discover that there were zero indications of the gas cloud.

"So that's how we know this appeared between 2002 and 2006," he said.

Daniel Progra, a physics professor at the University of Nevada, Las Vegas and an expert on gas outflows from astronomical objects, indicated the discovery is a lucky one.

"I am most excited about this work," he said. "We humans cannot directly monitor changes in quasars as they take very many years. Therefore, a discovery of a change over a few years is very interesting. It is not unexpected, but chances are very small."

He said the discovery supports a computer model he developed that predicts the gas outflows are dynamic and complicated.

Hamann said the discovery also opens a window to understanding more about how quasars come into being.

"The fact that we saw one appear in so short a time frame means that it's a volatile type of structure," he said. "It could be an evolutionary phase, or maybe a transition stage from one phase to another."

It also poses interesting questions about the role of quasars in the formation of galaxies. Astronomers hope future observations will prove telling, Hamann said.

"One interesting question in astronomy is 'how does the evolution of quasars relate to the evolution of galaxies?,'" he said. "The matter ejected from quasars might be the key to this relationship because it can disrupt or regulate the formation of galaxies around quasars. This discovery is a small piece of that story that we can see happening in real time, and what we are going to do now is keep watching."

Source: University of Florida


   
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  • Atomicat - Oct 21, 2008
    • Rank: 3.7 / 5 (3)
    Ummm... just one thing... when the hell did astronomers and cosmologists start measuring things in Miles per Hour??? ARGH!!!
  • Connor - Oct 21, 2008
    • Rank: 5 / 5 (4)
    I think there is a discrepancy in the definition of a black hole...

    A billion times more massive than the sun, not a billion times larger. The entire principal of black holes relies on the mass of the object augmenting the power of the gravitational field surrounding an object to the point where light can not escape.

    Still though, pretty neat article.
  • tkjtkj - Oct 22, 2008
    • Rank: 2 / 5 (4)
    If light originating from
    some event that occurred soon after
    the 'Big Bang' is only now
    reaching us, how come we're here
    first, to greet it? Doesnt our
    presence, then, suggest that we
    must have travelled faster than
    c ?
  • Quantum_Conundrum - Oct 22, 2008
    • Rank: 2 / 5 (4)
    Doesnt our
    presence, then, suggest that we
    must have travelled faster than
    c ?


    Yes and no.

    The Big Bang is a self contradicting paradox.

    They say "evidence" points to a Big Bang, and yet, the evidence does not obey the laws of physics. So then they explain that away by introduction the spontaneously starting and ending "inflationary period" into the model.

    Light moves "through" space at speed c. But according to relativity and the big bang theory, space itself can move. so then the light leaving the quasar might only get "closer" to earth at a net speed of like 0.01c.

    Picture a balloon 1/4 inflated. Put two points on the balloon. Now one person continue blowing the balloon up while another person simultaneously draws a line between the two points at a slow rate. This line represents the path of a photon leaving the quasar.
  • yyz - Oct 22, 2008
    • Rank: not rated yet
    'Emergence of a Quasar Outflow' by F Hamann et al was published Aug. 20, 2008 at arXiv:0808.3998v1 and contains details of high speed (SiIV and CIV absorption lines at 4000 km/s) from the quasar J105400.40 034801.2 at z=2.1!The outflow occured between 2002.18 and 2006.96. For such a distant QSO, this is a most exciting & lucky observation. Outflows from closer QSOs have been observed( see arXiv:0807.0228v1 published July 1, 2008 by N Arav et al on the z=0.868 quasar QSO 2359-1241 as observed by the VLT ). What makes this current QSO so interesting is its' extreme distance & the short specified time of appearance of this high speed outflow, so early in the age of our universe. Further study of this object may answer many questions on what role SMBHs have played in the early formation of galaxies in the distant past. Quite a lucky observation indeed.
  • Lord_jag - Oct 22, 2008
    • Rank: 3.5 / 5 (2)
    no... Travelling away would lead to the wavelength getting shorter, but light will still move at the speed of light. Time will distort so that the light is arriving at the same speed.

    This Quasar didn't originate at the big bang. It happened quite some time later. We both moved a long long way away from each other and then it burst.

    The universe is older than 10 billion years.

October 21, 2008 all stories

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