GRB 110328A: First ever observation of a newly formed quasar!

Nascent Quasar GRB 110328A

When a formerly quiescent galactic nucleus is observed by astronomers to suddenly begin radiating high energy emission, it is probably natural for them at first to avoid interpreting the sighting as the birth of a quasar and instead propose something on a far smaller less dramatic scale.  Knowing very well the psychology of his astronomer peers, Sir Fred Hoyle forsaw a similar sighting downplay in his science fiction story The Inferno (1973). His story was about astronomers first sighting the explosion of our own galactic nucleus, its sudden activation into the quasar state.  A passage from his book describes how some members on the astronomical discovery team at first wrongly concluded that what they had discovered was a supernova explosion:

“Except this supernova does seem unusually bright,” interjected Tom Cook.
“Has brightened up still more,” announced Bill Gaynor, who had just come in. “Didn’t go to bed. I stayed up till it rose—in the east, about an hour ago.”
“What is it now?”
“I’d say about minus eight.” [25 times brighter than Venus]
There was a whistle around the common room.
“More like a bloody quasar than a supernova,” muttered someone.
A long silence followed this remark. It was broken by Almond. “Which would explain something that’s been worrying the hell out of me.”
“What’s that, Dr. Almond?” Gaynor asked, his eyes red with lack of sleep.
“Why the position of the thing is so precisely the same as the Galactic center. It’s obvious really, isn’t it? The center of the Galaxy has blown up.” Almond’s deep voice was grave as he made this pronouncement.

The Inferno, Sir Fred Hoyle and Geoffrey Hoyle
passage quoted in Earth Under Fire by P. LaViolette

We may be seeing the same sequence of events playing out in real life with the discovery of the source GRB 110328A which may actually prove to be a quasar, the first ever to be seen turning on.  The initial appearance of this X-ray and gamma ray source was first detected by the Swift telescope on March 28, 2011.  It was found to be located at the center of a galaxy in the constellation of Draco situated about 3.8 billion light years away (z = 0.35).

Seeing that the source continued its highly energetic activity even days afterward, astronomers began to realize that what they had been observing was something other than a mere gamma ray burst (GRB).  Most gamma ray bursts, on the other hand, last from a minute or so to several hours at most.  But in seeking an alternate interpretation, astronomers have leaned towards the less dramatic and proposed that we are observing a “supermassive black hole” that is in the process of tidally disrupting and consuming a passing star.

For example, on April 14th, after the source had been active for over two weeks, astronomers Almeida and De Angelis proposed just this in a paper they had submitted for publication to Astronomy and Astrophysics journal.  They propose that we are seeing a black hole having a mass of ~107 solar masses ripping apart and consuming a red giant star of mass 0.5 to 5 solar masses which had happened to orbit too close to it.  They state that if their theory is correct, we should expect that the intense X-ray emission from GRB 110328A to not last more than a few weeks to a few months, i.e., the time taken for the red giant star’s mass to become completely consumed.  In fact in their April 14th paper to Astronomy and Astrophysics, they state that the emission should be seen to begin to fade within a few days to a few months.

Now more than a week has passed since the date they posted their paper, so the predicted lower limit of a “few days” has been well exceeded.  If the source continues its current variable activity after a few months from now, then like Dr. Almond in Hoyle’s novel, astronomers will be forced to consider the inevitable, that what we are seeing is more like a “bloody quasar” than the transitory burp of a black hole!

I predict that GRB 110328A is a quasar and that we just happen to be viewing it at a point in its cycle when it has happened to turn on.  I would prefer not to call it a supermassive black hole as has become customary in astronomy for the reason that I don’t believe in the existence of black holes.  I prefer to use the more neutral term galactic core or alternatively supermassive mother star.  Here are some facts to consider that favor the interpretation that GRB 110328A is a quasar:

1) the X-ray emission is coming from the exact center of the host galaxy, hence from its core.  Similarly, quasars are known to be galactic nuclei in their active state, hence a galactic core observed during its active phase.

2) the average long-term emission coming from GRB 110328A is seen to have an intensity in the range of what is observed to come from a quasar.  That is, quasars typically have X-ray luminosities that range from 1043 to 1048 ergs/s whereas Almeida and De Angelis report that this object has an average X-ray luminosity of about 2.5 X 1047 erg/s.  So GRB 110328A is near the upper end of the quasar luminosity range.

3) Whereas the X-ray luminosity from quasars is observed to erratically vary by many fold over a period of anywhere from hours to weeks, similarly the emission from GRB 110328A has been observed to vary erratically on a timescale of a few hours to a day, very similar to a more rapidly varying quasar.

4) Like a quasar, GRB 110328A emits synchrotron radio emission.  Radio emission from this source was reported on April 11th by Brunthaler et al.

X-ray intensity light curve for source GRB 110328A

X-ray intensity lightcurve for quasar PDS 456.

Considering that we may be observing for the first time the onset of a quasar, there are several interesting things that we can learn from GRB 110328A.
First we can get an idea about the rapidity of the onset of the quasar state.  The observed event occurred without prior warning and reached maximum intensity within 15 minutes.  I have previously stated that we could expect a similar sneak attack from the core of our own Galaxy.  (GRB 110328A instead lies several billion light years away.  So we need not worry about it.)
Second, when it initially turned on, its luminosity was about 20 times greater than the value it attained days later.  At its initial onset it achieved a luminosity of around 5 X 1048 ergs/s in two peak events separated a day apart.  Hence in its first days it would have been one of the most luminous quasars in the sky.  This is very significant.  For it implies that a first strike from our own galactic core may deliver its most deadly effects in the first day or two, with intensities an order of magnitude greater than what we would later be exposed to.

We will keep you updated with more as this story unfolds.  Meanwhile, for those interested about the core explosion phenomenon, click here.  For those who might have doubts that GRB 110328A is an example of a supermassive black hole tidally disrupting a passing star, and who might be interested in learning of an alternative way to conceive of the supermassive objects that form the cores of galaxies, click here.  For evidence that the core of our own Galaxy is most likely not a supermassive black hole, but a mother star, visit our subquantum kinetics forum ( and in particular the posting entitled “Evidence Against Black Hole in Galactic Core“.  Further evidence against the black hole theory is discussed in the books Subquantum Kinetics and Genesis of the Cosmos.

Bookmark the permalink.

One Response to GRB 110328A: First ever observation of a newly formed quasar!

  1. Nick Darby says:

    Has there been any news on this since April 21? Is it still emitting GRBs?

    There seems to be a news blackout on this!

Leave a Reply