The control room of the ESO Very Large Telescope at Paranal.
Here, astronomers observe the sky,
using the advanced capabilities
of this high-tech installation
in the Chilean Atacama desert.
With great expertise
scientists and telescope operators
master the VLT controls
and make the difficult observations appear routine.
But suddenly an alarm rings
and calls for their undivided attention.
This is the ESOcast!
Cutting-edge science and life behind the scenes of ESO,
the European Southern Observatory.
Exploring the ultimate frontier with our host Dr J, a.k.a. Dr Joe Liske.
Hello and welcome to the ESOcast.
In this episode we are going to learn about the Very Large Telescope’s
so-called Rapid Response Mode.
The point of this observing mode is to study gamma-ray bursts
only a few short minutes after they are first spotted.
Now because the optical afterglow of a gamma-ray burst fades extremely rapidly,
the observations must start as soon as possible after
the initial discovery of the burst.
And the VLT can deal with such time-critical observations better
than any other telescope.
Gamma-ray bursts are the most powerful explosions in the Universe.
Astronomers do not fully understand their origin,
but they are thought to be caused by incredibly energetic events
such as the collapse of massive stars.
Gamma-ray bursts are so energetic,
that, for a brief instant, they outshine the rest of their entire galaxy.
They produce more energy in a few seconds
than the Sun will in its whole lifetime.
After the flash of gamma-rays has ended,
an optical afterglow can usually be detected for a few hours.
Astronomers look at this to learn more about how and why gamma-ray bursts occur.
Because gamma-ray bursts typically occur at a very large distance from Earth,
their afterglow is faint.
In addition, the afterglow fades very rapidly,
so that within a few hours it can be up to 500 times fainter still.
Hence, in order to learn more about the nature of a gamma-ray burst
and the influence of the explosion on its surroundings,
the event must be observed as quickly as possible.
Now the VLT is perfectly equipped to obtain
high-resolution observations of a gamma-ray burst.
But before it can do so, the burst must first be discovered.
The Swift satellite chases gamma-ray bursts
with its wide-field Burst Alert Telescope.
Once a burst has been discovered and verified,
it is immediately reported to the VLT and other observatories.
An alarm at the VLT console
indicates to the astronomers that the activation
of the Rapid Response Mode has been requested.
The scientists have to confirm that the VLT unit telescope can be moved safely,
and within seconds all on-going observations are stopped.
Then the system performs robotic observations
without any human intervention,
except for the alignment of the spectrograph slit.
This automated procedure guarantees quick and accurate observations.
In fact, the VLT allows astronomers
to begin observations within only a few minutes of detection by Swift.
With events as short-lived as these, this can mean the difference
between making high quality observations and seeing nothing at all.
But the VLT at the Paranal Observatory is not the only ESO facility
which carries out gamma-ray burst observations.
At the La Silla observatory there are also
telescopes that can observe these events.
The 2.2-metre MPG/ESO telescope features
the GROND instrument which takes images of the afterglow
simultaneously in seven different colours.
And that gives astronomers further insights into the physics of gamma-ray bursts.
In addition, there are two smaller telescopes,
the 60-cm REM and the 25-cm TAROT
and these are also located at La Silla.
These robotic telescopes are designed to react
immediately when they receive an alert on a gamma-ray burst,
making it possible to start observing the burst within seconds.
Scientists agree that gamma-ray bursts
are associated with the formation of black holes,
but until now the exact nature of the bursts remains enigmatic
and more high-resolution spectroscopy data is needed.
The VLT offers enormous light collecting power and high resolution.
In addition it is equipped with a suite of high-tech instruments.
It is the combination of the VLT’s enormous observational potential
with ultra fast response times,
which provides data of superb quality
to the scientists who study gamma-ray bursts.
The Rapid Response Mode at the VLT
will be triggered many more times in the future,
and ESO will continue to collect first-class data on gamma-ray bursts
– data which will perhaps one day help to unravel the secrets
of the most energetic explosions in the universe.
This is Dr J signing off for the ESOcast.
Join me again next time for another cosmic adventure.
ESOcast is produced by ESO, the European Southern Observatory.
ESO, the European Southern Observatory, is the pre-eminent intergovernmental science and technology organisation in astronomy
designing, constructing and operating the world’s most advanced ground-based telescopes.
Transcription by ESO ; translation by —
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