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|Pasadena, California – September 4, 2007: Astronomers from the California Institute of Technology and the University of Cambridge have developed a new camera that produces much more detailed pictures of stars and nebulae than even the Hubble Space Telescope, and it does all this from here on|
Until now, images from ground-based telescopes have been invariably blurred by Earth's atmosphere. Astronomers have developed a technique, known as adaptive optics (AO), to correct the blurring, but so far it has only worked successfully in the infrared, where the smearing is greatly reduced. However, a new noise-free, high-speed camera has been developed at the Institute of Astronomy in Cambridge that, when used behind the infrared Palomar Adaptive Optics System, at last makes very high resolution imaging possible in ordinary visible light.
The camera works by recording partially corrected adaptive optics images at high speed (20 frames per second or more). Software then checks each image to sort out which are the sharpest. Many are still significantly smeared by the atmosphere, but a small percentage of
The above image shows the Cat's Eye Nebula (NGC 6543)
seen in visible light using the 200-inch Hale Telescope at Palomar Observatory.
This animated image cycles between the standard visible-light view
which is blurred by Earth's atmosphere and a corrected image using
Palomar's Adaptive Optics System and LuckyCam.
The images of the Cat's Eye Nebula, 20 arcseconds on a side, are are a false-colour combination of three wavelengths of light. The green light is mostly 500nm oxygen emission, red light from H-alpha hydrogen emission and the blue colour represents near-infrared (I-band) light.
Image: Univ. of Cambridge, Caltech
them are unaffected.
These are combined to produce the final high-resolution image that astronomers want.
The technique is called
because it depends on the chance fluctuations in the atmosphere
sorting themselves out and providing a set of images that is easier for the adaptive optics system to correct.
This work was carried out on the 200-inch (5.1 m)
on Palomar Mountain.
Like all other ground-based telescopes,
the images it normally produces are typically 10 times less detailed
than those of the
Hubble Space Telescope.
produces superb images in the infrared,
but until now, its images in visible light have remained markedly poorer than
With the new
Lucky Camera, astronomers
were able to obtain images that are twice as sharp as those produced by the
Hubble Space Telescope –
a remarkable achievement.
The images produced in the study are the sharpest direct images
ever taken in visible light either from the ground or from space.
"The system performed even better than we were expecting.
It was fantastic to watch the first images come in and see that we were easily doing better than
says Nicholas Law, a postdoctoral scholar at
and principal investigator for the instrument.
Most astronomical objects are so far away that astronomers are desperate to see more and more detail within them. The new pictures of the globular star cluster M13, located 25,000 light years away, are sharp enough that astronomers are able to find stars as little as one light-day apart. A light-year is the distance light travels in one year (almost 6 trillion miles). A light-day is the distance light travels in just one day. Stars in the vicinity of the solar system are much farther apart – the nearest star to our solar system is over four light-years away.
The astronomers also observed very fine detail in objects such as the
Cat's Eye Nebula (NGC 6543).
It is eight times closer to earth than M13,
allowing filaments that are only a few light-hours across to be resolved.
The use of the camera at Palomar was a demonstration of the potential of visible-light adaptive optics and offers a glimpse of the detailed imagery to come. Astronomers at Caltech and the Jet Propulsion Laboratory are currently developing the first-ever astronomical adaptive-optics system fully capable of capturing visible-light images. The new system, known as PALM-3000, will routinely allow the 200-inch telescope at Palomar to outperform the Hubble Space Telescope at even blue wavelengths. Using state-of-the-art deformable mirrors, sensors, and a powerful laser, the upgraded Palomar adaptive-optics system will provide finer correction of the atmospheric blurring than any present adaptive optics system, allowing long-exposure images with the same fine detail as the "lucky" images taken recently.
Caltech's Richard Dekany, principal investigator for PALM-3000, says that the upgraded instrument could be available as early as 2010. "These Lucky Imaging results underscore the science potential of diffraction-limited visible-light observations on large ground-based telescopes," he explains.
The above image shows the Globular Cluster M13 imaged by the Palomar 200 inch telescope.
This animated image shows the conventional unsharpened view of the cluster, and the view when imaged with the Lucky Camera behind the adaptive optics system on the Palomar 200 inch telescope.
Image: Univ. of Cambridge, Caltech
To get even sharper pictures, astronomers will need to use bigger telescopes.
The results open up the possibility of further improvements on even larger telescopes,
such as the 10-meter
on the top of Mauna Kea in Hawaii or in the future even larger telescopes,
such as the
Thirty Meter Telescope (TMT).
Working on the Lucky Imaging project were Law, Dekany, Mike Ireland, and Anna Moore from Caltech and the Palomar 200-inch crew. Other team members included Craig Mackay from Cambridge, James Lloyd from Cornell University, and Peter Tuthill, Henry Woodruff, and Gordon Robertson from the University of Sydney.
About the "Lucky Camera" Detector:
This technique has only been possible because of a new kind of CCD camera chip developed by British company, e2v Technologies of Chelmsford. Normally cameras have a residual noise even in the absence of light which greatly limits how faint you can see. This new camera chip is so sensitive that it can detect individual particles of light called photons even when running at high speed. It is this extraordinary sensitivity that makes these detectors so attractive for astronomers. Engineers at Cambridge University have built some of these detectors into their astronomical cameras to make the Lucky Camera work so well.
About the Institute of Astronomy:
The Institute of Astronomy is a Department of the University of Cambridge. It is one of the foremost astronomy departments in the world with an unequalled record of scientific publication. It is the home of the Astronomer Royal, President of the Royal Society and Master of Trinity College, Lord Rees of Ludlow. The work of the Institute covers a wide range of astronomical subjects from the formation of planets and stars and galaxies up to the study of the cosmic microwave background. The Director of the Institute of Astronomy is Professor George Efstathoiu.
About the Palomar Observatory:
The Palomar Observatory is owned and operated by the California Institute of Technology (Caltech). It is located in Southern California about one hour drive from San Diego at an altitude of about 5500 feet (1650 m). The Palomar 200 inch telescope was constructed before and after the Second World War and opened in the late 1940s. For many years it was the largest telescope in the world.
Laser Points to the Future at Palomar, Nov 2004.
Back-Thinned L3Vision CCDs From e2v Set Unprecedented Standards In Low Light Sensitivity, Oct 2003.
Full Press Release: Caltech;
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