From: Particle Physics and Astronomy Research Council
Posted: Tuesday, October 2, 2001
A remarkable first light image has been obtained with a new state-of the-art instrument at the Gemini North Telescope on Hawaii's Mauna Kea. The image of the large galaxy in Pisces called NGC 628 (or Messier 74) has been called the "Perfect Spiral Galaxy" due to its nearly ideal form, which is clearly revealed in this new image.
Named GMOS or the Gemini Multi-Object Spectrograph, the instrument that took the image is primarily designed for spectroscopic studies where several hundred simultaneous spectra are required, such as when observing star and galaxy clusters. However, as the dramatic new image demonstrates, GMOS also has the ability to focus beautiful astronomical images on its huge array of almost 24 million ultra-sensitive pixels. When combined with Gemini's 8.1-metre main mirror, the GMOS first-light image of this spiral galaxy leaves no doubt about the instrument's potential on Gemini.
The instrument's first light image of the galaxy that is number 74 in Charles Messier's catalogue of celestial show-pieces (a.k.a. M-74), clearly shows many features of the galaxy such as star clusters, gas clouds and dust lanes. Some of these objects are similar to what we can see in our own Milky Way with the naked eye or small telescope on a clear moonless night. "To be able to routinely see fine details like this in a galaxy more than 30 million light years away is quite remarkable and helps to give some perspective of what our own galaxy might look like if there were another Gemini sized telescope looking back at us!" says Gemini North's Associate Director Dr. Jean-Rene Roy. It is estimated that M-74 is home to about 100 billion stars making it slightly smaller than our Milky Way.
"This instrument took world-class data on its first night, performing perfectly, right out of the box, or at least the 24 crates that brought the 2-ton instrument to Hawaii from Canada and the UK," said Gemini Observatory Director Dr. Matt Mountain. UK Scientists played a key role in designing and building the GMOS instrument during its seven year construction period.
Dr. Mountain added, "This is a considerable testament to the professionalism, planning and teamwork of the multi-national group of astronomers and engineers from the UK's Astronomy Technology Centre, Durham University and the Hertzberg Institute of Astrophysics in Canada who were able to build this instrument and commission it with our staff so successfully here on Mauna Kea. This type of multi-disciplined, multi-national effort represents a new and powerful way to do world-class observational astrophysics," continued Dr. Mountain.
The instrument was built as a joint partnership between Gemini, Canada and the UK at a cost of over ú3 million. Separately, the U.S. National Optical Astronomy Observatory provided the detector subsystem and related software.
Dr Adrian Russell, Director of the UK Astronomy Technology Centre in Edinburgh said: "I am proud of the achievements of everyone who has worked so hard to make this project such a success. The fact that it was commissioned so smoothly is a testament that hard work. The Gemini Partnership now has an immensely powerful scientific tool with which to study the Universe. The best is yet to come."
It is anticipated that GMOS will begin full scientific operations later this year when astronomers from the Gemini partnership, in which the UK has a 25% share, begin using the instrument for a wide variety of scientific studies. "It is extremely exciting to see the wide range of cutting-edge observations already scheduled for GMOS over the next few months," said Gemini Astronomer Dr. Inger Jorgensen who led the instrument's commissioning effort. Dr. Jorgensen also said, "I'm most interested in the planned observations of distant galaxy clusters where Gemini is able to work like a time machine and look back in time to study a much younger universe than we see around us today."
The Dr. Isobel Hook from the UK Gemini Support Group who helped obtain the instrument's first multi-object spectroscopic data said, "The first spectra produced by GMOS were brilliant!
When you combine GMOS with Gemini's resolution and great light gathering power we are able to study details that would otherwise be lost. One area where I think this instrument will excel is in the study of supernova, or exploding stars in very distant galaxies. Once we can obtain spectra from these stars we will be able to better understand the apparent acceleration of the universe."
Professor Roger Davies from Durham University is the leader of the UK's GMOS team. He obtained some early scientific demonstration data that will soon be released to astronomers. For this observation, the light from individual galaxies in a distant, massive swarm of galaxies was collected.
According to Davies, "We were able to observe these galaxies as easily as if they were our close neighbours. Now we'll use this superb spectroscopic data to determine their mass, size and composition and look back in time to see how they have changed through cosmic history. The combination of Gemini's tremendous light collecting power and the technology of GMOS allowed us to obtain phenomenal data only a few days after the instrument was installed on the telescope. I can see that this instrument is going to keep astronomers very busy and extremely happy for a long time!"
Notes for Editors
Peter Barratt - PPARC Press Office
Tel: 01793 442025
Dr Adrian Russell - Director, UKATC
Tel: 0131 668 8100
Professor Roger Davies - University of Durham
Tel: 0191 374 2163
Magnus Paterson - UK Gemini Project Manager
Tel: 0131 668 8100
An image of the spiral galaxy can be downloaded from the PPARC website www.pparc.ac.uk. Photo credit: Gemini Observatory - GMOS team. Alternatively, a high resolution version can be downloaded from www.gemini.edu/project/announcements/press/2001-2.html
Further information and images of GMOS can be found on the following websites:-
Notes to Editors
The Gemini Observatory is an international collaboration that has built two identical 8-meter telescopes. The telescopes are located at Mauna Kea, Hawaii (Gemini North) and Cerro Pach█n in central Chile (Gemini South), and hence provide full coverage of both hemispheres of the sky. Both telescopes incorporate new technologies that allow large, relatively thin mirrors under active control to collect and focus both optical and infrared radiation from space. Gemini North has begun science operations and Gemini South is scheduled to begin scientific operations in late 2001.
The Gemini Observatory provides the astronomical communities in each partner country with state-of-the-art astronomical facilities that allocate observing time in proportion to each country's contribution. In addition to financial support, each country also contributes significant scientific and technical resources. The national research agencies that form the Gemini partnership include: the US National Science Foundation (NSF), the UK Particle Physics and Astronomy Research Council (PPARC), the Canadian National Research Council (NRC), the Chilean Comisi█n Nacional de Investigaci█n Cientifica y Tecnol█gica (CONICYT), the Australian Research Council (ARC), the Argentinean Consejo Nacional de Investigaciones Cient╠ficas y T╚cnicas (CONICET) and the Brazilian Conselho Nacional de Desenvolvimento Cient╠fico e Tecnol█gico (CNPq). The Observatory is managed by the Association of Universities for Research in Astronomy, Inc. (AURA) under a cooperative agreement with the NSF. The NSF also serves as the executive agency for the international partnership.
The Particle Physics and Astronomy Research Council (PPARC) is the UK's strategic science investment agency. It funds research, education and public understanding in four broad areas of science - particle physics, astronomy, cosmology and space science.
PPARC is government funded and provides research grants and studentships to scientists in British universities, gives researchers access to world-class facilities and funds the UK membership of international bodies such as the European Organisation for Nuclear Research, CERN, and the European Space Agency. It also contributes money for the UK telescopes overseas on La Palma, Hawaii, Australia and in Chile, the UK Astronomy Technology Centre at the Royal Observatory, Edinburgh and the MERLIN/VLBI National Facility.
PPARC's Public Understanding of Science and Technology Awards Scheme provides funding to both small local projects and national initiatives aimed at improving public understanding of its areas of science.
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