CosmoView 42: Spanish Dancer Galaxy Twirls into View from NSF’s NOIRLab in Chile. This image, taken by astronomers using the US Department of Energy-fabricated Dark Energy Camera at Cerro Tololo Inter-American Observatory, a Program of NSF’s NOIRLab, captures the galaxy NGC 1566 as it twirls, flinging its arms through the vastness of space. Colloquially nicknamed the Spanish Dancer, this spiral galaxy is often studied by astronomers learning about galaxy groups, stars of different ages, and galactic black holes.
Newswise — Located in the constellation Dorado and lying around 70 million light-years away, NGC 1566 is a grand-design spiral galaxy with two arms that appear to wind around the galactic core, just like the arms of a dancer as they spin around and around in a furious twirl. This image was taken from Chile at the Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, using the Dark Energy Camera. The galaxy's face-on view to us, its location, and its composition make it a trove of observational opportunities for astronomers across many fields of astronomy.
NGC 1566 is home to stars at all stages of stellar evolution. In this image, the bright blue color that outlines the arms of the galaxy arises from young, brightly burning stars. Darker spots within these arms are dust lanes. The arms are rich in gas, and form large-scale areas that provide the perfect environment for new stars to form. Closer to the center of the galaxy are cooler, older stars and dust, all evident by the redder color in the image. This galaxy has even been host to an observed stellar end-of-life event, when a supernova, named SN2010el, burst onto the scene in 2010.
The center of NGC 1566 is dominated by a supermassive black hole. The distinct and highly luminous nucleus of the galaxy is known as an active galactic nucleus. The light from the nucleus changes on timescales of only hundreds of days, making it's exact classification difficult for astronomers.
NGC 1566 is the brightest member, and one of three dominant members, of a collection of galaxies known as the Dorado Group, another member of which is NGC 1515. Galaxy groups are collections of fewer than 50 galaxies, loosely held together by the gravitational pull that each exerts on the others. The Dorado Group consists of at least 46 galaxies. NGC 1566 itself is so dominant that it has its own group, the NGC 1566 Group. The commanding role of NGC 1566 in the Dorado Group has made it a key target for scientists aiming to determine the distance to the group itself, thereby improving our understanding of large-scale structures within the Universe.
The image was taken for the Dark Energy Survey (DES), a project funded by the US Department of Energy (DOE) and National Science Foundation (NSF) which aims to discover the nature of dark energy by mapping millions of galaxies. The Dark Energy Survey is a collaboration of more than 400 scientists from 26 institutions in seven countries. This image was captured using a camera specially designed for the DES: the Dark Energy Camera (DECam). One of the highest-performance, wide-field CCD imagers in the world, DECam was operated by the DOE and NSF between 2013 and 2019. DECam was funded by the DOE and was built and tested at DOE's Fermilab. Currently DECam is used for programs covering a huge range of science.
The galaxy pictured here continues to intrigue astronomers. NGC 1566 and eighteen other nearby galaxies will be observed in infrared light with NASA's James Webb Space Telescope (JWST) by Gemini Observatory's Chief Scientist, NOIRLab astronomer Janice Lee, as part of the PHANGS project. This project will make observations of galaxies that can be seen face-on from Earth, and will take advantage of JWST's ability to see through gas and dust to investigate stars in their earliest stages of formation.
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NSF’s NOIRLab (National Optical-Infrared Astronomy Research Laboratory), the US center for ground-based optical-infrared astronomy, operates the international Gemini Observatory (a facility of NSF, NRC–Canada, ANID–Chile, MCTIC–Brazil, MINCyT–Argentina, and KASI–Republic of Korea), Kitt Peak National Observatory (KPNO), Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), and Vera C. Rubin Observatory (in cooperation with DOE’s SLAC National Accelerator Laboratory). It is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF and is headquartered in Tucson, Arizona. The astronomical community is honored to have the opportunity to conduct astronomical research on Iolkam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawai‘i, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence that these sites have to the Tohono O'odham Nation, to the Native Hawaiian community, and to the local communities in Chile, respectively.
This work is supported in part by the US Department of Energy Office of Science. The Dark Energy Survey is a collaboration of more than 400 scientists from 26 institutions in seven countries. Funding for the DES Projects has been provided by the US Department of Energy Office of Science, US National Science Foundation, Ministry of Science and Education of Spain, Science and Technology Facilities Council of the United Kingdom, Higher Education Funding Council for England, ETH Zurich for Switzerland, National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, Kavli Institute of Cosmological Physics at the University of Chicago, Center for Cosmology and AstroParticle Physics at Ohio State University, Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and Ministério da Ciência e Tecnologia, Deutsche Forschungsgemeinschaft, and the collaborating institutions in the Dark Energy Survey.
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