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Galactic Ballet Photography by Modern Dark Energy Camera

Galactic Ballet Photography by Modern Dark Energy Camera

The DOE-funded dark energy camera at NSF’s NOIRLab in Chile captures some galaxies as they do gravitational binoculars.

The interactive galaxy pair NGC 1512 and NGC 1510 take center stage in this image from the US Department of Energy’s Dark Energy Camera, the latest 570-megapixel wide-angle imaging feature on the Víctor M. Telescope of America, a program of NSF NOIRLab. NGC 1512 merged with its smaller galactic neighbor 400 million years ago, and this prolonged interaction has led to waves of star formation.

Spiral bar galaxy NGC 1512 (left) and its small galaxy NGC 1510 were captured in this observation (photo at the top of the article) by the 4-meter Víctor M. Blanco Telescope. In addition to revealing the complex internal structure of NGC 1512, this image shows the galaxy’s faint outer tendrils extending outward and appearing to surround its small companion. The stream of starlight connecting the two galaxies is evidence of the interaction between the two galaxies – a luxurious and graceful connection that lasted 400 million years. The gravitational interaction between NGC 1512 and NGC 1510 affected the rate of star formation in both galaxies and distorted their shapes. Finally, NGC 1512 and NGC 1510 will merge into a single larger galaxy – a long-standing example of galactic evolution.

Wider crop image NGC 1512. Credit: Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA, Image processing: TA Rector (University of Alaska Anchorage/NSF’s NOIRLab), J. Miller (Gemini Observatory/NSF’s NOIRLab) , M. de Martin (NSF’s NOIRLab)

These interacting galaxies are located in the direction of the constellation Horologium in the southern celestial hemisphere and are located about 60 million light-years from Earth. The wide field of view of this observation shows not only the tangled galaxies, but also their star-rich surroundings. The frame is full of bright stars on the inside from the front[{” attribute=””>Milky Way and is set against a backdrop of even more distant galaxies.

The image was taken with one of the highest-performance wide-field imaging instruments in the world, the Dark Energy Camera (DECam). This instrument is perched atop the Víctor M. Blanco 4-meter Telescope and its vantage point allows it to collect starlight reflected by the telescope’s 4-meter-wide (13-foot-wide) mirror, a massive, aluminum-coated, and precisely shaped piece of glass roughly the weight of a semi truck. After passing through the optical innards of DECam — including a corrective lens nearly a meter (3.3 feet) across — starlight is captured by a grid of 62 charge-coupled devices (CCDs). These CCDs are similar to the sensors found in ordinary digital cameras but are far more sensitive, and allow the instrument to create detailed images of faint astronomical objects such as NGC 1512 and NGC 1510.

Galaxy NGC 1512 Wider

An even wider crop of the NGC 1512 image. Credit: Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA, Image processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), J. Miller (Gemini Observatory/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab)

Large astronomical instruments such as DECam are custom-built masterpieces of optical engineering, requiring enormous effort from astronomers, engineers, and technicians before the first images can be captured. Funded by the US Department of Energy (DOE) with contributions from international partners, DECam was built and tested at DOE’s Fermilab, where scientists and engineers built a “telescope simulator” — a replica of the upper segments of the Víctor M. Blanco 4-meter Telescope — that allowed them to thoroughly test DECam before shipping it to Cerro Tololo in Chile.

DECam was created to conduct the Dark Energy Survey (DES), a six-year (2013-2019) observational campaign involving more than 400 scientists from 25 institutions in seven countries. This international collaboration aims to map hundreds of millions of galaxies, discover thousands of supernovae and discover subtle patterns of cosmic structure – all to provide much-needed detail about the mysterious dark energy that’s accelerating the expansion of the universe. Today, DECam is still used for software by scientists around the world to continue its legacy of cutting-edge science.

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