Galactic ballet captured with state-of-the-art dark energy camera

The interacting pair of galaxies NGC 1512 and NGC 1510 are the focus of this image from the Dark Energy Camera, the 4-m Victor M. There is a state-of-the-art wide-field imager on the Blanco telescope. American Observatory, a program of NSF’s NOIRLab. NGC 1512 has been merging with its younger galactic neighbor for 400 million years, and this ongoing interaction has opened up waves of star formation and distorted both galaxies. credit: Dark Energy Survey/DOE/FNAL/DECAM/CTIO/NoirLab/NSF/Aura, Image processing: TA Rector (University of Alaska Anchorage/NSF NoirLab), J.J. Miller (Gemini Observatory/NSF NoirLab), M. Zamani and D. de Martin (NOIRLab by NSF)

The DOE-funded Dark Energy Camera at NSF’s NOIRLab in Chile captures a pair of galaxies exhibiting a gravitational attraction.

The interacting galaxies pair NGC 1512 and NGC 1510 are the focus of this image from the Dark Energy Camera, a state-of-the-art 570-megapixel wide-field imager built by the US Department of Energy on Victor M Blanco. The 4-meter Telescope at Cerro Tololo Inter-American Observatory, a program of NSF’s NOIRLab. NGC 1512 has been merging with its younger galactic neighbor for 400 million years, and this ongoing interaction has unleashed waves of star formation.

The barred spiral galaxy NGC 1512 (left) and its smaller neighbor NGC 1510 were captured with the 4-meter Victor M. Blanco telescope in this observation (image at the top of the article). This image reveals not only the complex internal structure of NGC 1512, but also the galaxy’s delicate outer tendencies that appear to be protruding and protruding from its smaller companion. The starry stream of light connecting the two galaxies is evidence of the gravitational interaction between them – a majestic and beautiful connection that has lasted for 400 million years. The gravitational interaction of NGC 1512 and NGC 1510 affected the rate of star formation in both galaxies and distorted their shape. Eventually, NGC 1512 and NGC 1510 will merge into one large galaxy – an extended example of galactic evolution.

A large part of the NGC 1512 image. credit: Dark Energy Survey/DOE/FNAL/DECAM/CTIO/NoIRLab/NSF/Aura, Image processing: TA Rector (University of Alaska Anchorage/NSF NoIRLab), Jay Miller (Gemini Observatory/NSF NOIRLab), M. Zamani and D. . de Martin (NSF NOIRLab)

These interacting galaxies are located about 60 million light-years from Earth toward the constellation Horologeum in the Southern Celestial Hemisphere. This wide field of observation reveals not only the interconnected galaxies, but also their starry surroundings. The frame is filled with bright stars in the foreground[{“ 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.

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 established to conduct the Dark Energy Survey (DES), a six-year (2013-2019) observational campaign involving over 400 scientists from 25 institutions in seven countries. This international collaboration aims to map hundreds of millions of galaxies, detect thousands of supernovae and uncover subtle patterns of cosmic structure – all providing much needed details about the mysterious dark energy that is accelerating the expansion of the universe. Today, DECam is still used in programs by scientists around the world and continues its legacy of cutting-edge research.