Image of the Week

21 December 2022: We at NSF NOIRLab would like to wish you the best this holiday season, and a peaceful and successful 2023! Check out our animated holiday card here. Happy Holidays, Felices Fiestas and Mele Kalikimaka and Hau‘oli Makahiki Hou!

14 December 2022: A full Moon is arguably the worst time to do any optical astronomy, whether it’s with a backyard telescope or at Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab, near Tucson, Arizona. But the full Moon does make for a spectacular view to the naked eye and in this shot beautifully illuminates the surrounding desert landscape. Taken from the west of KPNO, this image appears to show the Nicholas U. Mayall 4-meter Telescope eclipsing nearly half the diameter of the Moon after moonrise. The Mayall telescope is home to the Dark Energy Spectroscopic Instrument (DESI). DESI, led by the US Department of Energy, is acquiring the spectra of tens of millions of galaxies and quasars to construct a 3D map that will reveal the effects of dark energy in the Universe. This image was taken before the 2022 Contreras Fire, which affected KPNO. Read more here.

7 December 2022: Looking past Earth’s brightly lit atmosphere, incredibly brilliant and colorful celestial objects exist in the vast expanse of space. The Milky Way is the most conspicuous of these nighttime objects, captured here near Cerro Pachón in Chile, home to several facilities operated by NSF NOIRLab, including half of the International Gemini Observatory, the SOAR Telescope and Vera C. Rubin Observatory. The Milky Way’s luminous disk is partially obscured by the interstellar clouds of dust known as the Great Rift. Some of the rift’s dark nebulae fragments appear to stretch into the nearby neighborhood of nebulae. The small grouping of colors is known as the Rho Ophiuchi cloud complex, a dynamic bunch made of reflection nebulae, scattering bright blue and yellow hues from nearby stars, and emission nebulae, diffusing the reddish glow of hot hydrogen gas. Hidden among this interstellar complex are the stars Rho Ophiuchi itself and the ‘heart’ of …

30 November 2022: This Image of the Week shows the lava flows from Mauna Loa caught by one of the International Gemini Observatory’s Cloudcams, which operates 24/7 near the snow-covered summit of Maunakea (the highest point in the image). Mauna Loa, on the island of Hawaiʻi, began erupting on 27 November 2022, when lava emerged from fissures in Moku‘āweoweo, Mauna Loa's caldera at the summit. The reddish glow from the flows can be seen across the island. Mauna Loa is the world's largest active volcano and has not erupted in nearly 40 years. The image was taken in the early morning at 02:15 am local time on 29 November. This eruption is being watched closely by all inhabitants of the island of Hawaiʻi. Staff at Gemini North, operated by NSF NOIRLab, and the other Maunakea Observatories are monitoring with bated breath as the flows move down the flank of Mauna Loa towards the …

23 November 2022: A quartet of interacting galaxies is captured in this observation from Gemini South, which is one of the twin telescopes of the International Gemini Observatory, operated by NSF’s NOIRLab. The four galaxies in this image are collectively known as NGC 6845, and lie roughly 270 million light-years from Earth in a constellation named, appropriately, Telescopium. This constellation is one of a handful named after scientific instruments rather than animals or mythological figures. The galaxies in NGC 6845 come in two varieties: the pair of galaxies at the top of this image are well-defined spiral galaxies whereas the two below them are disk-shaped lenticular galaxies. Connecting the galaxies is evidence of star-forming regions and filaments made of stars detached from their original galaxies. Being relatively close neighbors, the galaxies in NGC 6845 are interacting. These gravitational interactions are subtly distorting the galaxies in NGC 6845, and astronomers believe that the two …

16 November 2022: This still image combines hundreds of time-lapse exposures that capture the entirety of the 8 November 2022 total lunar eclipse above the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory, a Program of NSF’s NOIRLab. Lunar eclipses occur when the Moon passes through the shadow of Earth. During a total lunar eclipse, when the whole Moon enters Earth’s shadow, our natural satellite is drenched in red. The period of totality is evident in this image by the red at the center of the lunar light ‘string.’ The other long streaks of light in the night sky are stars. These star trails form in the camera image as Earth turns. Polaris, the North Star, is the smallest trail in the top right corner of the image. On the ground, an observer drives down the hill, as revealed by the streak of their red tail lights, from the Mayall telescope. …

9 November 2022: Next to the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory, a Program of NSF’s NOIRLab, a total lunar eclipse crawls across the desert sky in the early morning hours of yesterday in this week’s Image of the Week. The Milky Way, dotted by star-forming regions, arches over the telescope (explore in the zoomable image). This year, the typical two annual lunar eclipses were both total, something which hasn’t happened since 2018. You can see the other 2022 total lunar eclipse above Cerro Tololo International Observatory, another Program of NSF’s NOIRLab, in the Image of the Week here and in comparison shots here and a compilation of all 2022 lunar and solar eclipses here. For a total lunar eclipse to occur, the Moon must enter the innermost part of the Earth’s shadow, the umbra. The Moon doesn’t align within the shadow every time it is full, but the …

2 November 2022: Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab, is seen in this daytime aerial panorama of the Arizona-Sonoran Desert on the Tohono O'odham Nation in Arizona. The two largest telescopes, towards the center of the image, are the Nicholas U. Mayall 4-meter Telescope (center) and the UArizona Bok 2.3-meter Telescope (right). The Mayall telescope is currently fitted with the Dark Energy Spectroscopic Instrument (DESI), led by the US Department of Energy. The DESI Survey will measure the effect of dark energy. This mysterious energy is causing the expansion of the Universe to accelerate, instead of being slowed by the effects of gravity as initially expected by researchers before observations of distant objects were possible. By collecting the optical spectra of tens of millions of galaxies and quasars, researchers will use the DESI Survey to construct a 3D map of the nearby Universe and measure its expansion. This image …

26 October 2022: This long-exposure image, taken shortly before sunrise, shows stars appearing to “trail” around the south celestial pole (at the center of the circles) above the Southern Astrophysical Research Telescope (SOAR Telescope). The SOAR Telescope is part of Cerro Tololo Inter-American Observatory, a Program of NSF’s NOIRLab. These trails are caused by the rotation of Earth, which makes stars appear to streak over a long exposure. A few airplanes, shooting stars and satellite trails are also faintly visible. To produce clear, sharp images of stars, planets, and galaxies without the trails seen in this image, astronomical research telescopes like SOAR use sophisticated tracking and guiding systems to precisely follow their targets for hours at a time. Combined with their adaptive optics systems, modern telescopes are able to generate clear images of all types of celestial objects.

19 October 2022: This panorama shows a menagerie of telescopes — including Gemini North (right), one half of the International Gemini Observatory, operated by NSF’s NOIRLab — basking in a glorious snowy sunset near the summit of Maunakea in Hawai‘i. The 8-meter-diameter Gemini North is visible at the right hand edge of this image, and the 3.8-meter-diameter United Kingdom Infrared Telescope is the leftmost telescope in view. Other telescopes are dotted along the ridge in the background, including the Subaru Telescope and the W. M. Keck Observatory. The Maunakea Observatories study phenomena across the electromagnetic spectrum, from radio to ultraviolet, and they all benefit from the dark, dry, still skies at the site. Gemini North — like its twin telescope Gemini South in the southern hemisphere — has silver-coated mirrors optimized for observing at mid-infrared wavelengths. Infrared observations from ground-based observatories are usually limited by water vapor in the atmosphere, which absorbs …

12 October 2022: The constellation Coma Berenices hosts the galaxy NGC 4495 among myriad other astronomical objects. This galaxy has a tumultuous history: several supernovae have been recorded over the years, including the three named 1994S, 2010lo, and 2011ca. This last burst of energy from a dying star can be triggered by a number of different processes. 1994S, for example, was triggered by interactions between a white dwarf and another star, which reignited the core of the stellar remnant — a Type Ia supernova. 2011ca on the other hand is a Type Ic supernova, triggered by the core collapse of a single massive star. This image was captured by the DOE-built Dark Energy Camera (DECam) on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO) as part of the DESI Legacy Imaging Surveys. The DESI Legacy Imaging Surveys were conducted to identify targets for the Dark Energy Spectroscopic Instrument (DESI) …

5 October 2022: The aboveground portion of the McMath-Pierce Solar Telescope at Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab, is seen here at moonrise. The telescope, located about 88 kilometers (55 miles) from Tucson, Arizona, saw its first light in 1962. For much of its life, it was the largest solar telescope on Earth and was notable for its unusual flat mirror, called a heliostat. This mirror tracked the Sun across the sky and continually sent sunlight down into an underground tunnel where the telescope itself was located. This construction helped minimize hot air currents in the light path to the telescope and preserve the quality of the collected data. The McMath-Pierce was also aimed at the Moon, planets, and bright stars for scientific research from time to time. Though decommissioned as a science instrument, the McMath-Pierce Solar Telescope facility is being repurposed as the NOIRLab Windows on the Universe …

28 September 2022: This Image of the Week captures the Milky Way arching over the SOAR Telescope of Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, on Cerro Pachón in Chile. The SOAR (Southern Astrophysical Research) Telescope was initiated by the University of North Carolina at Chapel Hill in the United States. Nineteen years in the making, SOAR saw first light in 2006. Today, the Brazilian and American governments along with two American universities operate and maintain SOAR. Consortiums, like the one for SOAR, allow more astronomers around the world to access state-of-the-art technology while encouraging collaboration between researchers in different countries. To the right, behind SOAR, is Gemini South, one half of the International Gemini Observatory, operated NSF’s NOIRLab. Gemini South is a short walk away — 400 meters (0.25 miles) — from SOAR.

21 September 2022: Gemini North, one the telescopes of the International Gemini Observatory, is pictured against a pastel sky along with three fellow telescopes near the summit of Maunakea in Hawai‘i. Gemini Observatory, which is operated by NSF’s NOIRLab, consists of twin telescopes, one in each of two of the world’s best sites for ground-based astronomy: Gemini North atop Maunakea in Hawai‘i and Gemini South on Cerro Pachón in Chile. The pristine observing conditions at Maunakea mean that Gemini North shares its site with more than a dozen other telescopes. This image shows the silver-clad dome of Gemini North flanked by the Canada-France-Hawaii Telescope and the University of Hawaii 2.2-meter telescope. It can be difficult to grasp the scale of large astronomical observatories, especially against the rugged backdrop of Manuakea’s summit area. If you look closely at the right hand side of this image you can spot the tiny figures of visitors arrayed …

14 September 2022: At Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab located near Tucson, Arizona, it’s unusual to have a cloudy night like this Image of the Week. The high desert climate and mountaintop location make it a great environment for world-class scientific research. The 19 research telescopes on the peak experience over 300 clear nights a year, allowing near year-round observing opportunities. This is great for the many exciting projects at KPNO. For example, the Dark Energy Spectroscopic Instrument (DESI), led by the US Department of Energy, is acquiring the spectra of tens of millions of galaxies and quasars to construct a 3D map that will reveal the effects of dark energy in the Universe. Another instrument, NEID, funded by the joint NASA/NSF Exoplanet Exploration Program, is designed to measure the motion of nearby stars with extreme precision with the WIYN 3.5-meter Telescope. This aerial image was taken before …

7 September 2022: The SMARTS 0.9-meter Telescope at Cerro-Tololo International Observatory (CTIO), a Program of NSF’s NOIRLab, has captured an echo of the past in this gorgeous Image of the Week. RCW 86 is a literal shell of its former self, the gaseous remnant of a supernova. Some 11,000 years ago a white dwarf, itself the core of a former star, became too massive and spectacularly exploded in a Type Ia supernova. Shockwaves reverberated through space, pushing the gas outward, whereupon it formed the multi-layered “bubble” we see today. Besides being a spectacular stellar object, the remnant may have been created by the earliest recorded supernova, observed by Chinese astronomers in 185 AD in the same area between the constellations Circinus and Centaurus.

31 August 2022: The sky over Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, is here densely packed with a brilliant array of curving lines, looking a little like a well-lit wheel that has been sent spinning. In fact, this light streak effect is indeed due to something spinning — Earth! The photographer has used a very long exposure to capture this image, so not only is CTIO visible in sharp detail, but the rotation of Earth on its own axis can be “seen” in the movement of the stars. The center of the circular effect, where the star streaks seem to be rippling out from a point in the upper left of the image, indicates the Earth’s southern geographic pole, i.e., the southern end of the Earth’s axis of rotation.

24 August 2022: Captured from Maunakea, home of Gemini North, one half of the international Gemini Observatory, operated by NSF’s NOIRLab, this Image of the Week features a skyscape of Mauna Loa, the second-highest volcano on the island of Hawai‘i. It seems like a bright, sunny day, but on closer inspection you can see that the sky is actually full of stars, which are most visible toward the center of the image. This means that the photo was actually taken at night, and the blazing ball of light in the upper left is actually the Moon! The image is so incredibly well lit because of the exposure time and camera setting used by the photographer, which allowed the camera to collect so much moonlight that the scene appears to be a bright day.

17 August 2022: The Triangulum Galaxy, otherwise known as Messier 33, lies almost 3 million light-years from Earth, and is a near neighbor of the Andromeda Galaxy. The galaxy is imaged here by the Nicholas U. Mayall 4-meter Telescope, located at Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab. The Triangulum Galaxy is the third-largest member of the Local Group, a cluster of galaxies that includes our Milky Way and its closest neighbors. The Andromeda Galaxy is the largest member. The Triangulum Galaxy and Andromeda Galaxy have history together, but astronomers are still investigating the details. Their close proximity has caused some researchers to suggest that Triangulum is a satellite of the Andromeda Galaxy, not unlike the way the Moon is a satellite of the Earth — just on a much, much bigger scale. Alternatively, some researchers propose that these two galaxies may be independent and have simply brushed past each …

10 August 2022: This Image of the Week shows hulking, smooth, white structures in the sky behind Gemini North, one half of Gemini Observatory, operated by NSF’s NOIRLab, which sits on Maunakea, Hawai‘i. If at first glance you thought the white shapes on the left looked like a flying saucer, then you are not alone. The white oval structures are in fact beautiful examples of lenticular clouds. These clouds most often form over large objects on Earth’s surface, such as the dormant volcano Maunakea, and at high altitudes. Combined with their smooth, saucer-like shape and defined “edge”, lenticular clouds are sometimes mistaken for UFOs.