Top 100 Images

Ranking
Date

1. DECam image of the bulge of the Milky Way

This color-composite shows a main part of the new Blanco DECam Bulge Survey of 250 million stars in our galaxy’s bulge. The 4 x 2 degrees excerpt can be explored in all its whopping 50,000 x 25,000 pixels in this zoomable version.
In the image interstellar dust and gas seemingly acts like a red “filter” in front of the background stars, scattering the blue light away. Since we are surrounded by dust and gas in the Milky Way, this scattering effect is important to many parts of astronomy and is known as interstellar reddening.
DECam was primarily funded by the ...

2. Galactic Dance

Image of the interacting galaxy pair NGC 5394/5 obtained with NSF’s National Optical-Infrared Astronomy Research Laboratory’s Gemini North 8-meter telescope on Hawai’i’s Maunakea using the Gemini Multi-Object Spectrograph in imaging mode. This four-color composite image has a total exposure time of 42 minutes.

3. Gemini South Captures Planetary Nebula CVMP 1

The international Gemini Observatory composite color image of the planetary nebula CVMP 1 imaged by the Gemini Multi-Object Spectrograph on the Gemini South telescope on Cerro Pachón in Chile.

4. Silver Galactic Sliver

The Silver Sliver Galaxy — more formally known as NGC 891 — is shown in this striking image from the Mosaic instrument on the 4-meter Nicholas U. Mayall Telescope at Kitt Peak National Observatory, a Program of NSF’s NOIRLab. NGC 891 is a spiral galaxy that lies almost perfectly edge-on to us, leading to its elongated appearance and its striking resemblance to our home galaxy, the Milky Way, as seen from the Earth. Since NGC 891 is oriented edge-on, it’s great for investigating the galactic fountain model. When stellar winds and supernovae from the disk of a galaxy eject gas ...

5. Jupiter's Red Spots

Gemini North adaptive optics image of Jupiter and its two red spots (which appear white because this is a near-infrared image; in visible light they appear reddish). In this color composite image, white indicates cloud features at relatively high altitudes; blue indicates lower cloud structures; and red represents still deeper cloud features. The two red spots appear more white than red, because their tops hover high above the surrounding clouds. Also prominent is the polar stratospheric haze, which makes Jupiter bright near the pole (unlike the other orange/red features in this image, the polar haze is high in Jupiter's atmosphere). ...

6. A Snowball SOARs

The white dome of the Southern Astrophysical Research (SOAR) Telescope looks a little like a giant snowball, juxtaposed against the icy backdrop. SOAR is an optical telescope, meaning that it observes the skies in the wavelength range that the human eye is sensitive to (and a little beyond). The telescope, however, is equipped with a 4.1-meter mirror, so it can collect a lot more light than human eyes. SOAR is based in Chile at Cerro Pachón. It stands at an altitude of 2,700 meters (8,900 feet) above sea level, which in this winter scene, explains the frosted mountain tops! SOAR ...

7. An Astronomer’s Crystal Ball

The Milky Way appears to be trapped in a crystal ball in this fisheye image taken at the Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab. Thanks to its remote location atop Cerro Tololo in northern Chile, CTIO enjoys a breathtaking panoramic view of the southern hemisphere’s night sky, and a spectacular perspective on the heart of the Milky Way. Though the dusty band of our Milky Way dominates this image, several of CTIO’s telescopes can also be seen along the edges. With more than 20 telescopes operating at the site, CTIO is fully equipped to take advantage ...

8. Rubin Observatory at sunset

This photo of the Rubin Observatory at sunset was taken from behind the nearby Gemini South telescope.

9. Gazing at the Milky Way

The Milky Way spills across the night sky above the Víctor M. Blanco 4-meter Telescope at the Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab. Commissioned in 1974, the telescope was once the largest optical telescope south of the equator and remains an astronomical powerhouse to this day. This photograph captures the open dome of the telescope as it gazes upwards at the luminous band of stars and dust lanes making up our galaxy. Like all telescopes at CTIO, the Blanco benefits from the crystal-clear observing conditions in northern Chile — as you can see from this star-filled ...

10. A Sign of the Zodiac

This image of the Gemini South telescope is so full of light that it is difficult to believe that it was captured at night. Gemini South is the southern half of the international Gemini Observatory, a Program of NSF’s NOIRLab. The wedge-shaped light on the right side of the photo is not from an artificial source (although there are city lights below it), but is a natural phenomenon known as zodiacal light. This occurs when sunlight is scattered off dust particles in the plane of our Solar System, causing part of the sky to become illuminated either after Sun-down or ...

11. A Colorful Night

These whirling lines in the sky are the trails of stars after an hour-long exposure above Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab. The trails are shortest around the North Star, Polaris, a star that happens to coincide almost directly with the celestial north pole. The different colors in the trails reflect the different temperatures of the stars, with blue being the hottest stars and yellow/red the coolest. The telescope visible above the horizon is the Nicholas U. Mayall 4-meter Telescope, and the red glow on the mountain is caused by red lights used to ensure the ...

12. Desert Stars

A shooting star streaks above Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab. Silhouetted against the night sky and the faint glow of Earth’s atmosphere are (from left to right) the Víctor M. Blanco 4-meter Telescope, the SMARTS 1.0-meter Telescope, the former University of Chile telescope, Las Cumbres Observatory 1-meter Telescope, and the KMTNet 1.6-meter Telescope. This image also features scattered boulders and desert plants (left) of Cerro Tololo. Before being purchased in 1967 to create an astronomical observatory, the land upon which CTIO stands supported a handful of subsistence farmers and goat herders. As the site’s old ...

13. Larger than Life

We are so accustomed to skies full of light pollution that this photograph of the Milky Way appears almost unreal in its vividness. It was taken at the site of the KPNO 2.1-meter Telescope of the Kitt Peak National Observatory, a Program of NSF’s NOIRLab. The locations for advanced telescopes are chosen based on several key criteria: the lack of artificial light sources nearby, an arid environment, and clear skies. Not only do these conditions facilitate science-quality telescopic observations, but they make for extraordinary astrophotography.

14. Dazzling in the dark

If you took only a quick glance at this image, you might think that the dark patches occulting the stars were smoke, rising from the ground. In fact this dazzling image — taken on Maunakea, Hawai’i at the northern site of the international Gemini Observatory (right), a program of NSF’s NOIRLab — shows the Milky Way in vivid detail, allowing us to see not only the stars, but the dusty regions which block their light. Tiny flecks mostly inorganic matter make up cosmic dust which in turn forms enormous obscuring clouds. The dark, smoke-like trail through the heart of the ...

15. Heart of the Milky Way

In this time-exposure photo, the center of the Milky Way glows in various colors — an effect invisible to oneʻs eyes — above the Cerro Tololo Inter-American Observatory (CTIO), a program of NSF’s NOIRLab. The heart of our galaxy is best viewed from the southern hemisphere and areas near the equator (such as Hawaiʻi) because of its orientation relative to the Earth. Thanks to its location in the mountains of northern Chile, CTIO makes the southern skies accessible to US astronomers. As well as hosting large research telescopes, CTIO accommodates a variety of smaller tenant observatories. The small domes populating ...

16. A (Galactic) Arm’s Length Away

The two galaxies in this image — NGC 672 (top right) and IC 1727 (bottom left) — appear to be so close that they are almost elbowing each other, like playful children. In fact, the galaxies shown in this beautifully detailed image taken at the Kitt Peak National Observatory, a program of NSF’s NOIRLab, are classified as a galactic pair, and the gravity of each galaxy influences the other. The pair are located around 20 million light-years away from Earth and the space between them spans over 80,000 light-years, a seemingly enormous gap. However, from the perspective of the galaxies’ ...

17. Sunlight Paints a Crimson Sky Over Gemini South

During rare cloudy weather, a vivid red sunset reflects off the dome of the international Gemini Observatory’s Gemini South telescope in Chile, a program of NSF’s NOIRLab. In this image, sunlight is scattered and reflected by gas, dust and particulates in the Earth’s atmosphere and spreads an artist’s palette of red and orange colors across the sky as the Sun sets over Chile’s Pacific coast. Fortunately, the nearby clouds reflecting these colors cleared out in time for the 8.1-meter Gemini primary mirror to collect starlight and complete a productive night of science observations — but not before treating the observatory ...

18. An Insider’s View

Take a peek at the inner workings of a world-class observatory in this image of the international Gemini Observatory, a program of NSF’s NOIRLab. Illuminated by the Moon outside this picture, the open structure of silver beams holding the secondary mirror (center) allows cool night air to pass freely between the mirrors. Combined with the open sides of the dome, the entire design ensures a uniform temperature matching the outside environment. Any variations of temperature create local turbulence that blurs astronomical images. Although this is a picture of the Gemini South telescope in Chile, its twin, the Gemini North telescope ...

19. Radiant Horizons

The stars and dust lanes of the Milky Way hang above telescope domes in this richly hued image of Cerro Tololo Inter-American Observatory (CTIO), a program of NSF’s NOIRLab. The two bright wispy ovals to the right are the Large and Small Magellanic Clouds, dwarf galaxies visible only in the southern hemisphere. The band of color along the horizon is a phenomenon known as airglow, a visible reaction between molecules in the Earth’s atmosphere and solar radiation. In this picture are the Curtis-Schmidt telescope (left), the Victor M. Blanco 4-meter Telescope (middle) and the SMARTS Consortium: 1.5-meter Telescope (right). These ...

20. WIYN Enveloped by Celestial Aura

The glow behind the 3.5-meter WIYN telescope looks like a celestial aura, but it is really a phenomenon known as the Zodiacal Light. This faint glow, created by the scattering of light by small dust particles left over from the formation of our Solar System, is only visible during evening and morning twilight (in the west and east, respectively) and along the plane of the Solar System or the zodiac (hence the name zodiacal light). The WIYN telescope is part of the Kitt Peak National Observatory (KPNO), a program of NSF’s NOIRLab. Also visible is the brilliant light of the ...

21. A Backdrop of Blue and Red

A colorful sunset and layers of blue mountaintops backdrops the Cerro Tololo Inter-American Observatory (CTIO), a program of NSF’s National Optical-Infrared Astronomy Research Laboratory. Most prominent in the image is the 4.0-meter Victor Blanco telescope, which sits atop Cerro Tololo itself. The Cerro Tololo 1.5-meter and 0.9-meter telescopes, as well as a selection of CTIO’s tenant observatories, are scattered along the ridge. This location allows astronomers a stellar view of the southern night sky, providing access to objects not visible from the northern hemisphere, such as the Large and Small Magellanic Clouds and the center of the Milky Way.

22. Milky Way over McMath

The summer Milky Way rises behind the iconic McMath-Pierce Solar Telescope at NSF’s National Optical-Infrared Astronomy Research Laboratory’s Kitt Peak National Observatory. The McMath-Pierce was the largest solar telescope in the world from its dedication in 1962 until it ceased research operations at the end of 2017. The interior of the facility is currently being renovated to become the Windows on the Universe Center for Astronomy Outreach. This new facility will give visitors to Kitt Peak a variety of educational experiences, including a portable planetarium, Science on a Sphere, displays highlighting NSF’s astronomy facilities and an unprecedented look at this ...

23. Purple Sky at Night: Astronomer’s Delight!

This scene shows an arresting purple sky streaked with star trails over Cerro Pachón, the site of the Gemini South telescope (right) and the 4.1 meter Southern Astrophysical Research telescope (SOAR, left), both programs of the NSF’s Optical Infrared Astronomy Research Laboratory. From this mountaintop perch, which lies at an altitude of 2,737 meters (8980 ft) in the Chilean Andes, the 8.1-meter Gemini South telescope can survey the Southern sky — complementing the view from Gemini North atop Maunakea in Hawaiʻi. Together, these astronomical twins can access the entire night sky.

24. Hawai‘i Students Take a Journey Through the Universe!

Over the past week, almost 300 classrooms in the Hilo, Hawai‘i area engaged with local Maunakea observatory staff and other astronomy STEM professionals during the 16th annual Journey Through the Universe program. Here, Scot Kleinman, Gemini’s Associate Director of Development, shares how a coronagraph helps scientists discover exoplanets with second-grade students from Hilo’s E. B. De Silva elementary school. Now in its 16th year, the annual Journey Through the Universe program, led by staff at the international Gemini Observatory, a program of the NSF’s National Optical-Infrared Astronomy Research Laboratory, brings hands-on science demonstrations into K-12 classrooms to inspire the next ...

25. Shooting for the Stars!

Kitt Peak National Observatory, a program of NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab), is located on land leased from the Tohono O’odham Nation. NSF’s NOIRLab staff frequently partner with the American Indian Science and Engineering Students (AISES) chapter at Tohono O’odham Community College to host star-gazing events and other local engagement activities. One popular activity is for students to build and launch water rockets out of two-liter bottles with glow sticks attached to make the flights visible against the dark Arizona skies. This image shows the trajectory of a launch that reaches its apex near the constellation of Orion. ...

26. Trails Near and Far

This long-exposure photograph shows the motion of stars during the night above the Blanco 4-meter telescope (left) and the SMARTS 1.5-meter telescope (right) at Cerro Tololo Inter-American Observatory in Chile, a program of the NSF’s National Optical-Infrared Astronomy Research Laboratory. Also visible in the photo are the trails left by astronomers walking to the Blanco telescope, created by their flashlights. Stars streak through the sky over the course of this one-hour exposure, appearing to spin around the south celestial pole in the upper left of the image. The star closest to the south celestial pole is Sigma Octantis, a relatively ...

27. Circumpolar Laser Tests at Gemini North

As stars appear to circle around the north celestial pole, a new laser at the Gemini North telescope on Hawaii’s Maunakea undergoes rigorous testing, as seen in this image from early October 2019.
The international Gemini Observatory, a program of the National Science Foundation’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab), recently completed testing of a new laser from the company TOPTICA which is a critical component in the telescope’s adaptive optics system. Adaptive optics utilize artificial guide stars, produced by a laser, as a reference when compensating for distortions caused by turbulence in the Earth’s atmosphere. The result is ...

28. Where Discoveries Begin

A young artist adds his touch to the United States National Science Foundation’s (NSF’s) graphic wall at the 235th meeting of the American Astronomical Society in Honolulu, Hawai‘i. This wall, designed by graphic designer Pete Marenfeld, was the center of the NSF Pavilion at the meeting, and encouraged participants to take a break from the meeting and indulge their creative sides — while exploring some of NSF’s world-class observatories which are part of NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab). A time-lapse video shows the fascinating evolution of this wall painting over the duration of the 4-day meeting.
Equipped with ...

29. Starlit Solar Panels at Gemini South

This night-time photo of the Gemini South telescope on Cerro Pachón, Chile features a marvelous view of the Milky Way arching overhead and reflecting off some of the 668 photovoltaic panels that help power the facility. The same clear skies that provide such spectacular views of our galaxy also allow Gemini South, one of two telescopes making up the international Gemini Observatory a program of NSF’s Optical-Infrared Astronomy Research Laboratory, to enjoy abundant sunlight during the day — making solar panels a down-to-earth addition to the facility. Starlight isn’t bright enough to generate electricity at night, when the astronomical observations ...

30. Glowworm Glowing in the Dead of Night

When the weather conditions are just right, glowworms come out at night at Kitt Peak National Observatory. This glowworm crossed the road in front of the WIYN 3.5-meter telescope as the last of the summer Milky Way sets behind the WIYN dome. Although only the tail end of the glowworm is bioluminescent, the glowworm appears as a streak over the 10 second exposure, and the image shows how much distance it covered over the period of the exposure.

31. Storm Lifting Over Gemini

After more than a week of wintery weather, the clouds started lifting over the Gemini North telescope of the international Gemini Observatory (center) on Maunakea. Joy Pollard of NSF’s National Optical-Infrared Astronomy Research Laboratory snapped this shot during a visit to the mountain on 15 January. While snow is not uncommon on the nearly 14,000-foot summit area, this is the first major snowfall this winter on the mountaintop. The snowfall left drifts as high as 2 meters (7 feet) surrounding Gemini North and required the recruitment of staff volunteers to help shovel snow off the dome in order to get ...

32. Sunset at Dawn of Big Data

The Vera C. Rubin Observatory (formerly known as the Large Synoptic Survey Telescope or LSST — see the press release) is featured in this peaceful twilight image. Currently under construction on Cerro Pachón in the Chilean Andes, the Rubin Observatory will produce the Legacy Survey of Space and Time (LSST), a ten-year optical survey of the visible sky that begins in October 2022. The survey will be conducted using the 8.4-meter Simonyi Survey Telescope, which is currently being assembled inside the summit facility, and the 3200-megapixel DOE-funded LSST Camera, which is nearing completion at SLAC National Laboratory. The Rubin Observatory ...

33. Galactic Center Illuminates Cerro Tololo’s Blanco 4-Meter Telescope

The Milky Way arches high over the Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory (CTIO) in Chile. The Blanco 4-meter telescope began operating in 1976, providing astronomers with a world-class observatory in the southern hemisphere, and it continues to produce cutting-edge science. The Blanco is currently equipped with the Dark Energy Camera (DECam), a state-of-the-art 500-megapixel camera which completed the five-year Dark Energy Survey in early 2019. DECam continues with an expanded mission and is providing astronomers with a powerful tool for studying dark energy, exoplanets and more.

34. Sunset over Kitt Peak National Observatory

Every year around the winter solstice, the Sun appears to set behind Kitt Peak National Observatory as seen from Mount Lemmon almost 100 km (60 miles) away. Local photographers meet every year around the holidays to capture photos and videos of this interesting alignment. For a brief time, you can see many of the Kitt Peak telescopes, from the distinctive McMath-Pierce Solar telescope (left) to the large dome of the Mayall 4-meter telescope (right). The still image depicts the silhouettes of the telescopes with a green segment above the Sun and was taken on 17 December 2016. The video was ...

35. Galactic Rainbow

The Milky Way hangs poised over the Gemini South telescope
The colorful band of the Milky Way is poised above the 8.1-meter Gemini South telescope of NSF’s National Optical-Infrared Astronomy Research Laboratory in this arresting image, which depicts bright patches of stars threaded through with winding lanes of dust. The Galactic Center hangs directly above the telescope, framing one of the most powerful astronomical observatories in the southern hemisphere.
The picture also captures the Large and Small Magellanic Clouds, which appear on the left side of the image. These dwarf irregular galaxies are satellites of the Milky Way, and lack ...

36. Convergence Over Cerro Pachón

Jupiter, Venus and the Moon Converge over Observatories
Southern Astrophysical Research (SOAR) Telescope operator Carlos Corco obtained this image of the recent conjunction of Jupiter, Venus and the Moon (right) over the 8-meter Gemini South telescope (left) on Cerro Pachón in Chile. A conjunction is the apparent meeting of two or more celestial bodies in the night sky.
Also visible (in the distance, just right of center) is the silhouette of the Large Synoptic Survey Telescope (LSST) which is currently under construction. In late 2022, LSST is slated to begin an unprecedented, decade-long, survey of the night sky in optical ...

37. Starry Skies at CTIO

Breathtaking observatory panorama showcases the Milky Way
This breathtaking panorama was captured by Hernan Stockebrand, and showcases the pristine skies at the Cerro Tololo Inter-American Observatory (CTIO). CTIO, a program of the NSF’s National Optical-Infrared Astronomy Research Laboratory, is a complex of astronomical telescopes and instruments in the Chilean Andes. CTIO’s mountainous surroundings and altitude — the site is 2200 meters (7200 feet) above sea level — ensure the mountaintop observatory enjoys spectacular night skies. This colorful panorama shows the arch of the Milky Way hanging above the observatory facilities, as well as strands of low clouds illuminated by the ...

38. Starlink Satellites Imaged from CTIO

Earlier this week, while observing with DECam on the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF's NOIRLab, astronomers Clara Martínez-Vázquez and Cliff Johnson noticed something interesting. One of their images, the 333 seconds-exposure seen here, contained at least 19 streaks that they quickly surmised were due to the second batch of Starlink satellites launched last week. The gaps in the satellite tracks are due to the gaps between the DECam CCD chips in the 2.2-degree field.
At the same time, the CTIO all-sky camera recorded the satellites which were even visible with the ...

39. Carina Nebula western wall (with adaptive optics)

A 50-trillion-km (33-trillion-mile, or 5 light-year) long section of the western wall in the Carina Nebula, as observed with adaptive optics on the Gemini South telescope. This mountainous section of the nebula reveals a number of unusual structures including a long series of parallel ridges that could be produced by a magnetic field, a remarkable almost perfectly smooth wave, and fragments that appear to be in the process of being sheared off the cloud by a strong wind. There is also evidence for a jet of material ejected from a newly-formed star. The exquisite detail seen in the image is ...

40. Cerro Tololo Inter-American Observatory from above

Cerro Tololo Inter-American Observatory seen from Cerro Pachón.

41. Through the Camera Lens

Cameras allow us to see things which our eyes cannot! This atmospheric light painting was captured at Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab. The composition is framed by an inky sky and the spectacular arch of the McMath-Pierce Solar Telescope serves as a backdrop. Light painting — where a moving light source is captured with a long camera exposure — has been practiced for well over a century. It has both scientific and artistic applications. NOIRLab’s Colors of Nature Summer Academy explores the science of color and the role color plays in art and nature. Colors ...

42. High resolution solar spectrum

A high resolution version of the spectrum of our Sun, this image was created from a digital atlas observed with the Fourier Transform Spectrometer at the McMath-Pierce Solar Facility at the National Solar Observatory on Kitt Peak, near Tucson, Arizona (‘Solar Flux Atlas from 296 to 1300 nm’ by Robert L. Kurucz, Ingemar Furenlid, James Brault, and Larry Testerman: National Solar Observatory Atlas No. 1, June 1984.). The images shown here were created to mimic an echelle spectrum, with wavelength increasing from left to right along each strip, and from bottom to top. Each of the 50 slices covers 60 ...

43. Whole disk NIRI image sharp

This image showing the entire disk of Jupiter in infrared light was compiled from a mosaic of nine separate pointings observed by the international Gemini Observatory, a program of NSF’s NOIRLab on 29 May 2019. From a “lucky imaging” set of 38 exposures taken at each pointing, the research team selected the sharpest 10%, combining them to image one ninth of Jupiter’s disk. Stacks of exposures at the nine pointings were then combined to make one clear, global view of the planet. Even though it only takes a few seconds for Gemini to create each image in a lucky imaging ...

44. Orion Bullets

Gemini's Laser Vision Reveals Striking New Details in Orion Nebula This composite image at infrared wavelengths was obtained using the Gemini North laser guide star system in conjunction with the ALTAIR adaptive optics system and the NIRI near-infrared imager. The image shows the Orion "bullets" as blue features and represents the light emitted by hot iron (Fe) gas. The light from the wakes, shown in orange, is from excited hydrogen gas.This image brings into focus a remarkably detailed view of supersonic “bullets” of gas and the wakes created as they pierce through clouds of molecular hydrogen in the famous Orion ...

45. Víctor M. Blanco 4-meter Telescope and SMARTS telescopes

CTIO Víctor M. Blanco 4-meter Telescope and SMARTS telescopes.

46. Under the Dome

This image shows an immersive view from inside the dome of the Víctor M. Blanco 4-meter Telescope at the Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab. The rotating dome is an impressive feat of engineering — designed to protect the delicate telescope from the elements. It weighs in at 430 tonnes (475 tons) and was built to withstand Chilean earthquakes. In addition to the Blanco’s dome, this photograph shows some of the equipment needed to run an astronomical observatory, ranging from calibration targets to good old-fashioned ladders! Glimpses of the mountains surrounding CTIO can be seen through ...

47. Glistening Spiral Galaxy

The spiral galaxy NGC 2541 is shown in extravagant detail in this astronomical snapshot from the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory, a Program of NSF’s NOIRLab. Astronomers recognize a variety of galaxy types, and NGC 2541 is classified as an unbarred spiral galaxy. These galaxies possess spectacular spiral arms like the ones shown here, but lack the central bar-shaped structure displayed by galaxies such as the Milky Way. NGC 2541 lies 37 million light-years from Earth in the constellation of Lynx (The Lynx). Sandwiched between the constellations of Ursa Major, Gemini, and Leo, Lynx is ...

48. Cerro Tololo Inter-American Observatory

Cerro Tololo Inter-American Observatory.

49. Take II on an Interstellar Comet

International Gemini Observatory follows a comet from beyond
NOIRLab’s International Gemini Observatory continues tracking a visiting comet from beyond our Solar System. Gemini’s second image release of the comet, discovered by Russian amateur astronomer Gennady Borisov in August of this year, reveals the evolution of the comet as it approaches its closest approach to our sun in December. The image also features the distant background galaxy (going by the catchy designation: 2dFGRS TGN363Z174) that happened to appear adjacent to the comet when the image was captured on the night of November 11–12 2019.
“The comet is doing what we would ...

50. Comet NEOWISE Over Gemini North

Comet NEOWISE — technically known as C/2020 F3 (NEOWISE) — is visible in this spectacular image of the pre-dawn sky to the right (East) of the Gemini North telescope on Maunakea in Hawai‘i, one of the pair of telescopes of the international Gemini Observatory, a Program of NSF’s NOIRLab. First discovered by the NEOWISE project using the Wide-field Infrared Survey Explorer space telescope in March 2020, the comet is a dirty snowball of gas, dust and ice roughly 5 km (3 miles) across. The curving golden tail of C/2020 F3 visible in this image is composed of gas and dust ...

51. Cosmic Fireworks

The spiral galaxy NGC 925 reveals cosmic pyrotechnics in its spiral arms where bursts of star formation are taking place in the red, glowing clouds scattered throughout it.

52. McMath Pierce Solar telescope at night with star trails

A nine-hour exposure of the McMath-Pierce Solar Facility on Kitt Peak. The normally white building appears red due to high altitude haze following the 1991 eruptions of Mount Pinatubo. No filters or multiple exposures were used.

53. Heart of the Crab

In the heart of the Crab Nebula (Messier 1) a neutron star is rotating 30 times every single second. This pirouetting star, known as the Crab Pulsar, consists purely of neutrons, and has an intense magnetic field which ejects jets of material from its poles at nearly the speed of light. The Crab Pulsar has a mass about one and a half times that of our Sun, yet all this mass is packed into a sphere only 28 km (17 miles) in diameter — roughly the size of Mars’s small moon Phobos.
The wispy structures shown in this image are ...

54. Star trails and Víctor M. Blanco 4-meter Telescope

Star trails and Víctor M. Blanco 4-meter Telescope.

55. One Half of a Whole

Pictured here is Gemini South, sitting on the summit of Cerro Pachón in Chile. It is the southern member of the pair of 8.1-meter telescopes, which together comprise the international Gemini Observatory, a Program of NSF's NOIRLab. Gemini North saw its first light in 1999, and — appropriately for twin telescopes — Gemini South followed quickly behind with its first light in 2000. Since then, the united Gemini twins have provided a wealth of scientific observations. In this image, Gemini South is framed by the spectacular Milky Way, which — thanks to the photographic technique used — appears as a ...

56. Cerro Tololo Inter-American Observatory

The Total Solar Eclipse over Cerro Tololo Inter-American Observatory in Chile on 2 July 2019. Photo was taken with a DJI Phantom Pro 3. Clearly visible are the eclipse and the path of totality in the sky.

57. The Sun Gazer

Not all telescopes are nocturnal. This stunning image may look like a piece of abstract art, but it in fact features the iconic McMath-Pierce Solar Telescope, which is stationed at the Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab. Telescopes like the KPNO 2.1-meter telescope seen at the center of the arch operate at night, so that the blazing light of our Sun does not drown out the light from the rest of the sky. However, the McMath-Pierce Solar Telescope took observations day and night before ending operations in 2017. During its years of operation, this telescope observed ...

58. Above the Clouds

This aerial view of the summit area of Maunakea showcases one of the best sites in the world for ground-based astronomy. Against a backdrop of snow and dark volcanic rock, the domes of the Maunakea Observatories harbor some of the world’s most advanced astronomical equipment. These telescopes, including the 8.1-meter Gemini North (the open silver dome on the higher ridge), utilize the high elevation, dark skies, and good weather to observe the Universe in astounding clarity. Despite the occasional snowfall, the air at the summit of Maunakea is extremely dry, making the site perfect for infrared observations — as well ...

59. Galactic Waterfall

The Milky Way resembles a waterfall rushing down the colorful night sky above Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab. The green-tinged light on the horizon is airglow, originating from the naturally occurring gases in Earth’s atmosphere. Airglow is present at all latitudes but is incredibly dim at visible wavelengths, making it difficult to spot with the naked eye but vivid and bright with long exposure photography. While the horizon softly glows with light, the skies above the telescopes remain awash with stars.

60. Fireball over KPNO

Last week, on the night of Thursday 17 September 2020 10:52 pm, a very bright meteor was reported by more than 25 eyewitnesses in and around Tucson and Phoenix, Arizona. The phenomenon, also known as a fireball or bolide, was also spotted by one of the robotic cameras at Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab: an all-sky camera operated by the University of Arizona’s Spacewatch who operates the Spacewatch 0.9-meter Telescope and the Spacewatch 1.8-meter Telescope (seen in the image as the white dome near the top of the image respectively on the left). The image ...

61. Sky Aglow at CTIO

The glowing light suffusing the night sky in this photograph is due to two fascinating effects — zodiacal light and airglow. The first effect, zodiacal light, is due to sunlight scattered by interplanetary dust in our Solar System, and causes the dim white vertical gleam dominating the left hand side of this image. Airglow, on the other hand, originates in Earth’s own atmosphere. It is visible as bands of colored light along the horizon to the right of the Víctor M. Blanco 4-meter Telescope of Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab.

62. Moonlit Heliostat

The full Moon rises behind the heliostat of the McMath-Pierce Solar Telescope at Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab. The heliostat has a 2.03-meter (80-inch) mirror that reflects sunlight into the optical path of the telescope. The McMath-Pierce Solar Telescope was the largest solar telescope in the world upon its completion in 1962, a title it held until the first light of the National Solar Observatory’s Daniel K. Inouye Solar Telescope in December 2019. The interior of the McMath-Pierce Solar Telescope is currently being renovated to become the Windows on the Universe Center for Astronomy Outreach.

63. Follow the Yellow Lit Road

Momentarily lit by the lights of a passing vehicle, this road leads to Gemini North, perched near the summit of Maunakea on Hawaiʻi Island. It is the northern member of the twin Gemini telescopes, which together comprise the international Gemini Observatory, a Program of NSF's NOIRLab. There are no artificial lights present at the summit. However, the occasional wandering visitor will illuminate the domes with their headlights while in search of the world-famous views of Maunakea’s dark skies.

64. A Lonely Spiral in a Tapestry of Galaxies

This stunning image features NGC 3198, a galaxy that lies about 47 million light-years away in the constellation Ursa Major. This image was taken with the Mosaic instrument on the 4-meter Nicholas U. Mayall Telescope at Kitt Peak National Observatory, a Program of NSF’s NOIRLab, and shows the full extent of the galaxy, from the bright central bulge to the tenuous outer reaches of the tightly-wound spiral arms. Almost all the objects lurking in the background are galaxies or galaxy clusters — a sea of distant galaxies of all shapes, sizes, and orientations.
Accurately measuring the distance to an astronomical ...

65. Artist’s impression of a brown dwarf orbiting a white dwarf

Artist’s impression of one of this study’s superlative discoveries, the oldest known wide-separation white dwarf plus cold brown dwarf pair. The small white orb represents the white dwarf (the remnant of a long-dead Sun-like star), while the brown/orange foreground object is the newly discovered brown dwarf companion. This faint brown dwarf was previously overlooked until it was spotted by citizen scientists, because it lies right within the plane of the Milky Way.

66. Trails Through the Night Sky

Although this appears to be a daytime scene, star trails circle and illuminate the night sky in this long-exposure photo of Kitt Peak National Observatory (KPNO), a Program of NSF’s NOIRLab. The telescope visible at the highest peak is the Nicholas U. Mayall 4-meter Telescope and almost directly above it, at the center of the concentric star trails, sits the North Star, Polaris. As the Earth turns and the stars appear to move through the sky, Polaris remains stationary at the north celestial pole, our planet’s axis of rotation. The lights of Tucson, Arizona, glow yellow on the horizon about ...

67. Cerro Tololo Inter-American Observatory

Cerro Tololo Inter-American Observatory, Chile.

68. Artist’s interpretation of the calcium-rich supernova 2019ehk

Artist’s interpretation (without labels) of the calcium-rich supernova 2019ehk. Shown in orange is the calcium-rich material created in the explosion. Purple coloring represents gas shed by the star right before the explosion, which then produced bright X-ray emission when the material collided with the supernova shockwave.

69. Maunakea and Mauna Loa

Aerial view of Maunakea in the midground, and Maunaloa in the background. The ocean and shore of the Hawai‘i island make up the foreground.

70. Striking image shows mass distribution of nearby galaxy cluster

Using the Dark Energy Camera at Cerro Tololo Inter-American Observatory, a Program of NSF’s NOIRLab, astronomers are measuring weak gravitational lensing to map the distribution of mass in nearby galaxy clusters. As well as producing remarkable images like this one, the information will shed light on the relationships between the constituent parts of nearby galaxy clusters, such as gas, stellar populations, and dark matter.
The galaxy cluster Abell 3827 is the subject of this striking image. In addition to featuring a field of galaxies and foreground stars, the image is overlaid with a map with hues of red, blue and ...

This picture compares the spectra of different classifications of star, in the visual range from 400 to 700 nanometers (4000 to 7000 Angstroms). Thirteen regular types are shown, and at the bottom are three special cases, all selected from the spectrophotometric atlas by Jacoby, Hunter and Christian, 1984, which used data from the Kitt Peak National Observatory's 0.9-meter telescope. From top to bottom, the stars and their type are: HD12993, O6.5; HD158659, B0; HD30584, B6; HD116608, A1; HD9547, A5; HD10032, F0; BD 61 0367, F5; HD28099, G0; HD70178, G5; HD23524, K0; SAO76803, K5; HD260655, M0; and YALE 1755, M5. The ...

72. M45 Pleiades

This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9-meter telescope on Kitt Peak, Arizona. The Pleiades are an open cluster easily visible to the naked eye. The cluster is dominated by several hot, luminous and massive stars. The blue nebulosity surrounding the brightest stars are due to blue light from the stars scattering off of dust grains in the interstellar gas between us and the stars. The cluster is also known as the 'Seven Sisters'. And in Japan it is called Subaru. The image was generated with observations in the B (blue), V ...

73. Reflection Nebula NGC 1788

This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. NGC 1788 is an unusual reflection nebula (bluish white at the center of the image) surrounded by a glowing red ring of hydrogen gas. The stars inside the nebula are only about a million years old, which is very young compared to most stars. The ring of glowing hydrogen gas is energized by nearby hot, massive stars not visible in the image. The image was generated with observations in the B (blue), I (orange) and Hydrogen-Alpha (red) filters. ...

74. Planetary Nebula HFG1

This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. HFG1 is a planetary nebula in the constellation of Cassiopeia. It was produced by a binary star system (V664 Cas) that is moving rapidly through our Galaxy. The star is moving towards the upper-right of the image. As HFG1 plows through the interstellar medium, a bluish bowshock is produced; and a red trail of gas is left behind in its wake. The image was generated with observations in the Hydrogen alpha (red) and Oxygen [OIII] (blue) filters. In ...

75. Carina Nebula (NGC 3372)

This image shows a giant star-forming region in the southern sky known as the Carina Nebula (NGC3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulfur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright star near the center of the image is Eta Carinae, which is one of the most massive and luminous stars known. This ...

76. Star-Birth “Fireworks”

This Gemini North telescope image reveals no less than six gas jets emerging at supersonic speeds from the reddish Herbig-Haro 24 (HH 24) complex — a small cluster of young stars embedded in a molecular cloud some 1,300 light years distant in the constellation Orion. It is the most detailed image ever obtained from the ground of this remarkable region, which contains the highest concentration of jets known anywhere. One jet is highly disturbed, suggesting that the source may be a close binary whose orbit perturbs the jet body. This dynamic environment also may be responsible for expelling some of ...

77. Rich Young Cluster Cep OB 3b

Cep OB 3b is rich young cluster located in the northern constellation of Cepheus. This image was created by combining individual images observed through four different filters on the 0.9 meter telescope at Kitt Peak: blue, visual (cyan), near infrared (orange) and an emission line of hydrogen (red). The brightest yellow star near the center of the image is a foreground star, lying between us and the young cluster. The other bright stars are the massive young stars of the cluster that are heating the gas and dust in the cloud and blowing out cavities. Surrounding these massive cluster stars ...

78. Soap Bubble Nebula, PN G75.5+1.7

Informally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G75.5+1.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17th, 2008. This image was obtained with the Kitt Peak Mayall 4-meter telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters. In this image, north is to the left and east is down. PN G75.5+1.7 is located in the constellation of Cygnus, not far from the Crescent Nebula (NGC 6888). It is embedded in a diffuse ...

79. The Starry Dandelion and the Cosmic Gecko NGC 6520

Millions of years ago, a dust cloud about 5,200 light-years from the Sun coalesced to begin the process of star birth. Today, some 190 million years later, NGC 6520 is ablaze with hot, massive young stars arrayed in a dandelion seed-shaped cluster. Not far away lies the gecko-shaped remains of what may be their birth cloud, Barnard 86. This image, taken using the Gemini Multi-Object Spectrograph on Gemini South, shows details in a 9.7- x 5.4-arcmin section of a larger, highly populated region in the Sagittarius star cloud. It provides the clearest optical view of the cluster and its nearby ...

80. Nebula NGC 6164-5

NGC 6164-5 imaged at Gemini South. The emission nebula NGC 6164-5 is a rectangular, bipolar cloud with rounded corners and a diagonal bar producing an inverted S-shaped appearance. It lies about 1,300 parsecs (4,200 light-years) away in the constellation Norma. The nebula measures about 1.3 parsecs (4.2 light-years) across, and contains gases ejected by the star HD 148937 at its heart. This star is 40 times more massive than the Sun, and at about three to four million years of age, is past the middle of its life span. Stars this massive usually live to be only about six million ...

81. The Helix Nebula, NGC 7293

This composite picture is a seamless blend of nine ultra-sharp images from the Hubble Space Telescope’s Advanced Camera for Surveys with the wide-field view of the Mosaic Camera on the WIYN 0.9-meter telescope at Kitt Peak National Observatory. The image shows a fine web of filamentary “bicycle-spoke” features embedded in the colorful red and blue gas ring, which is one of the nearest planetary nebulae to Earth. One of the largest and most detailed celestial images ever made, the picture was released on May 9, 2003, by the Space Telescope Science Institute and NOAO in honor of Astronomy Day 2003, ...

82. Maunakea - Aerial

Aerial view of the summit of Maunakea.

83. vdB 152, Barnard 175

This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. Also known as Barnard 175, vdB 152 is a reflection nebula atop of a dark Bok globule. Embedded in the top right side of the nebula is the Herbig Haro object HH 450, a jet emitted from a newly forming star. The thin, red filaments in the upper-right corner of the image are the remnants of a supernova explosion. It is not yet clear whether or not the supernova remnant will collide with vdB 152. The image was ...

84. The Veil Nebula, NGC 6960

This image of the Veil Nebula was taken with the Mosaic camera on the WIYN 0.9-meter telescope at Kitt Peak National Observatory. The Veil Nebula (NGC6960) is part of a supernova remnant known as the Cygnus Loop. It is the shattered remains of one, and possibly two, supernovae that exploded more than 15,000 years ago at a distance of 2,500 light-years from Earth in the direction of the constellation of Cygnus, the Swan. At the time of the explosion, it would have been seen as a very bright star, rivaling the crescent Moon. The bright star near the center of ...

85. Panorama of Spiral Galaxy, M31

This image was created with data from the Local Group Survey, completed with the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. M31, M33 and our Milky Way are the three largest members of the Local Group of galaxies. M31 is a spiral galaxy very similar in size and mass to our own. Ten 'pointings' of the camera along the galaxy in five filters were used to make the image. You could line seven full moons across the image. The image was generated with observations with the U (violet), B (blue), V (cyan), I (orange) and ...

86. Spiral Galaxy IC342

Spiral Galaxy IC342 is located roughly 11 million light-years from Earth in the constellation Camelopardalis, “the giraffe.” Its face-on appearance in the sky—as opposed to our tilted and edge-on views of many other nearby galaxies, such as the large spiral galaxy Andromeda (M31)—makes IC342 a prime target for studies of star formation and astrochemistry. The image, obtained in late 2006, was taken using the 64-megapixel Mosaic-1 digital imager on the Mayall 4-meter telescope. This image is the subject of NOAO press release 07-03

87. M78, NGC 2068

This image of M78, the brightest diffuse reflection nebula in the sky, was taken in 2006 with the Mosaic imager on the Mayall 4-meter telescope on Kitt Peak. Located some 1600 light-years away and around 4 light-years across, M78 is part of the Orion complex, a large region of star-forming gas and dust.

88. A Mysterious Rash of Star Birth

"A Mysterious Rash of Star Birth In this crisp Gemini North image, pink bubbles of glowing hydrogen gas spread across the arms of the face-on spiral galaxy NGC 6946 like a rash. This amazing infusion of color is fueled by the ubiquitous birth of massive stars throughout NGC 6946; these hot young stars blast copious amounts of ultraviolet radiation into their natal shrouds of hydrogen gas, causing the clouds to glow red. For reasons unknown, NGC 6946 has a much higher rate of star formation than all of the other large galaxies in our local neighborhood. The prodigious output of ...

89. Nicholas U. Mayall 4-meter Telescope

Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory.

90. Maunakea Panorama

Panoramic view of Maunakea rising above the Daniel K. Inouye Highway (Saddle road) after a light dusting for snow, as seen from Kipuka Pu'u Huluhulu.

91. Telescope structure as seen at sunset

Gemini North telescope at zenith "looking" through the open observing slit just before the beginning of nighttime observations. The 1-meter secondary mirror is visible at the top end.

92. Summit ridge telescope panorama

93. Gemini North Sunset Mirror Panorama

The 8-meter Frederick C. Gillett Gemini North telescope is located near the summit of Hawai‘i’s Maunakea — a long dormant volcano rising 4,214 meters into the dry, stable air of the North Pacific. Gemini North was designed and built, in part, to provide the best image quality possible from the ground for telescopes of its size. Four significant features help the telescope achieve this goal: (1) An ~20-centimeter-thin primary mirror on a bed of 120 hydraulic actuators; (2) a 1-meter-diameter secondary mirror capable of rapid tip-tilt corrective motions; (3) vents on the cylindrical walls to provide a smooth flow of ...

94. Orion "Bullets with GeMS

This image, obtained during the late commissioning phase of the GeMS adaptive optics system, with the Gemini South AO Imager (GSAOI) on the night of December 28, 2012, reveals exquisite details in the outskirts of the Orion Nebula. The large adaptive optics field-of-view (85 arcseconds across) demonstrates the system's extreme resolution and uniform correction across the entire field. The three filters used for this composite color image include [Fe II], H2, and, K(short)-continuum (2.093 microns) for blue, orange, and white layers respectively. The natural seeing while these data were taken ranged from about 0.8 to 1.1 arcseconds, with AO corrected ...

95. Panorama of Cerro Tololo Inter-American Observatory

Panorama of Cerro Tololo Inter-American Observatory, Chile.

96. Cerro Tololo Inter-American Observatory

Cerro Tololo Inter-American Observatory.

97. Telescope structure as seen at sunset

The top end of the Gemini North telescope pointed at zenith with the observing slit open at sunset.

98. Gemini North at night

The northern Gemini 8-meter telescope on Mauna Kea, Hawaii, is seen here in a long exposure at night. Behind the telescope can be seen the usual star trails due to the rotation of the Earth, as well as the trail of an incoming meteor over the summit. The streaks in front are from the tail lights of vehicles which drove up to the telescope while the camera shutter was open.

99. Star forming region NGC 7129

NGC 7129 is a star-forming region and reflection nebula in the constellation of Cepheus. It is about 3000 light years away from the Earth. The stars in this nebula are very young, only about a million years old. The red blobs above and below the nebula are Herbig Haro objects, which are the result of jets of gas streaming away from young stars in the nebula.

100. Star forming region, NGC 206

This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9m-meter telescope at Kitt Peak National Observatory. NGC 206 is a massive star-forming region (also known as an “OB association”) embedded in the Andromeda Galaxy (M31). It is clearly visible in the center to upper-left corner of the image. It is estimated to have a mass about 200,000 times that of our Sun. Its distinctive bluish color is from very young hot, massive stars in the cluster. The presence of these massive stars indicate that the cluster is less than 10 million years old, which ...

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