1.5 billion cosmic objects dazzle in the largest infrared Milky Way map ever created

‘We have changed the view of our galaxy forever.’

Posted on Sep 26, 2024

This collage highlights a small selection of regions of the Milky Way imaged as part of the most detailed infrared map ever of our galaxy. Here we see, from left to right and top to bottom: NGC 3576, NGC 6357, Messier 17, NGC 6188, Messier 22 and NGC 3603. All of them are clouds of gas and dust where stars are forming, except Messier 22, which is a very dense group of old stars. — This collage highlights a small selection of regions of the Milky Way imaged as part of the most detailed infrared map ever of our galaxy. Here we see, from left to right and top to bottom: NGC 3576, NGC 6357, Messier 17, NGC 6188, Messier 22 and NGC 3603. All of them are clouds of gas and dust where stars are forming, except Messier 22, which is a very dense group of old stars. Credit: ESO/VVVX survey

Astronomers from the European Southern Observatory (ESO) have released the most detailed infrared map of the Milky Way galaxy ever compiled. Completed after more than 13 years of monitoring using the ESO’s Visible and Infrared Survey Telescope for Astronomy (VISTA) at the group’s Paranal Observatory in Chile, the project adds up to 500 terabytes of data containing over 1.5 billion cosmic objects. Taken as a whole, the mapping is the largest survey of its kind to employ an ESO telescope.

This is an infrared view of the Messier 22 globular cluster, a densely packed group of very old stars located about 10 000 light-years away in the constellation Sagittarius. The image was taken with ESO’s VISTA ― the Visible and Infrared Survey Telescope for Astronomy ― and its infrared camera VIRCAM. It is part of a record-breaking infrared map of the Milky Way containing more than 1.5 billion objects. The data were gathered as part of the VISTA Variables in the Vía Láctea (VVV) survey and its companion project, the VVV eXtended survey (VVVX). — This is an infrared view of the Messier 22 globular cluster, a densely packed group of very old stars located about 10 000 light-years away in the constellation Sagittarius. The image was taken with ESO’s VISTA ― the Visible and Infrared Survey Telescope for Astronomy ― and its infrared camera VIRCAM. It is part of a record-breaking infrared map of the Milky Way containing more than 1.5 billion objects. The data were gathered as part of the VISTA Variables in the Vía Láctea (VVV) survey and its companion project, the VVV eXtended survey (VVVX). Credit: ESO/VVVX survey

According to a September 26 announcement, the survey began in 2010 and continued through the first half of 2023, ultimately collecting images over 420 nights. The results are detailed in the September issue of the journal Astronomy & Astrophysics. Observing specific patches of evening sky multiple times allowed astronomers to determine object locations, movement, and changes in brightness. A star’s shifts in luminosity, for example, allows experts to use them as “cosmic rulers” to measure distances between galactic entities, which then helped generate an accurate 3D view of the Milky Way’s interior. VISTA’s infrared camera, VIRCAM, also allowed the team to filter through cosmic dust and keep tabs on “hypervelocity stars,” whose extreme speeds originate from near-misses with the galaxy’s central supermassive black hole, Sagittarius A*.

This Picture of the Week shows a new view of NGC 3603 (left) and NGC 3576 (right), two stunning nebulas imaged with ESO’s Visible and Infrared Survey Telescope for Astronomy (VISTA). This infrared image peers through the dust in these nebulas, revealing details hidden in optical images. NGC 3603 and NGC 3576 are 22,000 and 9,000 lightyears away from us, respectively. Inside these extended clouds of dust and gas, new stars are born, gradually changing the shapes of the nebulas via intense radiation and powerful winds of charged particles. Given their proximity, astronomers have the opportunity to study the intense star formation process that is as common in other galaxies but harder to observe due to the vast distances. The two nebulas were catalogued by John Frederick William Herschel in 1834 during a trip to South Africa, where he wanted to compile stars, nebulas and other objects in the sky of the southern hemisphere. This catalogue was then expanded by John Louis Emil Dreyer in 1888 into the New General Catalogue, hence the NGC identifier in these and other astronomical objects. — This Picture of the Week shows a new view of NGC 3603 (left) and NGC 3576 (right), two stunning nebulas imaged with ESO’s Visible and Infrared Survey Telescope for Astronomy (VISTA). This infrared image peers through the dust in these nebulas, revealing details hidden in optical images. NGC 3603 and NGC 3576 are 22,000 and 9,000 lightyears away from us, respectively. Inside these extended clouds of dust and gas, new stars are born, gradually changing the shapes of the nebulas via intense radiation and powerful winds of charged particles. Given their proximity, astronomers have the opportunity to study the intense star formation process that is as common in other galaxies but harder to observe due to the vast distances. The two nebulas were catalogued by John Frederick William Herschel in 1834 during a trip to South Africa, where he wanted to compile stars, nebulas and other objects in the sky of the southern hemisphere. This catalogue was then expanded by John Louis Emil Dreyer in 1888 into the New General Catalogue, hence the NGC identifier in these and other astronomical objects. Credit: ESO/VVVX survey

This image shows a detailed infrared view of Messier 17, also known as the Omega Nebula or Swan Nebula, a stellar nursery located about 5500 light-years away in the constellation Sagittarius. This image is part of a record-breaking infrared map of the Milky Way containing more than 1.5 billion objects. ESO’s VISTA ― the Visible and Infrared Survey Telescope for Astronomy ― captured the images with its infrared camera VIRCAM. The data were gathered as part of the VISTA Variables in the Vía Láctea (VVV) survey and its companion project, the VVV eXtended survey (VVVX). — This image shows a detailed infrared view of Messier 17, also known as the Omega Nebula or Swan Nebula, a stellar nursery located about 5500 light-years away in the constellation Sagittarius. This image is part of a record-breaking infrared map of the Milky Way containing more than 1.5 billion objects. ESO’s VISTA ― the Visible and Infrared Survey Telescope for Astronomy ― captured the images with its infrared camera VIRCAM. The data were gathered as part of the VISTA Variables in the Vía Láctea (VVV) survey and its companion project, the VVV eXtended survey. Credit: ESO/VVVX survey

“We made so many discoveries, we have changed the view of our galaxy forever,” Dante Minniti, VISTA Variables in the Vía Láctea (VVV) survey project lead and an astrophysicist at Chile’s Universidad Andrés Bello, said in a statement. Vía Láctea is the Latin name for the Milky Way.

The total area of the sky mapped is equal in size to 8,600 full moons that include an estimated 10 times more galactic objects than the team’s previous map, released in 2012. Among these hundreds of millions of tiny specks of light lurk newborn stars, extremely cold brown dwarfs that only glow at infrared wavelengths, free-floating planets, and globular clusters—groupings containing millions of the Milky Way’s oldest stars in existence.

More than 300 scientific articles containing numerous discoveries and new information have been published thanks to the survey and its partner project, the VVV eXtended (VVVX) survey. Moving forward, VISTA will receive a new instrument, the 4-meter Multi-Object Spectrograph Telescope (4MOST), which will allow the system to perform larger spectroscopic surveys capable of imaging 2,400 objects’ spectra at the same time across a region of the sky equal to 20 full moons.

[Related: Humongous stellar-mass black hole is the biggest ever found in Milky Way.]

Meanwhile, ESO’s Very Large Telescope (VLT) will receive an upgrade through the Multi-Object Optical and Near-infrared Spectrograph (MOONS), which is dedicated to studying galaxy formations and evolutions throughout the known universe’s history.