July 6, 2024
1 Solar System Way, Planet Earth, USA
Space

Euclid Telescope Reveals Groundbreaking Images and Data – Sky and Telescope

The European Space Agency (ESA) Euclid space mission just launched your first scientific dataalong with another impressive set of five images revealing wide, deep and detailed views of stellar nurseries and galaxies near and far. These materials are part of Euclid's early published Observations, spanning 513 scientific pages and 10 images (the first five of which were launched in 2023).

The five images of Euclid.
The Euclid mission has shared five new views of the universe: The five targets shown here are (clockwise from top left) the Dorado Group of galaxies, the star-forming nebula Messier 78, the galaxy spiral NGC 6744 and the two Abell galaxy clusters. 2764 and Abell 2390
ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi

This cosmic treasure is the result of only 24 hours of observation, showing the advantages of Euclid: speed and range. The space telescope has created these expansive cosmic portraits in just one hour of observation.

Euclid carries two instruments: the visible instrument (VIS) and the near-infrared spectrometer and photometer (NISP). VIS is a 609-megapixel visible-band imager, sensitive to low light levels and capable of imaging 0.5 square degrees at a time, equivalent to the area of ​​2.5 full moons as seen from Earth. Similarly, NISP has the widest field of view of any infrared instrument ever lifted into space, at 0.57 square degrees per exposure.

Together, the two instruments produce wide, deep, high-resolution images hundreds of times faster than other telescopes. These snapshots are at least four times sharper than any of their ground-based Euclid counterparts, and hundreds of times larger than comparable other space telescopes.

The published images show Euclid's prodigious field of view and sharp resolution. The mission will use them to capture cosmic evolution in 3D, from 10 billion years ago to the present, investigating the distribution and functioning of dark matter, as well as the influence of dark energy in accelerating the expansion of our planet. universe.

Five new images of Euclid

A filamentary orange veil covers a bright star-forming region.  The background is dark, dotted with stars and galaxies ranging from small bright dots to starry shapes.  The foreground veil extends from the top left to the bottom right and resembles a seahorse.  Bright stars illuminate the regions of the
This stunning image shows Messier 78 (the central and brightest region), a vibrant stellar nursery shrouded by interstellar dust.
ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre (CEA Paris-Saclay) / G. Anselmi

In the first image, Euclid's infrared eyes pierce the dense dust and gas of the Messiest 78 nebula, 1,300 light-years away in Orion, to reveal hot young stars enveloped by gas and entwined by darker filaments of interstellar dust.

By looking through the shroud for the first time, “Euclid has discovered half a million objects, including galaxies and stars,” explains Maruša Žerjal, member of the scientific team (Institute of Astrophysics of the Canary Islands, Spain).

Surprisingly, astronomers can use Euclid to study much smaller objects in such wide images, including brown dwarfs and planets only a few times more massive than Jupiter. A complete census of these objects will reveal some of the mass hidden in the universe's population of small bodies, adds Jerry Zhang (also at the institute). The team also plans to measure the ratio between stars and substellar objects over cosmic time.

A spiral galaxy on a dark background dotted with bright dots.  The clockwise spiral has many arms, not completely distinguishable from each other, extending from a bright central point.  There is a thin cloud structure just above the galaxy, on the outskirts of its farthest arm.  At the bottom left of the image, two bright spots are surrounded by a halo of light.
NGC 6744 is one of the largest spiral galaxies beyond our local space.
ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre (CEA Paris-Saclay) / G. Anselmi

This image of the spectacular spiral NGC 6744, 30 million light years away in the southern constellation of Pavo, NGC 6744 captures an “archetype of the type of galaxy that currently forms most of the stars in the local Universe,” according to a study. ESA press release. The image shows the galaxy's spiral arms, as well as finer features such as the feathered dust lanes between the arms. Euclid's millimeter precision even allows astronomers to “count individual stars and reveal the distribution of dust,” says researcher Francesca Annibali (INAF-OAS, Italy).

Astronomers will use Euclid to create comprehensive maps of diverse stellar populations, including newborn stars, old star clusters, and the dusty distribution of future stars, relating their formation to the physics of spiral structures.

A starry sky on a black background with three large glowing structures.  The two largest, in the center and center right of the image, have very bright centers with large spherical halos surrounding them.  The edges of these halos appear to touch each other.  A third bright structure is present at the bottom left and looks like a small ellipsoid version of the other two.  Finally, a thin, elongated, shiny ellipse is located in the upper left corner.
The Golden Group of galaxies is one of the richest groups of galaxies in the southern hemisphere. Here, Euclid captures signals of galaxies evolving and merging “in action”, with beautiful tidal tails and shells visible as a result of ongoing interactions.
ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre (CEA Paris-Saclay) / G. Anselmi

The Golden Group of galaxies, located 62 million light-years away in the constellation Dorado, shows “the evolution of galaxies as it is happening,” says Karina Voggel (Strasbourg Observatory, France).

Some of its members are merging or showing signs of recent mergers. As an intermediary between immense galaxy clusters and smaller galaxy groups, the Golden Group is a valuable snapshot of medium-scale structure and galactic collisions.

Clusters of many thousands of stars appear around the Golden Group. Teymoor Saifollahi (Strasbourg Observatory, France) points out that these globular clusters are part of the Golden Group, since both the clusters and the group were born together approximately 10 billion years ago.

A starry sky on a dark background.  One star is large and bright and is located at the bottom of the image.  In the upper right corner, the galaxies are grouped together.  They look like small, shiny, ellipsoid spheres.  Throughout the image, small bright dots and a handful of glowing spheres are evenly distributed.
This nearly empty “blank field” is actually centered on the outskirts of the dense galaxy cluster Abell 2764, which is located at the top right.
ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre (CEA Paris-Saclay) / G. Anselmi

One of the main scientific goals of the Euclid mission is to search for dark matter, and Abell 2674, a billion light years away in Pisces, offers a main goal. This galaxy cluster, top right, is a gravitationally bound package of hundreds of galaxies “orbiting a halo of dark matter,” according to Hakim Atek (Paris Institute of Astrophysics).

Such dense regions of space are perfect places to explore the effects of dark matter. Atek describes these “blank fields” as “more representative of the large-scale distribution of galaxies in the universe.”

This single targeting, which already contains 250,000 galaxies and other celestial objects, is one of the first of many: Euclid will map an area 30,000 times larger than this image, or about a third of the sky.

The downward shining star (V*BP-Phoenicis/HD 1973) is located within our Milky Way and demonstrates Euclid's design, which minimizes light scattering. “This is precisely what defines Euclid's keen vision of the universe,” says Atek.

Thousands of stars and galaxies dot the image on a pitch black background.  Some bright stars show six diffraction peaks from a central halo of light.  Other stars and galaxies are just small bright spots, like flecks of paint spread over the image.  The brightest star is in the upper left corner.  In the center of the image, the small bright spots are more abundant.
This image of the galaxy cluster Abell 2390 contains about 50,000 galaxies.
ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre (CEA Paris-Saclay) / G. Anselmi

The galaxy cluster Abell 2390, 2.7 billion light years away in Pegasus, is an immense agglomeration of galaxies like our Milky Way. It is accompanied by an impressive panorama of 50,000 galaxies. And thanks to Euclid, scientists can now measure their distances and shapes.

Galaxy clusters can contain “the mass of 10 trillion suns,” explains Jason Rhodes (NASA JPL), and much of that mass may be in the form of dark matter. The gravity of these clusters warps the path of background photons in a phenomenon known as gravitational loans. This effect can be seen in the curved arcs of the image, some of which show multiple images of the celestial objects behind them.

Astronomers can also use this image to study intracluster light Cast by orphan stars. Intergalactic interactions have driven these stars from their galactic homes to wander alone through intergalactic space.


This quintet of status quo changes is just the beginning, as Euclid only began its six-year scientific study in February. He will observe more than a third of the sky and see billions of galaxies 10 billion light years away, creating a monumental three-dimensional map through space and time.

The only drawback? The next data release is scheduled for March 2025. But since Euclid inspires imagination and innovation, who knows what enlightening discoveries will be made in the meantime.

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