One of the first images captured by Euclid shows the Perseus cluster, a group of thousands of galaxies located 240 million light-years from Earth. The closest galaxies appear as swirling structures while hundreds of thousands of background galaxies are visible only as points of light.
ESA/Euclid/Euclid Consortium/NASA, image processing by
J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO
The new images from the Euclid mission include a cluster of thousands of
distant galaxies, demonstrating the spacecraft’s unique abilities.
The Euclid mission, which will
investigate the mysteries of dark matter and dark energy, released its first five science images Tuesday, Nov. 7 The observatory, led by ESA
(European Space Agency) with NASA contributions, is scheduled to begin regular
science operations in early 2024.
The new images include views of a
large cluster of thousands of distant galaxies, close-ups of two nearby
galaxies, a gravitationally bound group of stars called a globular cluster, and
a nebula (a cloud of gas and dust in space where stars form) – all depicted in
vibrant colors.
“The Euclid observatory will
uncover a treasure trove of scientific discoveries that will be used across the
world, including by U.S. scientists, for years to come,” said Nicola Fox,
associate administrator, Science Mission Directorate, at NASA Headquarters in
Washington. “Together, NASA and ESA are paving the way for a new era of
cosmology for NASA’s forthcoming Nancy Grace Roman Space Telescope, which will build upon what Euclid learns and will
additionally survey objects on the outskirts of our solar system, discover
thousands of new planets, explore nearby galaxies, and more.”
The spiral galaxy IC 342, located about 11 million
light-years from Earth, lies behind the crowded plane of the Milky Way: Dust,
gas, and stars obscure it from our view. Euclid used its near-infrared
instrument to peer through the dust and study it.
ESA/Euclid/Euclid Consortium/NASA, image processing by
J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO
Euclid launched on July 1 from Cape Canaveral, Florida, then traveled nearly 1 million miles to
its vantage point. Following a period of commissioning (testing of the
instruments and other components), the space telescope is performing as
expected.
NASA’s Jet Propulsion Laboratory in
Southern California delivered critical hardware for one of the Euclid spacecraft’s instruments.
In addition, NASA has established a U.S.-based Euclid science data center, and
NASA-funded science teams will join other Euclid scientists in studying dark
energy, galaxy evolution, and dark matter. The agency’s Nancy Grace Roman
mission will also study dark energy – in ways that are complementary to Euclid.
Mission planners will use Euclid’s findings to inform Roman’s dark energy work.
Surveying the Dark Universe
During its planned six-year
mission, Euclid will produce the most extensive 3D map of the universe yet,
covering nearly one-third of the sky and containing billions of galaxies up to
10 billion light-years away from Earth.
The galaxy NGC 6822 is located 1.6 million light-years
from Earth. Euclid was able to capture this view of the entire galaxy and its
surroundings in high resolution in about one hour, which isn’t possible with
ground-based telescopes or targeted telescopes (such as NASA’s Webb) that have
narrower fields of view.
ESA/Euclid/Euclid Consortium/NASA, image processing by
J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO
To do this, Euclid needs a wide field of view, which enabled these new
images covering a relatively large area. In this way, Euclid differs from
targeted observatories like NASA’s
James Webb Space Telescope that focus on a smaller area of the sky at any one time but typically
offer higher-resolution images. Wide-field observatories like Euclid can
observe large sections of the sky much faster than targeted telescopes. In
addition, Euclid has high resolution compared to previous survey missions,
which means it will be able to see more galaxies in each image than previous
telescopes.
For example, Euclid’s wide view was
able to capture the entirety of the Perseus galaxy cluster, and many galaxies
beyond it, in just one image. Located 240 million light-years from Earth,
Perseus is among the most massive structures known in the universe. Euclid’s
full survey will ultimately cover an area 30,000 times larger than this image.
The Horsehead Nebula, also known as Barnard 33, is
part of the Orion constellation. About 1,375 light-years away, it is the
closest giant star-forming region to Earth. With Euclid, which captured this
image, scientists hope to find many dim and previously unseen Jupiter-mass
planets in their celestial infancy, as well as baby stars. Full image here.
ESA/Euclid/Euclid Consortium/NASA, image processing by
J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO
The telescope’s survey approach is necessary to study dark energy, the
mysterious driver behind our universe’s accelerating expansion. While gravity
should pull everything in the universe together, everything is instead moving
apart faster and faster. “Dark energy” is the term scientists use for this
unexplained expansion.
To study the phenomenon, scientists
will map the presence of another cosmic mystery, dark matter. This invisible
substance can be observed only by its gravitational effect on “regular” matter
and objects around it, like stars, galaxies, and planets. Dark matter is five
times more common in the cosmos than regular matter, so if dark energy’s
expansive influence on the universe has changed over time, the change should be
recorded in how dark matter is distributed on large scales across the universe,
and Euclid’s 3D map should capture it.
This sparkly image shows Euclid’s view of a globular
cluster – a collection of gravitationally bound stars that don’t quite form a
galaxy – called NGC 6397. No other telescope can capture an entire globular
cluster in a single observation and distinguish so many stars within it.
ESA/Euclid/Euclid Consortium/NASA, image processing by
J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO
“Euclid’s first images mark the beginning of a new era of studying dark
matter and dark energy,” said Mike Seiffert, Euclid project scientist at JPL.
“This is the first space telescope dedicated to dark universe studies, and the
sheer scale of the data we’re going to get out of this will be unlike anything
we’ve had before. These are big mysteries, so it’s exciting for the
international cosmology community to see this day finally arrive.”
NASA’s Roman mission will study a
smaller section of sky than Euclid, but it will provide higher-resolution
images of hundreds of millions of galaxies and peer deeper into the universe’s
past, providing complementary information. Scheduled to launch by May 2027.
The data from the new Euclid images
is now available to the scientific community, and scientific papers analysing
that data are expected to follow. As the mission progresses, Euclid’s bank of
data will grow. New batches will be released once per year and will be
available to the global scientific community via the Astronomy Science Archives hosted at ESA’s European Space Astronomy Centre
in Spain.
More About the Mission
Euclid is a European mission, built
and operated by ESA, with contributions from NASA. The Euclid Consortium –
consisting of more than 2,000 scientists from 300 institutes in 13 European
countries, the U.S., Canada, and Japan – is responsible for providing the
scientific instruments and scientific data analysis. ESA selected Thales Alenia
Space as prime contractor for the construction of the satellite and its service
module, with Airbus Defence and Space chosen to develop the payload module,
including the telescope. NASA provided the detectors of the Near-Infrared
Spectrometer and Photometer, NISP. Euclid is a medium-class mission in ESA’s
Cosmic Vision Programme.
Source: First Science Images Released From ESA Mission With NASA Contributions - NASA
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