Astronomy
Follow me on X Follow me on Bluesky Follow me on Pinterest
English Français Español Português 日本語 Deutsch
 
Last updated: December 15, 2023

The hidden galaxy

The hidden galaxy
The galaxy IC 342 or Caldwell 5 is nicknamed the “hidden galaxy” because, in the visible domain, it is partially hidden by dust from our galaxy, the Milky Way. However, Euclid allows it to be observed in the near infrared. The “hidden galaxy” is one of the four images that Euclid took during its first observation of the cosmos, 4 months after its launch.
Credit: ESA

The hidden galaxy, one of Euclid's first images

The hidden galaxy IC 342 is a spiral galaxy located approximately 3.28 megaparsecs or 10.7 million light years from Earth, in the constellation Giraffe. Despite its size and actual brightness, its location behind dusty areas near the galactic equator makes it difficult to observe, earning it the nickname "The Hidden Galaxy." If the galaxy were not obscured, it would be visible to the naked eye.
However, thanks to ESA's Euclid space mission, which was launched in July 2023 and which observes the universe in the near infrared, we can see this galaxy in exceptional clarity.

The Euclid image shows that the galaxy IC 342 is an active galaxy, with many stars forming. It also contains a large number of nebulae, regions of gas and dust where stars form. We can also distinguish filaments and bubbles which testify to interactions between galaxies.

Although close, the hidden galaxy is not a member of the Local Group. IC 342 as well as NGC 1560, NGC 1569, UGCA 92 and UGCA 105 are galaxies of the IC 342/Maffei16 group, a neighboring group of the Local Group.

Euclid's image allowed astronomers to discover that the hidden galaxy contains about 100 billion stars, and is a significant source of ultraviolet radiation. It interacts with another neighboring galaxy, the galaxy NGC 1569. This galaxy is an irregular dwarf galaxy that is located approximately 1.5 million light years from the galaxy IC 342. It has a diameter of 2,000 light years, or about 10% of the diameter of the Milky Way. Its star formation rate is 100 times that of the Milky Way.
Astronomers believe that the galaxy NGC 1569 is being absorbed by the galaxy IC 342. This gravitational interaction between the two galaxies is responsible for active star formation in the galaxy IC 342.

Euclid is a space telescope that aims to study the influence of dark matter and energy on the expansion and structure of the universe. It measures the distances and movements of billions of galaxies that it observes over a wide swath of the sky. From javier 2024, he will create the largest 3D cosmic map ever made.

To explore in this category

The Great Attractor: The Celestial Fountain Pulling Us into the Abyss The Great Attractor: The Celestial Fountain Pulling Us into the Abyss
The 5 Strangest Objects in Our Galaxy: From Zombie Stars to Diamond Planets The 5 Strangest Objects in Our Galaxy: From Zombie Stars to Diamond Planets
Why Is It So Hard to See the Milky Way? Why Is It So Hard to See the Milky Way?
What Is a Galaxy? Journey to the Land of Billions of Stars What Is a Galaxy? Journey to the Land of Billions of Stars
Galaxies from the Depths: Light from the Primordial Universe Galaxies from the Depths: Light from the Primordial Universe
Journey to the Heart of the Milky Way: Mysteries and Wonders Journey to the Heart of the Milky Way: Mysteries and Wonders
JWST and Protogalaxies: Exploring the First Cosmic Structures JWST and Protogalaxies: Exploring the First Cosmic Structures
Collision and Cannibalism: How Large Galaxies Absorb Smaller Ones Collision and Cannibalism: How Large Galaxies Absorb Smaller Ones
Beyond Our Senses! Beyond Our Senses!
Future Collision of Our Galaxy with the Sagittarius Galaxy Future Collision of Our Galaxy with the Sagittarius Galaxy
Differences between the Milky Way and the Andromeda Galaxy Differences between the Milky Way and the Andromeda Galaxy
Why are Galaxies, Unlike Stars, So Close to Each Other? Why are Galaxies, Unlike Stars, So Close to Each Other?
Galaxies of the Local Group Galaxies of the Local Group
The hidden galaxy, one of Euclid's first images The hidden galaxy, one of Euclid's first images
The Virgo Cluster spans approximately three Full Moons The Virgo Cluster spans approximately three Full Moons
Where did the dark matter in our Galaxy go? Where did the dark matter in our Galaxy go?
Galaxy Mergers: From Encounter to Coalescence Galaxy Mergers: From Encounter to Coalescence
Gravitational Lenses: When Spacetime Bends Light Gravitational Lenses: When Spacetime Bends Light
Cartwheel Galaxy: A Wheel of Fire in the Universe Cartwheel Galaxy: A Wheel of Fire in the Universe
From Dust to Stars: The Composition of Galaxies From Dust to Stars: The Composition of Galaxies
Galaxy Merger NGC 6745: A Traversal of One by the Other Galaxy Merger NGC 6745: A Traversal of One by the Other
The mystery of gamma bursts The mystery of gamma bursts
The Cigar Explosion The Cigar Explosion
Extreme Shock Waves in the Universe: Impact on the Evolution of Cosmic Structures Extreme Shock Waves in the Universe: Impact on the Evolution of Cosmic Structures
Gould's belt, a stellar fireworks display Gould's belt, a stellar fireworks display
Zoom on Our Galaxy: Journey to the Center of the Milky Way Zoom on Our Galaxy: Journey to the Center of the Milky Way
One Galaxy, Two Hearts: The Mystery of Andromeda's Double Nucleus One Galaxy, Two Hearts: The Mystery of Andromeda's Double Nucleus
The most beautiful galaxy clusters The most beautiful galaxy clusters
Tinker Bell's Gravitational Flight: A Merger of Three Galaxies Tinker Bell's Gravitational Flight: A Merger of Three Galaxies
Aligned Galaxies Around Andromeda: Chance or Hidden Structure? Aligned Galaxies Around Andromeda: Chance or Hidden Structure?
Coma or Berenice’s Hair: The Cosmic Colossus Coma or Berenice’s Hair: The Cosmic Colossus
When Dark Matter Reveals Itself When Dark Matter Reveals Itself
El Gordo galaxy cluster El Gordo galaxy cluster
Einstein ring and cross Einstein ring and cross
How to measure distances in the Universe? How to measure distances in the Universe?
The Cigar Galaxy: A Smoke of Stars in the Night The Cigar Galaxy: A Smoke of Stars in the Night
The Hubble Sequence: The Secret Code of Galactic Shapes The Hubble Sequence: The Secret Code of Galactic Shapes
Dance of the Stars: The Arms of the Milky Way Dance of the Stars: The Arms of the Milky Way
The most beautiful galaxies The most beautiful galaxies
Ancient Galaxies and Cosmic Evolution: A Deep Look Back in Time Ancient Galaxies and Cosmic Evolution: A Deep Look Back in Time
Quasars: Beacons of the Distant Cosmos Quasars: Beacons of the Distant Cosmos
Sagittarius A black hole at the center of our Galaxy Sagittarius A black hole at the center of our Galaxy
MOND Theory and Dark Matter: Why MOND Fails in Cluster Collisions MOND Theory and Dark Matter: Why MOND Fails in Cluster Collisions
Central area of the Milky Way Central area of the Milky Way
Laniakea, our supercluster of galaxies Laniakea, our supercluster of galaxies
The Antennae Galaxies: An Ongoing Cosmic Collision The Antennae Galaxies: An Ongoing Cosmic Collision
NGC 1275: A Turbulent Galaxy in the Perseus Cluster NGC 1275: A Turbulent Galaxy in the Perseus Cluster
NGC 1672: A Barred Spiral Galaxy in Full Activity NGC 1672: A Barred Spiral Galaxy in Full Activity