The Euclid Space Telescope has made an exciting discovery—a new Einstein ring in the nearby galaxy NGC 6505, located 590 million light-years from Earth.
- This rare celestial phenomenon, now called Altieri’s Ring, was first noticed in September 2023 by astronomer Bruno Altieri in an early, unfocused image from Euclid.

About Euclid Space Telescope
- The Euclid Space Telescope is a European Space Agency (ESA) mission, launched on July 1, 2023.
- It was launched to study dark matter and dark energy—two of the most mysterious components of the universe.
- It aims to create a 3D map of the universe, covering billions of galaxies up to 10 billion light-years away.
Key Features of the Euclid Telescope |
Feature |
Details |
Orbit |
Sun-Earth Lagrange Point 2 (L2), approximately 1.5 million kilometers from Earth in the opposite direction of the Sun. |
Instruments |
Visible Imaging Camera (VIS) & Near-Infrared Spectrometer and Photometer (NISP) |
Resolution |
High-resolution images covering large sky areas |
Mission Duration |
6 years (extendable) |
Significance of the Euclid Mission
- Deepens Our Understanding of the Cosmos: Helps solve fundamental questions about dark energy and the universe’s fate.
- Largest Cosmic Map Ever Created: Covers 10 billion years of cosmic history.
- Supports Future Astronomy Missions: Complements NASA’s James Webb Space Telescope (JWST) and ESA’s Gaia mission.
What is an Einstein Ring?

- Over a century ago, Albert Einstein predicted that massive objects, like galaxies or galaxy clusters, can bend light from distant objects due to their gravitational pull.
- This effect, known as gravitational lensing, can create arc-like or circular patterns of light around the foreground object.
- When the alignment between the observer, the lens, and the distant object is nearly perfect, the result is a complete circle of light called an Einstein ring.
- It Is Not visible to the naked eye, can only be observed through powerful space telescopes like Euclid.
Einstein rings are scientifically valuable because they
- Help study dark matter by revealing how mass is distributed in the foreground galaxy.
- Provide insights into the expansion of the universe and test Einstein’s General Theory of Relativity.
- Allow astronomers to observe distant galaxies that would otherwise be hidden.
Einstein Cross
- The Einstein Cross is a rare and visually striking example of gravitational lensing.
- It occurs when a massive object, like a galaxy, bends and distorts the light from a more distant object behind it, creating multiple images of the background object.
- The first Einstein Cross, known as Q2237+030 or Huchra’s Lens, was discovered in 1985.
- It is located in the constellation Pegasus, about 8 billion light-years from Earth.
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The Discovery of Altieri’s Ring

- The discovery was made by astronomer Bruno Altieri in September 2023, just two months after the Euclid telescope was launched.
- Initially, the image of NGC 6505 was blurry, as it was taken during the testing phase of the mission.
- However, subsequent focused images confirmed the presence of the Einstein ring, which has since been named Altieri’s ring in his honor.
- The ring is formed by the distorted light of a galaxy located 4.5 billion light-years behind NGC 6505.
Why is Altieri’s Ring Special?
- Proximity: Most Einstein rings are found much farther away, but Altieri’s Ring is one of the closest ever observed. Only five other gravitational lenses have been found at a similar distance.
- A New View of an Old Galaxy: The foreground galaxy, NGC 6505, has been known to astronomers since the 19th century. Yet, Euclid’s advanced instruments revealed the Einstein ring for the first time.
- Distant Background Galaxy: The light forming the ring comes from a galaxy 4.5 billion light-years away, which is no longer forming new stars.
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