Astronomers Detect Eleven New Active Galactic Nuclei

Astronomers Detect Eleven New Active Galactic Nuclei

17-05-2025

Relevance: GS III; Science and Tech; Space Technology;

Why in the News?

Astronomers from the Russian Academy of Sciences, using the Spektr-RG (SRG) space observatory, have detected 11 new Active Galactic Nuclei (AGNs) during their all-sky X-ray surveys.

  • The team has also previously identified more than 50 AGNs and several cataclysmic variable stars.

What are Active Galactic Nuclei (AGNs)?

  • There are active supermassive black holes at the center of galaxies that are emitting gas and dust as light all along the electromagnetic spectrum. These are known as Active Galactic Nuclei’s (AGNs).
  • There are majorly three types of Active Galactic Nuclei (AGNs):

  • Seyfert Galaxy is one among the most luminous and persistent energy sources in the universe and is critical to understanding galaxy formation and evolution. All new detected 11 AGNs were classified as Seyfert galaxies, a type of AGN that is common and well-studied:
    • 7 galaxies were classified as Seyfert Type 1 (Sy 1), characterized by broad optical emission lines.
    • 3 galaxies were classified as Seyfert Type 1.9 (Sy 1.9), showing partially broadened lines.
    • 1 galaxy was classified as Seyfert Type 2 (Sy 2), which exhibits narrow emission lines only.
  • The newly detected AGNs were identified during an optical and X-ray inspection of sources listed in the ARTSS1-5 catalog, using SRG’s ART-XC telescope.
  • Characteristics of the 11 Newly Detected AGNs: All 11 AGNs are located at redshifts ranging from 0.028 to 0.258, indicating they are relatively nearby in cosmic terms. Their X-ray luminosities fall within the typical range of 2 to 300 × 10³⁹ erg/s, which is consistent with known AGN profiles.

About the Spektr-RG (SRG):

  • Spektr-RG (Spektr-Rentgen-Gamma, SRG) is a Russian–German high-energy astrophysics space observatory designed to study the universe in the X-ray range of the electromagnetic spectrum. (with contributions from NASA and several European institutes)
  • It was launched on July 13, 2019, from Baikonur, Kazakhstan, on a Proton-M rocket.
  • The observatory is operational and actively conducting its all-sky X-ray survey.
    • It orbits around the Sun-Earth Lagrange point L2, about 1.5 million km from Earth, allowing stable and uninterrupted observations.
  • SRG carries two unique X-ray telescopes:
    • eROSITA (Germany): Specializes in soft X-ray surveys.
    • ART-XC (Russia): Focuses on higher-energy X-rays.

Aims and Objectives of the Mission:

  • To perform an all-sky survey in the X-ray energy band (0.3–11 keV) with unprecedented sensitivity.
  • To map and study massive structures in the universe, including galaxy clusters, Active Galactic Nuclei (AGNs), supermassive black holes, and other energetic phenomena.
  • To answer key questions in cosmology, such as the role of dark energy and dark matter in the formation of large-scale cosmic structures.
  • To detect and catalog about 100,000 galaxy clusters and around three million supermassive black holes in AGNs over the mission duration.

Way Forward: SRG’s surveys are expected to revolutionize our understanding of the high-energy universe by providing the most detailed X-ray maps to date. The mission enables the discovery of new cosmic objects, studies of galaxy evolution, and insights into the physics of black holes and the intergalactic medium.

PYQ Significance:

Mains:

Q. Launched on 25 th December, 2021, James Webb Space Telescope has been much in the news since then. What are its unique features which make it superior to its predecessor Space Telescopes? What are the key goals of this mission? What potential benefits does it hold for the human race? (UPSC CSE 2022)

 


 

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