Giant Metrewave Radio Telescope - SCIENCE
News: Indian
astronomers use the Giant Metrewave Radio Telescope (GMRT) to discover
34 new giant radio sources (GRSs).
What’s
in the news?
- Discovery of Giant Radio
Sources: A team of Indian radio astronomers
has identified 34 new giant radio sources (GRSs).
- The
findings have been published in the Astrophysical Journal
Supplement Series (ApJS) of the American Astronomical Society.
- Challenging Conventional Views: Two
of the newly discovered GRSs, J0843+0513 and J1138+4540, challenge
the conventional notion that GRSs grow only in low-density
environments.
- Researchers
said that factors other than environmental density play a significant
role in the exceptionally large size of Giant Radio Galaxies (GRGs).
- Telescope Used: The
discovery was made using the Giant Metrewave Radio Telescope
(GMRT), located near Khodad village, about 90
km north of Pune.
- The GMRT is operated
by the National Centre for Radio Astrophysics (NCRA) of
the Tata Institute of Fundamental Research (TIFR).
- This
telescope surveyed the radio sky at a low frequency, making
it ideal for detecting these faint, distant objects.
- Survey Used: From
2010 to 2012, a survey was performed using the GMRT to map the radio
sky at 150 MHz, known as the TIFR GMRT Sky Survey (TGSS) covering
about 90% of the sky.
- The
team of astronomers used TIFR GMRT Sky Survey (TGSS) for their research
due to its low frequencies and the sensitivity of the GMRT.
- Advantages of Low-Frequency Radio
Surveys
- Suitability
for Identification: Low-frequency radio
surveys are more effective for identifying GRSs compared to
higher-frequency surveys.
- Brightness
of Aged Plasma: Aged plasma in GRSs is brighter
at low frequencies, making it easier to detect.
Historical
Background
- Past Discovery Rate: Only
about 100 giant radio sources were known 20 years ago.
- Reason for Limited Discovery: This
number was a tiny fraction of the actual population due to observational
limitations.
- Advancements in Detection: The
commissioning of new telescopes operating at low frequencies, such
as GMRT (Giant Metrewave Radio Telescope) and LOFAR (Low-Frequency
Array), has significantly increased the number of known giant radio
sources to a few thousand.
Giant
Radio Sources (GRS)
- About: Giant Radio Sources (GRS) are
among the largest structures in the universe.
- They
are powered by supermassive black holes at their centres, which
are millions to billions of times heavier than the Sun.
These
black holes emit powerful jets of hot plasma that create massive radio-emitting
lobes, extending well beyond the visible parts of the galaxy.
- Significance:
- Final
Stage of Radio Galaxies: GRSs are
believed to represent the final stage in the life of a radio
galaxy due to their immense size.
- Insights
into Radio Galaxy Evolution: The size and
structure of GRSs provide valuable insights into the evolution of
radio galaxies.
- The study of GRSs helps scientists
understand the relationship between black hole activity and the
evolution of radio galaxies.
- Understanding
Interstitial Space: GRSs offer
insights into the interstitial space between the lobes of radio galaxies.
- Cosmic
Matter Distribution and Behavior: Research on
giant radio galaxies aids in comprehending the distribution and
behaviour of matter in the cosmos.
- Challenges in Observing and
Discovering Giant Radio Sources:
- Separation
Issue: As radio sources grow in size, their
ends become more widely separated.
- Connection
Difficulty: The increased separation makes
it challenging to observationally connect the ends as part of the same
source.
Source:
https://indianexpress.com/article/cities/pune/indian-astronomers-discover-giant-radio-sources-9489547/