Description
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Context
Astrophysicist Raga Deepika Pucha's team discovers extensive samples of intermediate-mass black holes and active dwarf galaxies, enhancing cosmic evolution research
About Dwarf Blackholes
About Blackholes
- These are extremely dense, the gravitational attraction is so high that even light cannot escape.
- Albert Einstein first predicted the existence of black holes in 1916
- The first image ever recorded of a black hole was released in 2019
- Black holes do not die.
- They are theoretically predicted to evaporate over extremely long-time scales.
- Hawking predicted that black holes could radiate away energy.
- Black holes are not wormholes which can be thought of as tunnels that connect two separate points in space and time.
- Dwarf blackholes are small galaxies which typically contain just a few billion stars different from larger ones which can hold hundreds of billions.
- They are the most abundant but difficult to detect type of galaxy in the universe.
- They are difficult to detect because of
- low luminosity
- low mass
- smaller size
- They are most commonly found in galaxy clusters.
- Our Milky Way galaxy is orbited by more than 20 dwarf galaxies.
- Because most of them come from galaxy collisions, many dwarf galaxies are grouped into irregular shapes.
- However, some dwarf galaxies have spiral arms or look like mini-elliptical galaxies.
- The closest dwarf galaxy to Earth is the Canis Major Dwarf Galaxy.
- The Andromeda Galaxy (M31) is the closest major galaxy to the Milky Way.
- The nearest known black hole to Earth is Gaia BH1
Sources:
TOI
PRACTICE QUESTION
Q. What significant discovery was made by the team led by Raga Deepika Pucha?
A) Detection of the first exoplanet
B) Identification of the largest sample of intermediate-mass black holes and active dwarf galaxies
C) Discovery of water on Mars
D) Observation of the oldest known star
Answer: B) Identification of the largest sample of intermediate-mass black holes and active dwarf galaxies
Explanation:
Raga Deepika Pucha's team utilized data from the Dark Energy Spectroscopic Instrument (DESI) to compile the most extensive sample to date of intermediate-mass black holes and dwarf galaxies hosting active black holes, tripling the existing census and providing deeper insights into black hole and galaxy evolution.
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