Discovery of 12 rare ‘quadruple quasars’ can better tell the rate of universe expansion
- Posted By
10Pointer
- Categories
Science & Technology
- Published
15th Apr, 2021
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Context
The international astronomers from the Gaia Gravitational Lenses Working Group (GraL) have discovered 12 rare quasars.
About the rare quadruple quasars
- Quasars are distant galaxies with extremely luminous nuclei.
- Characteristics: They are consist of black holes.
- They measure many million times larger than our Sun.
- They are surrounded by thick gaseous matter.
- The first quadruple quasar image was captured in 1985.
- The latest finding has now increased the total confirmed Einstein’s crosses by 25 percent.
- Significance:Quasar observations are mainly used-
- to study dark matter in determining the evolution of galaxies
- to understand the rate of expansion of the universe., which is measured by using the Hubble-Lemaítre constant.
Hubble-Lemaítre constant
- It is expressed by the equation v = H0D, with H0 the constant of proportionality.
- Hubble constant is most frequently quoted in (km/s)/Mpc.
- Its value is about 70 (km/s)/Mpc.
- The SI unit of H0 is simply s−1, and the SI unit for the reciprocal of H0 is simply the second.
- The reciprocal of H0 is known as the Hubble time.
- The Hubble constant can also be interpreted as the relative rate of expansion.
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How the study is conducted for quasars?
- Each of the discovered quasars offersfour distinct quadruple images, which is commonly called Einstein’s cross.
- Gravity causes massive objects like galaxies and emissions from them to bend over time and space. Emissions from a quadruple quasar are said to bend over time and space causing ‘natural’ lenses.
- Some deflection is resultant of the presence of numerous galaxies which act as barriers located between a source and Earth, ultimately split it into four images.
- Big Data and Augmented Intelligence were applied to confirm this rare discovery.
How it is significant?
- Efforts are being conducted to confirm that the four closely packed images were not a pure chance alignment of four independent sources, but four images of a single, distant source, lensed by an intervening galaxy.
- This will help in refining the existing understanding of the universe’s rate of expansion and mysteries surrounding dark matter.