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Science

Red Dwarf – Astronomy

Red Dwarf – Astronomy

A Red Dwarf, as explained is the smallest and coolest kind of Star on the main sequence. The Red Dwarfs have a low Luminosity and individual Red Dwarfs can not hence be easily observed. They are the most common type of star in the Milky Way in the neighbourhood of the Sun. Proxima Centauri, the nearest star to the Sun is a Red Dwarf. The Red Dwarfs make up three-quarters of the stars in the Milky Way.

Read More about Red Dwarfs here

As reported by the Sci-News in their article dated 13th October 2021, Astronomers have detected coherent low-frequency radio emissions from a sample of 19 Red Dwarf (M-Dwarf) Stars. They detected this using the Low Frequency Array (LOFAR). LOFAR is a large Radio Telescope Network located mainly in the Netherlands. The Radio Emissions measured by them were of frequency less than 200 MHz.

Co-Author of the report Dr. Benjamin Pope mentioned “We have discovered signals from 19 distant Red Dwarf Stars, four of which are best explained by the existence of planets orbiting them. He is an Astronomer in the School of Mathematics and Physics at the University of Queensland and the Centre for Astrophysics at the Southern Queensland.

Read the detailed report of this detection on Sci-News

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Born and brought up in Kerala, I did my schooling in Kerala and graduated (B.Sc Physics) from the Calicut University. I have worked with a Swedish Company from 1994 to 2015, as a Senior Project Manager in their Group IT Division in Dubai. This blog is the result of my strong desire to communicate with others, sharing what I know and what I could gather from various sources.

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