(GIST OF SCIENCE REPORTER) Molecular Cloud

(JANUARY-2026)

Recently, astronomers studied the L328 molecular cloud, located around 700 light years away, to map the magnetic fields at multiple scales.

It is an interstellar cloud of gas and dust in which molecules can form, the most common of which is Hydrogen (H2).

These are characterized by their low temperatures (below 40 K, colder than liquid nitrogen) and relatively high densities.
Size: The size of these clouds can be from a few light years up to 600 light years. Their total mass can reach several million solar masses.
Molecular clouds with dimensions of more than about 15 light years are also called giant molecular clouds.
The complex interplay between three key forces, namely gravity, magnetic fields, and turbulence, determines how these clouds collapse to form stars.
The central regions of these clouds are completely hidden from view by dust.
They are the raw material of stars and planets. These clouds do not last for a very long time.
After the new stars are born, their solar winds blow away the remaining gas and dust.

Molecular clouds are so important because they are the raw material of stars and planets.
It is thought to be the birthplace of stars and planetary systems through processes of contraction, condensation, and accretion.