Molecular Cloud

Molecular Cloud

Molecular Cloud Latest News

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

About Molecular Cloud

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

Properties of Molecular Cloud

  • These are characterized by their low temperatures (below 40 K, colder than liquid nitrogen) and relatively high densities (103–104 particles per cubic cm).
  • 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. 

Significance of Molecular Cloud

  • 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.

Source: PIB

Molecular Cloud FAQs

Q1: What is the primary component of molecular clouds?

Ans: Molecular hydrogen

Q2: What is a molecular cloud?

Ans: A region of space with cold, dense molecular gas and dust

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