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They may be little, but they pack a big star-forming punch.

New observations from NASA's Hubble Space Telescope show that small galaxies, also known as dwarf galaxies, are responsible for forming a huge proportion of the universe's stars.

The researcher admit they were stunned by the results, and say the dwarf galaxies are far more prolific than they thought.

Hiding among these thousands of galaxies in an image from Hubble are faint dwarf galaxies residing in the early universe, between 2 and 6 billion years after the big bang, an important time period when most of the stars in the universe were formed. Some of these galaxies are undergoing starbursts, creating huge numbers of stars, researchers have found

Studying this early epoch of the universe's history is critical to fully understanding how these stars formed and how galaxies have grown and evolved 2 billion to 6 billion years after the beginning of the universe, the team say.

The finding is the result of a decade-long investigation into whether there is a link between a galaxy's mass and its star-forming activity, and helps paint a consistent picture of events in the early universe.

'We already suspected these kinds of galaxies would contribute to the early wave of star formation, but this is the first time we've been able to measure the effect they actually had,' said Hakim Atek of the École Polytechnique Fédérale de Lausanne (EPFL) in Switzerland, lead author of the study published in The Astrophysical Journal.

'They appear to have had a surprisingly huge role to play.'

Previous studies of star-forming galaxies were restricted to the analysis of mid- or high-mass galaxies, leaving out the numerous dwarf galaxies that existed in this era of prolific star formation.

Astronomers conducted a recent study using data from Hubble's Wide Field Camera 3 (WFC3) to take a further and significant step forward in understanding this formative era by examining a sample of starburst galaxies in the young universe.

Starburst galaxies form stars at a furiously fast rate, far above what is considered by experts to be a normal rate of star formation.

The Large Magellanic Cloud, which closely orbits the Milky Way and contains over 30 billion stars, is sometimes classified as a dwarf galaxy, although others consider it a full-fledged galaxy.

The infrared capabilities of WFC3 have allowed astronomers to finally calculate how much these low-mass dwarf galaxies contributed to the star population in our universe.

'These galaxies are forming stars so quickly that they could actually double their entire mass of stars in only 150 million years — an incredibly short astronomical timescale,' added co-author Jean-Paul Kneib, also of EPFL.

Researchers say such a mass gain would take most normal galaxies 1 billion to 3 billion years to accomplish.

In addition to adding new insight to how and where the stars in our universe formed, this finding may also help to unravel the secrets of galactic evolution.

Galaxies evolve through a jumble of complex processes.

As galaxies merge, they are consumed by newly formed stars that feed on their combined gases, and exploding stars and supermassive black holes emit galactic material — a process that depletes the mass of a galaxy.

It is unusual to find a galaxy in a state of starburst, which suggests to researchers that starburst galaxies are the result of an unusual incident in the past, such as a violent merger.