When Did the Universe Flood With Water?

By studying ancient molecular clouds in our galaxy, astronomers have revealed that the universe's reservoir of water likely appeared much earlier than thought -- only a billion years after the Big Bang.

By studying ancient molecular clouds in our galaxy, astronomers have revealed that the universe's reservoir of water likely appeared much earlier than thought - only a billion years after the Big Bang.

The challenge facing water formation, a molecule composed of two hydrogen atoms and an oxygen atom, is that any element heavier than helium had to have been formed in the cores of stars and not by the Big Bang itself.

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The earliest stars would have taken some time to form, mature and die, so elements as heavy as oxygen would have emerged from its furnace through stellar winds and supernovae some time later. With this delay in mind, and the time it would have taken for these oxygen atoms to disperse throughout the cosmos and attach to hydrogen, astronomers have long thought that H2O appeared throughout the universe rather late.

But according to new research published in the journal Astrophysical Journal Letters, this may not have been the case. In fact, there was likely an abundance of water only a billion years after the universe was born.

"We looked at the chemistry within young molecular clouds containing a thousand times less oxygen than our sun. To our surprise, we found we can get as much water vapor as we see in our own galaxy," said Avi Loeb, an astrophysicist at the Harvard-Smithsonian Center for Astrophysics (CfA), Mass.

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The first stars to pop into existence around 100 million years after the Big Bang were massive and unstable. They quickly burnt through their supply of hydrogen fuel, exploding as supernovae. These stellar explosions seeded the universe with heavier elements. The result was pockets of gas rich in heavy elements - but "rich" is a matter of perspective; compared with the oxygen content of our modern galaxy, these early gas clouds were very oxygen-poor.

But despite the low levels of oxygen, the environment at that time would have been ideal to "cook up" water molecules. Temperatures of 80 degrees Fahrenheit (300 Kelvin) would have been perfect to combine what oxygen that was available to the abundant hydrogen atoms.

"These temperatures are likely because the universe then was warmer than today and the gas was unable to cool effectively," said co-investigator Shmuel Bialy of Tel Aviv University.

"The glow of the cosmic microwave background was hotter, and gas densities were higher," added Amiel Sternberg, a co-author also from Tel Aviv University.

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However, also during this tumultuous time in our universe's history, the abundance of young stars would have pumped out powerful ultraviolet radiation that would have ripped these newly-formed water molecules apart. But after millions of years of water production, the destructive impact of ultraviolet light would have plateaued and water formation would have continued to accelerate.

This work only focuses on the formation of water in the gas phase and doesn't take into account water ice, which is the water phase that currently dominates our galaxy.

This research is interesting as it seems our universe, even in its first billion years, nurtured a rich environment for H2O production in clouds that were comparatively oxygen poor. This then set the stage for later epochs when later stars began forming planets where water was already present. And now we live in a universe apparently filled with water that just happens to be the key component for life as we know it.

Source: CfA

This Hubble image features dark knots of gas and dust known as "Bok globules," which are dense pockets in larger molecular clouds. Similar islands of material in the early universe could have held as much water vapor as we find in our galaxy today, despite containing a thousand times less oxygen.

In a discovery announced on Sept. 4, 2013, a population of planetary nebulae near the galactic core appear to be, weirdly, preferentially aligned to the Milky Way's galactic plain. The nebulae, known as "bipolar" (or "butterfly") planetary nebulae are completely non-interacting and of various ages, suggesting some external force is shaping their orientation. It's thought that a powerful magnetic field may be the culprit.

The researchers used observations from the Hubble Space Telescope and ESO's New Technology Telescope, so here are a small selection of some stunning examples of bipolar planetary nebulae as seen through the eye of Hubble. Shown here is the stunning NGC 6302 -- an intricate example of a bipolar planetary nebula's butterfly wings.

Hubble 5: A classically-shaped bipolar (or 'butterfly') planetary nebula.

NGC 6881: A binary star possibly shapes this wonderfully symmetrical nebula.

NGC 5189: A dramatic view of the ribbons of bright material being ejected from a planetary nebula.

PN Hb 12: An 'hourglass'-shaped bipolar planetary nebula.

Hen 3-1475: A planetary nebula in the making.

M2-9: What appears to be twin jet engines is in fact a stunning example of a bipolar planetary nebula.