‘Oumuamua Might Be a Giant Interstellar Hydrogen Iceberg

Ever since ‘Oumuamua was discovered in 2017, the first interstellar object detected in our solar system has been a source of endless intrigue for astronomers. The giant hunk of space rock has an unusual cigar shape, is tumbling end over end, and isn’t easily classified as a comet or an asteroid. The uncertainties about this interstellar interloper have resulted in a proliferation of theories about its provenance and composition. There’s been speculation that it’s a cosmic dust bunny, an alien spaceship, or the remnants of a small planet torn asunder by its host star.

This week, two Yale astrophysicists put forth a new theory arguing that ‘Oumuamua has the makings of an interstellar iceberg. The research, recently published as a preprint and accepted for publication in Astrophysical Journal Letters, traces ‘Oumuamua’s origins to a giant molecular cloud. These ghostly objects are massive stellar nurseries that can stretch for light years and contain enough gas to form tens of thousands of stars. But according to the new research, they might also spit out hydrogen icebergs that look and behave a lot like ‘Oumuamua.

“Even though the hydrogen iceberg thing is a little exotic, it explains every single mysterious thing about ‘Oumuamua,” says Darryl Seligman, an incoming postdoctoral researcher at the University of Chicago who coauthored the paper with astrophysicist Gregory Laughlin, his PhD adviser at Yale. If Seligman and Laughlin are right, ‘Oumuamua would not only be the first interstellar object discovered, but the first hydrogen iceberg, too.

Hydrogen typically exists as a gas and is the stuff that fuels the fusion process in stars like our sun. But if it gets cold enough, hydrogen can solidify. The only known regions of the universe frigid enough to cause this phase transition are the dense, icy hearts of giant molecular clouds. “There’s not much work on hydrogen ice, because its sublimation temperature is so low,” says Seligman, referring to the point at which a solid transitions directly into a gas. He says that hydrogen freezes at around -450 degrees Fahrenheit, just a few degrees above absolute zero.

The core of a giant molecular cloud has a relatively short lifespan of just a few hundred thousand years. Over time, it gets eroded by the churn of the galaxy until it disappears. But according to the hydrogen iceberg theory, during the core’s brief existence, frozen hydrogen molecules latch on to dust in the cloud to build up a large block of ice. It’s a painstakingly slow process; after a few hundred thousand years it would produce an iceberg only a few hundred of meters across. This is squarely in the ballpark for an object like ‘Oumuamua, which NASA researchers calculated to be less than 800 meters long.

The iceberg theory can also explain ‘Oumuamua’s weird cigar shape. After the core of the giant molecular cloud dissipates and the iceberg is set adrift in the void, it is constantly bombarded by cosmic radiation. The radiation would chip away at the iceberg from some directions more than others, which would result in a more elongated form. Seligman compares it to a bar of soap, which becomes more flat and oval as it is used.

But the reason Seligman is most excited about the hydrogen iceberg theory is because it can explain why ‘Oumuamua began speeding up as it entered the solar system, which couldn’t be explained by the tug of gravity alone. A leading theory advanced by several different astronomers argued that ‘Oumuamua was propelled by gases rapidly boiling off of space rocks, a phenomenon known as outgassing. This is what gives a comet its brilliant tail, which is typically composed of compounds like carbon dioxide and water. But when astronomers observed ‘Oumuamua, they didn’t detect outgassing that would explain the object’s acceleration—unless, of course, it was spitting out pure hydrogen, which couldn’t be detected by the telescopes conducting the observations.


Author: showrunner