Comet storm rages in Eta Corvi

NASA’s Spitzer Space Telescope has detected evidence of icy bodies raining down in an alien solar system. 

As Carey Lisse, senior research scientist at the Johns Hopkins University Applied Physics Laboratory points out, the downpour closely resembles our own solar system several billion years ago during a period known as the “Late Heavy Bombardment,” which is thought to have brought water and other life-forming ingredients to Earth.

During this epoch, comets and other frosty objects flung from the outer solar system pummeled the inner planets, scarring our moon and producing large amounts of dust.

Now Spitzer has spotted a band of dust around a nearby bright star in the northern sky known as Eta Corvi which strongly matches the contents of an obliterated giant comet. 

The dust is located close enough to Eta Corvi that Earth-like worlds could exist, suggesting a collision occured between a planet and one or more comets. The Eta Corvi system is approximately one billion years old, which researchers think is about the right age for such a hailstorm.

“We believe we have direct evidence for an ongoing Late Heavy Bombardment in the nearby star system Eta Corvi, occurring about the same time as in our solar system,” said Lisse.

Indeed, astronomers used Spitzer’s infrared detectors to analyze the light coming from the dust around Eta Corvi. Certain key chemical fingerprints were observed, including water ice, organics and rock, all of which indicate a giant comet source.

The light signature emitted by the dust around Eta Corvi also resembles the Almahata Sitta meteorite, which fell to Earth in fragments across Sudan in 2008. The similarities between the meteorite and the object obliterated in Eta Corvi imply a common birthplace in their respective solar systems.

A second, more massive ring of colder dust located at the far edge of the Eta Corvi system appears to be a “proper” environment for a reservoir of cometary bodies. 

This bright ring, discovered by astronomers in 2005, looms at approximately 150 times the distance from Eta Corvi as the Earth is from the sun.

Our solar system has a similar region, known as the Kuiper Belt, where icy and rocky leftovers from planet formation linger. Interestingly enough, the new Spitzer data suggests the Almahata Sitta meteorite may have originated in our own Kuiper Belt.

The Kuiper Belt was home to a vastly greater number of these frozen bodies, collectively dubbed Kuiper Belt objects. About 4 billion years ago – some 600 million years after our solar system formed – the Kuiper Belt was likely disturbed by a migration of the gas-giant planets Jupiter and Saturn. 

This jarring shift in the solar system’s gravitational balance scattered the icy bodies in the Kuiper Belt, flinging the vast majority into interstellar space and producing cold dust in the belt. Some Kuiper Belt objects, however, were set on paths that crossed the orbits of the inner planets.

The resulting bombardment of comets lasted until 3.8 billion years ago. After comets impacted the side of the moon that faces Earth, magma seeped out of the lunar crust, eventually cooling into dark “seas,” or maria. When viewed against the lighter surrounding areas of the lunar surface, those seas form the distinctive “Man in the Moon” visage. 

Comets also struck Earth or incinerated in the atmosphere, and are thought to have deposited water and carbon on our planet. This period of impacts might have helped life form by delivering its crucial ingredients.

“[As such], we think the Eta Corvi system should be studied in detail to learn more about the rain of impacting comets and other objects that may have started life on our own planet,” Lisse added.