Every 27.5 million years, the Earth’s heart beats catastrophically - Big Think

Geologists discover a rhythm to major geologic events.

Now, a study in the journal Geoscience Frontiers finds that Earth itself has a pulse, with one "beat" every 27.5 million years.

But our study provides statistical evidence for a common cycle, suggesting that these geologic events are correlated and not random.".

The authors of the study collected the latest, best dating for 89 known geologic events over the last 260 million years:.

Putting all the events together, the scientists performed a series of statistical analyses that revealed that events tend to cluster around 10 different dates, with peak activity occurring every 27.5 million years.

"The correlations and cyclicity seen in the geologic episodes may be entirely a function of global internal Earth dynamics affecting global tectonics and climate, but similar cycles in the Earth's orbit in the Solar System and in the Galaxy might be pacing these events.

The last occurred some seven million years ago, meaning the next won't happen for about another 20 million years.

A recent expedition off the coast of Java discovered a new isopod species remarkable for its size and resemblance to Darth Vader.

It is one of several known species of giant ocean-going isopod.

The incredible size of this species is likely a result of deep-sea gigantism.

This is the tendency for creatures that inhabit deeper parts of the ocean to be much larger than closely related species that live in shallower waters.

The discovery of a new species is always a cause for celebration in zoology.

Researchers discovered a galactic wind from a supermassive black hole that sheds light on the evolution of galaxies.

A galactic wind driven by a supermassive black hole located in the center of a galaxy (artist's impression).

An enormously powerful galactic wind generated by a supermassive black hole 13.1 billions years ago has been discovered by researchers.

This is the earliest example of this type of wind yet spotted that underscores the role of black holes in the formation of galaxies.

In previous studies, scientists have noticed an unexpected proportional relationship between the mass of a supermassive black hole at the center of a large galaxy, which can grow up to billions of times more massive than the sun, and the mass of the galaxy's central area (known as a "bulge").

The proportionality of the masses is especially unusual considering that galaxies and black holes are so different in size, with the bulge generally being orders of magnitude larger?

This led the researchers to conclude that galaxies and black holes developed together through coevolution, which involved some physical interaction courtesy of the galactic wind

As ALMA's press release explains, a galactic wind starts coming into existence when a supermassive black hole gobbles up giant quantities of matter

It is then moved at such a high speed by the black hole's gravity that it radiates intense energy, which in turn, pushes surrounding matter away, creating the galactic wind

Takuma Izumi, the paper's lead author and a researcher at the National Astronomical Observatory of Japan (NAOJ), says an important question is: "When did galactic winds come into existence in the universe?" Finding this out can lead to understanding how galaxies and supermassive black holes coevolved

The researchers used NAOJ's Subaru Telescope to locate over 100 galaxies that existed more than 13 billion years ago that featured supermassive black holes

This allowed the scientists to detect the presence of an intense galactic wind that rushes forth from the supermassive black hole at about 1,118,468 miles per hour (500 km/second)

Interestingly, the mass of the bulge in J1243+0100 was found to be about 30 billion times larger than that of the sun, while the mass of the galaxy's supermassive black hole was estimated to be about 1 percent of that

This ratio is essentially the same as the mass ratio of black holes to galaxies in today's universe

To the scientists, this demonstrates how essential black holes are in affecting the growth of galaxies, supporting the notion of coevolution from the early period of the universe