When future historians look back at the beginning of the 21st century, they’ll note that we grappled with many big issues.
They’ll write about the battle between nationalism and globalism, soaring global debt, a dysfunctional healthcare system, societal concerns around automation and AI, and pushback on immigration. They will also note the growing number of populist leaders in Western democracies, ranging from Marine Le Pen to Donald Trump.
However, these historians will not view these ideas and events in isolation. Instead, they will link them all, at least partially, to an overarching trend that is intimately connected to today’s biggest problems: the “hollowing out” of the middle class.
VISUALIZING THE COLLAPSE OF THE MIDDLE CLASS
The fact is many people have less money in their pockets – and understandably, this has motivated people to take action against the status quo.
And while the collapse of the middle class and income inequality are issues that receive a fair share of discussion, we thought that this particular animation from Metrocosm helped to put things in perspective.
The following animation shows the change in income distribution in 20 major U.S. cities between 1970 and 2015:
The differences between 1970 and 2015 are intense. At first, each distribution is more bell-shaped, with the majority of people in a middle income bracket – and by 2015, those people are “pushed” out towards the extremes as they either get richer or poorer.
A BROADER LOOK AT INCOME INEQUALITY
This phenomenon is not limited to major cities, either.
Here’s another look at the change in income distribution using smaller brackets and the whole U.S. adult population:
Courtesy of: FT (h/t Metrocosm)
It’s a particularly challenging issue, because while a significant portion of middle class households are being shifted into lower income territory, there are also many households that are doing the opposite. According to Pew Research, the percentage of households in the upper income bracket has grown from 14% to 21% between 1971 and 2015.
