The universe is expanding faster than it should

It’s one of the biggest puzzles in modern astronomy: Based on multiple observations of stars and galaxies, the universe seems to be flying apart faster than our best models of the cosmos predict it should. Evidence of this conundrum has been accumulating for years, causing some researchers to call it a looming crisis in cosmology.

Now a group of researchers using the Hubble Space Telescope has compiled a massive new dataset, and they’ve found a-million-to-one odds that the discrepancy is a statistical fluke. In other words, it’s looking even more likely that there’s some fundamental ingredient of the cosmos—or some unexpected effect of the known ingredients—that astronomers have yet to pin down.

“The universe seems to throw a lot of surprises at us, and that’s a good thing, because it helps us learn,” says Adam Riess, an astronomer at Johns Hopkins University who led the latest effort to test the anomaly.

The conundrum is known as the Hubble tension, after astronomer Edwin Hubble. In 1929 he observed that the farther a galaxy is from us, the faster it recedes—an observation that helped pave the way toward our current notion of the universe starting with the big bang and expanding ever since.

Researchers have tried to measure the universe’s current rate of expansion in two primary ways: by measuring distances to nearby stars, and by mapping a faint glow dating back to the infant universe. These dual approaches provide a way to test our understanding of the universe across more than 13 billion years of cosmic history. The research has also uncovered some key cosmic ingredients, such as “dark energy,” the mysterious force thought to be driving the universe’s accelerating expansion.

But these two methods disagree on the universe’s current expansion rate by about 8 percent. That difference might not sound like much, but if this discrepancy is real, it means the universe is now expanding faster than even dark energy can explain—implying some breakdown in our accounting of the cosmos.

The Hubble tension comes from attempts to measure or predict the universe’s current rate of expansion, which is called the Hubble constant. Using it, astronomers can estimate the age of the universe since the big bang.

One way of getting the Hubble constant relies on the cosmic microwave background (CMB), a faint glow that formed when the universe was just 380,000 years old. Telescopes such as the European Space Agency’s Planck observatory have measured the CMB, providing a detailed snapshot of how matter and energy were distributed in the early universe, as well as the physics that governed them.

Using a model that predicts many of the universe’s properties with spectacular success—known as the Lambda Cold Dark Matter model—cosmologists can mathematically fast-forward the infant universe as seen in the CMB and predict what today’s Hubble constant should be. This method predicts that the universe should be expanding at a rate of about 67.36 kilometers per second per megaparsec (a megaparsec equals 3.26 million light-years).

By contrast, other teams measure the Hubble constant by looking at the “local” universe: the more modern stars and galaxies that are relatively close to us. This version of the calculation requires two kinds of data: how quickly a galaxy is receding from us, and how far away that galaxy is. That in turn requires astronomers to develop what’s known as a cosmic distance ladder.

The new studies’ cosmic distance ladder, assembled by Riess’s research group SH0ES, starts with measurements of the distances between us and certain kinds of stars called Cepheid variables. Cepheids are valuable because in essence they act as strobe lights of known wattage: They brighten and dim regularly, and the brighter the Cepheids, the more slowly they pulsate. Using this principle, astronomers can estimate the intrinsic brightnesses of even more distant Cepheids based on their pulsation rates and ultimately calculate the stars’ distances from us.

To extend the ladder even farther, astronomers have added rungs based on stellar explosions called type 1a supernovae. By studying galaxies that host both Cepheids and type 1a supernovae, astronomers can work out the relationship between the supernovae’s brightnesses and their distances. And because type 1a supernovae are much brighter than Cepheids, they can be seen at much greater distances, letting astronomers extend their measurements to galaxies deeper in the cosmos.

National Geographic