What fascinated Kenneth Wong about astronomy as an undergraduate was that despite its grand scale, “physics is the same on Earth as it is out there. So a lot of the principles you learn in the classroom, you apply them, and they work on large scales also.”
Today, Wong, 36, exploits one such principle on the largest possible scale: Just as a lens can bring to a point light coming from across a classroom, the gravitational pull of a galaxy cluster can focus light across billions of light-years, producing multiple images of a single distant object on the sky. By using these cosmic gravitational lenses to measure how quickly the universe is expanding, Wong and his colleagues at the H0LiCOW collaboration are working on one of the most intriguing mysteries in cosmology.
The heart of the problem is a number known as the Hubble constant (H0 ), a measure of the universe’s rate of expansion. Thanks to the European Space Agency’s Planck satellite, which observed the cosmic microwave background radiation left by the Big Bang, scientists know that under prevailing cosmological theory, H0 = 67.4 kilometers per second per megaparsec.
But in 2016, a different team studying type I supernovae in distant galaxies found that H0 is significantly higher, between 71.5 and 75 km/s/Mpc. “This actually points to something going on,” says Wong. If their methods are sound, then perhaps our entire prevailing cosmological theory is wrong.
