The age of the universe is crucial because it affects our understanding of physics and the standard model. A discrepancy in measurements could indicate missing elements in our current understanding, potentially leading to new discoveries.
The Hubble constant measures the rate of expansion of the universe. It is significant because it allows scientists to calculate the age and size of the universe, which is fundamental to cosmology.
The universe's expansion involves space itself expanding, not objects expanding into something else. Unlike everyday experiences, space is being created as the universe expands.
A discrepancy could mean there is something wrong with our standard model of physics, potentially pointing to missing elements or new fundamental physics that we haven't discovered yet.
JWST has allowed for more accurate measurements of the Hubble constant due to its larger mirror, better resolution, and higher sensitivity. These improvements bring us closer to resolving the discrepancy between different measurement methods.
Challenges include accounting for dust, resolving crowded stars, and ensuring the accuracy of distance measurements. These factors can affect the precision of the Hubble constant calculations.
Cepheid variable stars are used as distance indicators because their brightness correlates with their pulsation period. This allows astronomers to measure distances to galaxies and calculate the Hubble constant.
Dark energy is a form of energy causing the universe to expand at an accelerating rate. It is a mystery because there is no physical explanation for it, and its properties are not well understood.
The cosmic microwave background provides information about the early universe. By studying its properties, scientists can estimate the age of the universe, which is currently calculated to be 13.8 billion years.
Resolving the Hubble tension could either confirm the standard model of physics or reveal missing elements, leading to new discoveries and a better understanding of the universe's composition and behavior.
How old is the universe—and how fast is it expanding? These are part of one of the biggest—and most contested—questions in science, and the answers could change our understanding of physics.
In this episode, we talk with renowned UChicago astronomer Wendy Freedman, who’s spent decades trying to solve these very questions. There are two ways to measure how fast the universe is expanding, also known as the Hubble constant; Freedman has done groundbreaking research to calculate this number using stars, but the problem is, her numbers don’t match up with scientists using a different method. And the implications of that difference are massive, because it could indicate that our Standard Model of physics could be broken.
Yet Freedman’s latest research, using the powerful James Webb Space Telescope, might finally give us a clearer answer. In our conversation, we explore the age of the universe, the mysteries of dark matter and what all this could mean for the future of physics—and maybe even the discovery of life beyond Earth.