
science & techESA/Hubble
Big Bang light gets a tiny energy boost passing through galaxy clusters
The cosmic microwave background is the oldest light in the universe, emitted about 14 billion years ago and now seen as faint microwave radiation filling the sky. As these photons travel through galaxy clusters, which contain hot gas of high-energy electrons, they gain a tiny boost of energy. This is the Sunyaev-Zel'dovich effect, first observed over thirty years ago. Detecting it is difficult, but it reveals where massive clusters are and how they are distributed. In this case, Hubble observed the cluster RX J1347.5-1145, about 5 billion light-years away, while the ALMA telescope in Chile measured the microwave signal from it.
Hot electrons in a cluster's gas scatter microwave photons, giving them extra energy. This shifts the cluster's signal in a measurable way, so its size and gas content can be inferred.
The effect lets astronomers weigh and map the most massive structures in the universe using light from the Big Bang. It connects the earliest light with the largest structures we see today.
ESA/Hubble · CC BY 4.0
Image: ESA/Hubble & NASA, T. Kitayama (Toho University, Japan)/ESA/Hubble & NASA
