Australian astronomers have combined all observations of supernovae ever made to determine that the strength of gravity has remained unchanged over the last nine billion years. Newton’s gravitational constant, known as G, describes the attractive force between two objects, together with the separation between them and their masses. It has been previously suggested that G could have been slowly changing over the 13.8 billion years since the Big Bang. But researchers have now analyzed the light given off by 580 supernova explosions in the nearby and far Universe and have shown that the strength of gravity has not changed.
Newton’s gravitational constant, known as G, describes the attractive force between two objects, together with the separation between them and their masses. It has been previously suggested that G could have been slowly changing over the 13.8 billion years since the Big Bang.
If G has been decreasing over time, for example, this would mean that Earth’s distance to the Sun was slightly larger in the past, meaning that we would experience longer seasons now compared to much earlier points in Earth’s history.
But researchers at Swinburne University of Technology in Melbourne have now analysed the light given off by 580 supernova explosions in the nearby and far Universe and have shown that the strength of gravity has not changed.
“Looking back in cosmic time to find out how the laws of physics may have changed is not new” Swinburne Professor Jeremy Mould said. “But supernova cosmology now allows us to do this with gravity.”
A Type 1a supernova marks the violent death of a star called a white dwarf, which is as massive as our Sun but packed into a ball the size of our Earth.
Our telescopes can detect the light from this explosion and use its brightness as a ‘standard candle’ to measure distances in the Universe, a tool that helped Australian astronomer Professor Brian Schmidt in his 2011 Nobel Prize winning work, discovering the mysterious force Dark Energy.
Professor Mould and his PhD student Syed Uddin at the Swinburne Centre for Astrophysics and Supercomputing and the ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) assumed that these supernova explosions happen when a white dwarf reaches a critical mass or after colliding with other stars to ‘tip it over the edge’.
“This critical mass depends on Newton’s gravitational constant G and allows us to monitor it over billions of years of cosmic time — instead of only decades, as was the case in previous studies,” Professor Mould said.
Despite these vastly different time spans, their results agree with findings from the Lunar Laser Ranging Experiment that has been measuring the distance between Earth and the Moon since NASA’s Apollo missions in the 1960s and has been able to monitor possible variations in G at very high precision.
“Our cosmological analysis complements experimental efforts to describe and constrain the laws of physics in a new way and over cosmic time.” Mr Uddin said.
In their current publication, the Swinburne researchers were able to set an upper limit on the change in Newton’s gravitational constant of 1 part in 10 billion per year over the past nine billion years.
Reference: Jeremy Mould, Syed A. Uddin. Constraining a possible variation of G with Type Ia supernovae. Publications of the Astronomical Society of Australia, 2014; (accepted)