Scientists at the University of Sheffield have been working with HiPERCAM, a high-speed, multicolor camera, which is capable of taking more than 1,000 images per second, allowing experts to measure both the mass and the radius of a cool subdwarf star for the first time.

For the first time scientists have been able to prove a decades old theory on stars thanks to a revolutionary high-speed camera. (Artist's impression of a binary star. Credit: Mark Garlick)

The findings have allowed researchers to verify the commonly used stellar structure model — which describes the internal structure of a star in detail — and make detailed predictions about the brightness, the color and its future evolution.

Scientists know that old stars have fewer metals than young stars, but the effects of this on the structure of stars was, until now, untested. Old stars (often referred to as cool subdwarf stars) are faint and there are few in the solar neighborhood. Up until now scientists have not had a camera powerful enough to be able to get precise measurements of their stellar parameters, such as the mass and the radius.

HiPERCAM can take one picture every millisecond as opposed to a normal camera on a large telescope which usually captures only one picture every few minutes. This has given scientists the ability to measure the star accurately for the first time. The researchers have been able to measure the size of the star to confirm it is in line with stellar structure theory. They say that these results would not have been possible with any other telescope. They have not only proved the stellar structure theory, but have also verified the potential of HiPERCAM.

HiPERCAM is mounted on the Gran Telescopio Canarias (GTC) — the world's largest optical telescope, with a 10.4-meter mirror diameter. The camera can take high-speed images of objects in the universe, allowing their rapid brightness variations — due to phenomena such as eclipses and explosions — to be studied in unprecedented detail. Data captured by the camera, taken in five different colors simultaneously, allow scientists to study the remnants of dead stars such as white dwarfs, neutron stars and black holes. The GTC is based on the island of La Palma, situated 2,500 meters above sea level, which is one of the best places in the world to study the night sky.

For more information, contact Emma Griffiths at This email address is being protected from spambots. You need JavaScript enabled to view it..


Photonics & Imaging Technology Magazine

This article first appeared in the July, 2019 issue of Photonics & Imaging Technology Magazine.

Read more articles from this issue here.

Read more articles from the archives here.