Long streamers of gas glow in the Large Magellanic cloud, remnants of a supernova blast that destroyed a white dwarf in a Type 1a supernova. Its remnants are known as SNR 0454-67.2. Such explosions occur when a white dwarf sucks in enough material from a companion star to reach a critical mass, triggering a catastrophic core collapse, rebound and shock wave that blows the star apart. Its remnants are blasted into the surrounding space, including heavy elements that were cooked up in the detonation. Because Type 1a supernovas all occur in the same fashion, they shine with a known brightness, or luminosity, that can be used to determine their distance. Such supernovae are known as “standard candles” and they are critical to modern cosmology, helping astronomers measure changes in the acceleration of the universe’s expansion due to dark energy.
Astronomers are using the NASA/ESA Hubble Space Telescope to study aurorae — stunning light shows in a planet’s atmosphere — on the poles of the largest planet in the solar system, Jupiter. This observation program is supported by measurements made by NASA’s Juno spacecraft, shortly to arrive at the gas giant.
Astronomers at Swinburne University of Technology, Melbourne, have discovered an unusually shaped structure in two nearby disc galaxies. The Swinburne team recently developed new imaging software, making it possible to observe the double “peanut shell shape” formed by the distribution of stars bulging from the centres of these galaxies.
A team of international scientists, led by astronomers from Cardiff University, has shown for the first time that galaxies can change their structure over the course of their lifetime. The researchers have shown that a large proportion of galaxies have undergone a major ‘metamorphosis’ since they were initially formed after the Big Bang.