Supernova remnant DEM L316A lies in the Large Magellanic Cloud some 160,000 light-years away in the far southern constellation of Dorado. Image credit: ESA/Hubble & NASA, Y. Chu.This NASA/ESA Hubble Space Telescope image captures the remnants of a long-dead star. These rippling wisps of ionised gas, named DEM L316A, are located some 160,000 light-years away within one of the Milky Way’s closest galactic neighbours — the Large Magellanic Cloud (LMC).
The explosion that formed DEM L316A was an example of an especially energetic and bright variety of supernova, known as a Type Ia. Such supernova events are thought to occur when a white dwarf star steals more material than it can handle from a nearby companion, and becomes unbalanced. The result is a spectacular release of energy in the form of a bright, violent explosion, which ejects the star’s outer layers into the surrounding space at immense speeds. As this expelled gas travels through the interstellar material, it heats it up and ionises it, producing the faint glow that Hubble’s Wide Field Camera 3 captured above.An image of the Large Magellanic Cloud captured with a DSLR and 85mm f/1.4 lens from New Zealand on 10 December 2015. Image credit: Ade Ashford.The LMC orbits the Milky Way as a satellite galaxy and is the fourth largest in our group of galaxies, the Local Group. DEM L316A is not alone in the LMC; Hubble came across another one in 2010 with SNR 0509, and in 2013 it snapped SNR 0519.
Discovered in 1779, M61 serves as a brilliant subject for ground- and space-based telescopes alike, with spiral arms bursting with young stars and a luminous core harboring a supermassive black hole.
Gravity, one of the four fundamental forces of nature, appears reassuringly constant across the universe, according to a decades-long study of a distant pulsar. This research helps to answer a long-standing question in cosmology: Is the force of gravity the same everywhere and at all times? The answer, so far, appears to be yes.
At the centre of this beautiful NASA/ESA Hubble Space Telescope image is a Wolf–Rayet star known as WR 31a, located about 30,000 light-years away in the southern constellation of Carina. The distinctive blue bubble is a Wolf–Rayet nebula — an interstellar cloud of dust, hydrogen, helium and other gases expanding at a rate of around 137,000 miles per hour.
