The drizzle of stars scattered across this image forms an irregular dwarf galaxy known as UGC 4879. Some 2.3 million light-years from its closest neighbour, UGC 4879’s isolation means that it has not interacted with any surrounding galaxies, making it an ideal laboratory for astronomers looking to understand the complex mysteries of starbirth throughout the universe.
In this image from ESO’s Very Large Telescope (VLT), light from blazing blue stars energises the gas left over from the stars’ recent formation. The result is a strikingly colourful emission nebula, called LHA 120-N55, in which the stars are adorned with a mantle of glowing gas. LHA 120-N55 lies within the Large Magellanic Cloud, a satellite galaxy of the Milky Way.
An international team of scientists has detected and confirmed the faintest early-universe galaxy ever using the ten-metre Keck II telescope on the summit on Maunakea, Hawaii. The team analysed three separate images of the object gravitationally lensed by a foreground galaxy cluster, revealing the distant galaxy as it was 13 billion years ago.
Astronomers recently found that a galaxy about 30 million light-years away nicknamed Leoncino, or “little lion,” contains the lowest level of heavy chemical elements, or “metals,” ever observed in a gravitationally bound system of stars. The elemental make-up of metal-poor galaxies is very close to that of the early universe.
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.
Using the Atacama Large Millimetre/submillimetre Array (ALMA), a team of astronomers has delved remarkably deep into the heart of a nearby elliptical galaxy to study the motion of a disc of gas encircling the supermassive black hole at its centre. These observations provide one of the most accurate mass measurements to date for a black hole outside of our galaxy.
Astronomers have discovered three planets orbiting an ultra-cool dwarf star just 40 light-years from Earth. These worlds have sizes and temperatures similar to those of Venus and Earth and are the best targets found so far for the search for life outside the solar system. They are the first planets ever discovered around such a tiny and dim star.
Two black holes in nearby galaxies have been observed in X-rays by ESA’s XMM-Newton space observatory devouring their companion stars at a rate exceeding classically understood limits, and in the process, kicking out matter into surrounding space at astonishing speeds of around a quarter the speed of light.
Now that scientists have confirmed the existence of gravitational waves, a NASA team using a balloon-borne observatory is set to search for a predicted signature of primordial gravitational waves that would prove the infant universe expanded far faster than the speed of light and began growing exponentially almost instantaneously after the Big Bang.
This NASA/ESA Hubble Space Telescope image reveals the simple beauty of NGC 339, a 6.5-billion-year-old massive intermediate age star cluster that lies in the SMC, a dwarf galaxy some 200,000 light-years away from us. The relationship between such clusters and true globular clusters is not yet fully understood.
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