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Jupiter’s Great Red Spot heats planet’s upper atmosphere

Astronomers from Boston University have discovered that Jupiter’s Great Red Spot (GRS) may provide the mysterious source of energy required to heat the planet’s upper atmosphere to the unusually high values observed. Heating in Jupiter’s atmosphere 500 miles above the GRS is thought to be caused by gravity waves and acoustic waves creating turbulent atmospheric flows.

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Hubble captures vivid aurorae in Jupiter’s atmosphere

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.

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Martian surface revealed in unprecedented detail

The surface of Mars — including the location of Beagle-2 — has been shown in unprecedented detail by University College London scientists using a revolutionary image stacking and matching technique. The UCL researchers used the Super-Resolution Restoration (SRR) process to reveal objects at a resolution up to five times greater than previously achieved.

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How big can a black hole grow?

Black holes at the heart of galaxies could swell to 50 billion times the mass of the Sun before losing the discs of gas they rely on to sustain themselves, according to research conducted by Professor Andrew King from the University of Leicester’s Department of Physics and Astronomy.

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NASA’s Swift spots its thousandth gamma-ray burst

NASA’s Swift spacecraft has detected its 1,000th gamma-ray burst (GRB). A GRB is a fleeting blast of high-energy light, often lasting a minute or less, occurring somewhere in the sky every couple of days. GRBs are the most powerful explosions in the universe, typically associated with the collapse of a massive star and the birth of a black hole.

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Scientists solve age-old planetary ring riddle

An international team of scientists has solved an age-old scientific riddle by discovering that planetary rings, such as those orbiting Saturn, have a universally similar particle distribution. The study also suggests that Saturn’s rings are essentially in a steady state that does not depend on their history.